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The Maserati Birdcage 75th is a concept car with extreme lines and performance that aims to achieve maximum impact on the public's imagination.
It is a futuristic extension of the Maserati brand which glorifies and reinforces the strong heritage of Maserati design.
A visionary project and the technological synthesis of three large companies: Pininfarina, Maserati and Motorola.
With the Birdcage 75th, Pininfarina returns to the idea of the pure dream car, the synthesis of a vision that combines exclusive design, sporty DNA and technological innovation.
The Birdcage 75th is a hi-tech sculpture in movement, which evokes an imaginary but possible future, paying tribute to the strong, distinctive characteristics of the Trident brand.
The concept car is based on the racing chassis of the Maserati MC12, the ultimate expression of speed, sensuality and elegance. The contrast between the organic fluidity of the aerodynamics and the stringent tension of the engineering creates a unique dynamism rarely seen before.
The central cell is divided into two parts: a transparent upper part and a lower part that acts as a structural aerodynamic sideskirt. The generous upper surface not only guarantees excellent visibility for its occupants, but also reveals the Maserati engineering so that it can be admired by everyone.
The result is a strong, elegant line which, just one metre high, gives the impression of movement even when it is stationary. The nose culminates in the oval mouth with low horizontal eyes on either side.
The vehicle interior plays an important role in the visual impact and in the historical bond with Maserati. Consistent with the overall concept of the car, the interior is an extension of the body itself, seamlessly incorporated into the carbon fibre chassis.
Two worlds successfully meet at the centre of the car: future-oriented technology by Motorola combined with the pure Maserati genes. The transparent head-up display reveals the car's intelligent heart, updated to reflect its environment and connected to the future. The Birdcage 75th extends the concept of car/user interface by means of a navigator mounted at the centre that allows the driver to navigate through a customised array of functions and menus.
The cameras positioned on the car make it possible to share the driving experience with others, while the images projected by infrared cameras on the transparent head-up display enhance the experience of night-time driving.
The Birdcage 75th is an application of seamless mobility by Motorola. The technologies incorporated into the concept car realise this vision, using payment systems, an iPen and a mobile router, exploiting protection screens for man-machine communication.
To mark the 75th anniversary of its foundation, Pininfarina decided to give free rein to its creative spirit, returning to an extreme sports prototype. This project links up ideally with the Italian Renaissance of car design, which began in the Fifties and continued in the following two decades. It was a period of optimism and unbounded creativity, that produced some of the loveliest and most surprising cars in the world.
The Maserati Birdcage 75th was born with the objective of setting new stylistic and technical frontiers, starting with the Maserati V12 that delivers over 700 bhp, ideally close to the racing car world.
This is combined with unprecedented aerodynamic research and a futuristic design for the interior, which emerges as a real extension of the car itself.
The project also stands out for a strong blend of design and technology, the fruit of joint work by Pininfarina Extra and Motorola. Pininfarina's vision of design takes concrete shape in the application of Motorola's vision of seamless mobility, producing a concept car that is ahead of the field.
The Birdcage 75th project was the fruit of collaboration between Maserati, Pininfarina, Pininfarina Extra and Motorola.
"Louis Vuitton Classic Concept Award" (2006)
"Best Concept" Geneva Motor Show (2005)
"L'automobile più bella del mondo" (2005)
Pininfarina Design and Engineering
Cambiano (Turin)
Pebble Beach Concours d'Elegance 2005
The sports Berlinetta with a great innovative power
A spider for collectors, symbol of the sweet life
2-seater Berlinetta, designed and engineered for competition
A new idea of safety
A car with a futuristic design
A high performance sport car
A very fast 12-cylinder berlinetta
The perfect combination of design, technology and emotions
Technical innovation and high end quality in a production car
an innovative concept car to analyse the safety of small cars
A convertible with a unique three-piece retractable hardtop
The Renaissance of car design made in Pininfarina: the Maserati Birdcage 75th
Two car models for China Signed by Pininfarina the A3 and the A3 sport
A new masterpiece created by Pininfarina
It is time for the Sintesi, the concept car that explores the car of the future.
Pininfarina returns to custom-built vehicle for special customers
The first Maserati convertible, the four-seater GranCabrio was designed by Pininfarina
The 2uettottanta is here, the Alfa Romeo sports car designed by Pininfarina
A dream comes true. The New Stratos takes to the road
A true concentrate of technology, creativity, innovation, style and passion. This is the visiting card of the Ferrari 458 Spider.
Pininfarina designs the new Ferrari FF, the fastest, most versatile four-seater in Ferrari history
22 unique models in Maranello Museum
A luxury electric sports saloon
Innovation and extreme technological research
a new, exclusive concept car
Consummate elegance
The perfect synthesis of innovation and technology
The high-class SUV with an Italian touch
Participation by Fuoriserie
The compact and sporty SUV
The Full Power of Hydrogen
An all carbon fiber supercar like no other
The eco-sustainable luxury sedan styled
The first electric-hydrogen racingcar
The sedan elegant and sporty
Elegant and eco-sustainable Gran Turismo
The most compact SUV ever
The car icon of the Italian joie de vivre
Design and functionality. Performance e look. For the new range of 3M multimedia products
When design plays at home: the new Pininfarina Extra headquarters
An innovative urban lighting device. It is called…
Elegance and essentiality. Ergonomics and functionality
A synthesis of innovation, technology, beauty and experimentation in a kitchen
The new Lange ski boot that offers the best technological innovation and design features
As high as a 20 floor building, it generates a 4 meter flame
The Torch for the 2006 Turin Olympics and Paralympics was designed, engineered and manufactured by Pininfarina
Designing a new space for the soul: the Pininfarina Gorenje Black Collection
A metal inner part inserted in a body made of transparent plastic and rubber
A formal and aesthetic sobriety transmitting balance and lightness for the innovative monitor LCD
The innovative steam shower with hydromassage
The ideal collection of office furniture
Pininfarina enters the residential design field with the Torre México project
With the Keating Hotel, Pininfarina enters the hospitality world
In the "Insegna" project Pininfarina explores interior architecture
Design that is accessible to all is on display at
The mood of architecture applied to interior design. Pininfarina has imagined and developed it for the
Pininfarina returns to custom-built vehicle for special customers
It is electric. It does not pollute and it makes no noise. And features the best technological innovations. It is the BLUECAR, conceived and designed by Pininfarina.
Pininfarina teams up with Aero Toy Store: design takes flight.
The Beast appears on the snow, the snow groomer designed by Pininfarina
the notebook designed by Pininfarina
The new Cardio-Fitness Line
The designer drinks dispenser: Coca-Cola Freestyle
Pininfarina and Amaro Ramazzotti: design to drink


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The presence of tight end Rob Gronkowski on the field during the portion of Monday's practice open to the media generated a flurry of tweets and reports indicating Gronkowski, whose most recent surgery was on his back, may soon be ready to play.
For coach Bill Belichick it was no big deal.
"He's been out there every day," Belichick told reporters on Tuesday. "He hasn't missed a day of camp."
That answer prompted from a reporter the one-word verbal equivalent of a spit take: "Gronkowski?"
"He was here the first day of camp," Belichick said. "He's been doing the same thing every day."
Those last four words quickly became the chorus to a song.
Question: "How has he looked recently?"
"He's been doing the same thing every day."
Question: "He's been out there every day?"
"The same thing every day. For those of us who have been here, it's been the same thing every day."
Question: "He was out in view of the media yesterday."
"Same thing every day."
Earlier in the press conference, Belichick was asked in general terms the question he'll face come Saturday when the time comes to put Gronkowski on the active roster or shut him down for at least six weeks by leaving him on the PUP list: What happens if the player otherwise destined for the PUP list would miss only the first two or three games?
"Every decision we make on a player comes down to two things really: What's best for the player and what's best for the team. When those are the same, it's easy. When they're not, something has to give and you have to make a call one way or the other. That's the way it is with everything."
It's unclear how Belichick will resolve that issue with Gronkowski. Until then, Gronkowski presumably will do the same thing every day.


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As the District prepares for the XIX International AIDS Conference, aka AIDS 2012, locals are preparing a smaller gathering for the days just prior. And, though smaller, this Gay Men's Health Summit may have even more to say to at least three letters of the LGBT acronym than AIDS 2012. Certainly, gay men's health in this decade goes far beyond one virus – even if HIV has cruelly demanded our attention and our sacrifices for decades.
That's not to say the summit is devoid of HIV/AIDS. One of the roughly 35 workshop/panels, however, sort of puts it in context: "HIV: 30 Years of Fear, Stigma. How to Move Forward." The Gay Men's Health Summit, first held in Boulder, Colo., in 1999, tries to look at gay men as whole individuals, as a community, and at their connections to the rest of the world. This is not health defined as not being sick, but of health as an expression of wellbeing – mind, body and soul.
Christopher Dyer
Christopher Dyer, 42, founder of the Youth Pride Alliance, former director of the Mayor's Office of GLBT Affairs – the man sometimes known to shake his moneymaker for a good cause as drag alter ego Cookie Buffet – is one of the men helping to organize the summit. Others are David Mariner, executive director The DC Center, the city's LGBT community center; Raymond Robbins, also of The DC Center; Blake Cornish and David Phillips. Thanks to them, the Gay Men's Health Summit will make its D.C. debut July 20 and 21, under a simple theme of "Resiliency. Activism. Advocacy."
Metro Weekly takes a look at some of the diverse lineup being readied for these two days community conclave.
First, however, to help get the ball rolling, Dyer offered Metro Weekly some of his own history with health, his sobriety, and the value of self-esteem.
METRO WEEKLY: How has health been part of your career?
CHRISTOPHER DYER: I went to college in Ithaca, N.Y., a history major. I remember getting some sort of HIV training. The thing that stuck out for me was, when you're taking a trick home, or when you're sleeping with someone for the first time, tell them what your status is and ask them what their status is. I wonder if that happens now, 22 years later. That stuck out with me as something very empowering.
MW: Some people might be offended by that today.
DYER: In the 1980s and '90s, when people were still dying in droves, some of the finer points of political correctness kind of went out the window. It was stay alive.
In '99 I got a job with the American Association of Colleges and Universities using HIV and AIDS as a way to teach liberal education. I looked at various curriculums of how colleges and universities used HIV/AIDS as a course and to teach civic engagement.


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Libraries have a lot of different uses, but this was a new one
for us: a wedding celebration. The bride and groom eloped to
Denver from Minneapolis and said their vows in an impromptu
location somewhere in the Museum. Then they found their way to the
Museum's Library where, to their delight, they discovered a book
that hinted at their future together: Osa Johnson's I
Married Adventure.
We invite others to also visit the library and discover their
own literary surprises. Begin your journey with a search in our catalog.
Photos used courtesy of Kristy Rowe, Moodeous Photography.


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PC and Mac versions, now through Friday
There's something about the first-person shooters of the '90s that makes them (some of them) still hold up to this day. I mean, Duke Nukem 3D shouldn't be aesthetically pleasing to me in 2012, but the old sprite-based characters are oddly charming, and these titles tended to move at a pace we don't always get with modern shooters. Plus, they were ridiculous.
Considering that Duke Nukem 3D: Atomic Edition is currently free for PC and Mac on GOG.com, much of that justification was probably unnecessary, but there you go. If you are looking for a way to relive a bit of Duke history, you can't go wrong with this deal.
[Thanks, DV2FOX]
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Express. Home of the Daily and Sunday Express.
Oscar nets late winner in Prague
Oscar saved Chelsea, interim boss Rafael Benitez and striker Fernando Torres from embarrassment with an 82nd-minute winner in the Europa League last 32 first-leg clash at Sparta Prague which ended 1-0.
Torres, a £50million striker now with one goal in 13 games, missed a straightforward effort after 35 minutes and sliced a second-half shot out for a throw-in in another impotent display from last season's Champions League winners at the Generali Arena.
With a stalemate looming and the visiting fans' ire for Benitez and Torres increasing, Oscar came on for Juan Mata and scored with his first involvement, netting neatly following a one-two with Eden Hazard.
After Frank Lampard's early shot from 25 yards was held at the second attempt by Sparta goalkeeper Tomas Vaclik, Hazard twice tried to engineer an opening for Torres, but on each occasion the World Cup winner did not contest good crosses into the six-yard box.
A promising opening from Chelsea, with Marko Marin lively, subsided quickly before an lapse in defence - all too familiar for Benitez of late - nearly presented Sparta with the opening goal after 17 minutes. Right-back Tomas Zapotocny's left-footed diagonal pass over a static defence found David Lafata, who lifted the ball over Petr Cech's goal when he had time to control the ball.
Sparta were finding spaces in and behind the Chelsea defence, but that left them exposed on the counter attack and Chelsea so nearly took advantage after 35 minutes. Marin found Hazard down the left and the Belgian picked out Mata with a cross-field pass. Instead of shooting, Mata teed up his compatriot Torres but his weak toe-poke did not trouble Vaclik.
Lampard shot straight at Vaclik before the break and on the resumption had to make a last-ditch interception to deny Ladislav Krejci a shooting opportunity.
Torres' evening was summed up when he shot right-footed from 20 yards, the ball slicing high and going out for a throw-in.
Mata made way after 82 minutes for Oscar, who had an immediate impact. He injected pace into proceedings and received a return pass from Hazard before clinically netting into the bottom corner.
Torres had an effort saved soon after before Ondrej Svejdik headed over from a corner.


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Burbank officials plan to send a list of qualms they have about a planned NBCUniversal project to the Los Angeles County Board of Supervisors, which is slated to vote on the $1.6-billion project early next year.
NBCUniversal's Evolution project would bring 2.6 million square feet of new studio, retail and hotel development, along with $100 million in roadway and traffic improvements to Los Angeles. While the proposed developments stretch beyond Burbank's borders, city officials maintain the project will impact quality of life for local residents, traffic flow and police operations.
The studio had originally proposed building nearly 3,000 new residential units, but vehement opposition prompted the studio to ditch the housing component and instead double the number of hotel rooms to 1,000.
The scaling back of the Evolution Plan is expected to reduce daily trips to the site by 9,000 — easing potential traffic impacts on Burbank streets — but local officials still aren't totally sold.
The Los Angeles City Council has already approved the project, but since the majority of the proposed development is on county land, the board of supervisors must also sign off on it.
According to the letter being drafted by Burbank, officials don't feel the NBCUniversal proposal addressed the Burbank Police Department's concern that the increase in tourism and commercial activity would also lead to an increase in traffic accidents and crime citywide, while also slowing down public agency response times.
The environmental impact report on the project suggested police use sirens and drive on the wrong side of the road to accelerate response times, which officials felt "disregards the importance" the issue plays in terms of maintaining residents' quality of life.
Officials also felt too much traffic associated with the Evolution project would be spill into residential neighborhoods, prompting requests that the studio fund better traffic protection programs for Media District residents.
The City Council also asked that the studio be required to add transit from the site to Bob Hope Airport, and extend the Los Angeles River bike path from Barham Boulevard and Lankershim Boulevard, which would link to Burbank's own bike infrastructure.
Planning Commission gives OK to NBCUniversal expansion
NBCUniversal scraps plan to build housing on Universal back lot
NBCUniversal cuts about 500 employees
Follow Alene Tchekmedyian on Google+ and on Twitter: @atchek.


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The second round of group matches in the Confederations Cup was anything but tame.
A seven-goal thriller between Italy and Japan threw up drama you'd be pushed to find at the World Cup itself. And Spain's utterly dominant performance with what was widely seen as their 'B' team, still brought only pride to Tahiti, who lost 10-0, showing a side of football rarely seen at international tournaments.
Here are just some of the stunning goals in round two of the Confederations Cup 2013.
3. Diego Forlan vs Nigeria
Diego Forlan may not be the flashiest of players at the tournament, but he's one of the most experienced.
He marked his 100th cap for Uruguay with a fearsome shot that flew past the 'keeper and hit the roof of the net.
The goal took Uruguay into the lead, with the two who were supposed to be the dangerous duo, Cavani & Suarez having to step aside for their elder statesman as he showed the world why he has reached 100 caps.
Watch the goal: https://www.youtube.com/watch?v=G2ns3MQb52E
2. Shinji Kagawa vs Italy
An unbelievable game with seven goals only really yielded one stand-out strike, and that was the goal from Shinji Kagawa to take Japan into a 2-0 lead inside 30mins against four-time world champions Italy.
The Manchester United star slipped seemingly past both Chiellini & Barzagli, swivelled and hit a sweet strike bast Gigi Buffon. The goal stunned the Recife crowd as the rain began to thunder down.
Italy came back to win the thriller, but this goal stood out for me.
Watch the goal: https://www.youtube.com/watch?v=hOKfwz2msTU
1. Neymar vs Mexico
He's back here again. After scoring a simply sensational tournament opener, Neymar struck a technically perfect ball to rip past Corona, who must feel exposed after conceding Pirlo's free-kick in the first game.
Not only was the volley itself brilliant, but to take a ball down from that height and strike it with that much venom is extremely difficult. This goal deserves its place at the top for me.
Watch the goal: https://www.youtube.com/watch?v=1O-1Y5YCzSs
Although Spain beat Tahiti 10-0, there weren't any stand-out goals.
Some notable goals that didn't make the cut:
Jo vs Mexico (Neymar's build up was superb)
Sebastian Giovinco vs Japan (Delicious through ball by De Rossi to get it going)
David Silva vs Tahiti (Great build-up play, albeit against weak defending and finesse shot)
John Obi Mikel vs Uruguay (Nice powerful strike, doesn't score often)
Visit the official 2013 Confederations Cup Facebook page: https://www.facebook.com/fifaconfederationscupbrazil2013
Write for GiveMeSport! Sign-up to the GMS Writing Academy here: https://bit.ly/12evFlH
DISCLAIMER: This article has been written by a member of the GiveMeSport Writing Academy and does not represent the views of GiveMeSport.com or SportsNewMedia. The views and opinions expressed are solely that of the author credited at the top of this article. GiveMeSport.com and SportsNewMedia do not take any responsibility for the content of its contributors.


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Photoshop Hell: The Worst, Most Hilariously Bad Album Covers Of All Time
We've heard the saying "don't judge a book by its cover". But what about albums?
So much investment is put into album packaging and determining how an artist is marketed. That starts with the album cover. Sometimes they're masterpieces that rile up their fans. Other times, they're pauseworthy moments of Photoshop awkwardness that we can't help but laugh at. So with that said, here are the most horrible album covers of all time.
Pooh Man – Funky As I Wanna Be – What in the name of Herpes is going on here? Is she dead or something? Pooh Man is a freak. Clearly.
Tony Tee – Time To Get Physical – Why does he need two burly guys to lift a bar with no weights on it. And what is that chick doing? There's so much awkward going on here.
Lil Wayne – Tha Carter III – What's going on with Weezy here? This was in the height of his crazy drugginess and the album cover is a perfect example. Tatted up babies? And a million people bought this damn thing in its first week.
Big Bear – Doin Thangs – So we're throwing bears on album covers like they're super hood or something? The Ghetto Berenstein Bears look means this should go straight to the trash bin.
Millie Jackson – Back To The Isht – Want to say that rappers are responsible for all the horrible album covers? Look at this old school cover from Millie Jackson. On the toilet? That's a little too much.
Spank Rock and Benny Blanco – Bangers & Cash – So we're just going to throw two chunky chicks in a vat of honey and pretend like they're dimes? They couldn't find other women? Or better names thank Spank Rock? Fail galore!
Continue Slideshow
Top Dog – Slam Dunk'n Hoes – He's just literally slam dunking a hoe. Who would pose for this? Did she think that getting dunked LeBron style into a goal would be her big break? She's probably at K-Mart wondering where it all went wrong.
TA Smallz – Who Killed My Mama – The title alone is enough to make us wonder what could possibly be in store for us. Why on earth would they feel the need to have digital roses? Real roses cost like ten bucks. So…fake roses? Why?!
Various Artists – Christmas N' Memphis – So, this is how Christmas is in Memphis? Crackhead-looking Santas getting held up at gun point? Can we never have Christmas in Memphis? Ever.
DJ Scream Kickstand – Toys, Trees And Snow – Actually, we have no clue what the title or musician is. There are just so many words! Can we just make rappers stay away from Christmas albums for ever and ever?
Wet Black – Errrr. No comment.
Uncle Murda – Murda's Muzik II – Why would anyone want to shoot a care bear? Or photoshop dead Care Bears on album covers? Maybe this is why nobody listens to Uncle Murda? It's karma.
Skillet & Leroy – The Okra Eaters – We think that "okra" might be code for something else. But why would you want to reference a hoo-ha as okra of all things?! That just doesn't make any man want to come anywhere near it. Ewwwww.
Big Shug – Who's Hard – The cover itself is pretty normal. But that title? Is this an album title or a solicitation? You can't be gangsta with a title like that? Sorry Mr. Shug.
Killa Klan – Kill Or Be Killed – Why are there KKK members in the background? Are they supposed to be Black guys in Klan hoodies? Nothing good can come from any of this. Just stop it.
Every No Limit Album Ever – We could donate a whole section to just the crappy No Limit Albums. They were all full of glitter, bright colors and were more gaudy than your aunt's church hat. What was Master P thinking?
Every Cash Money Album – And following in No Limit's footsteps was Cash Money. Their albums looked just as gaudy and embarrassing. Looks like Weezy hasn't changed too much since then.
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ColoradoLawyer needed a new logo design and created a contest on 99designs.
A winner was selected from 50 designs submitted by 12 freelance designers.
Looking for simple, but bold, square logo for legal podcast revealing the tips of winning a Social Security disability claim.
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Definitions of gimlet
n. - A small tool for boring holes. It has a leading screw, a grooved body, and a cross handle. 2
v. t. - To pierce or make with a gimlet. 2
v. t. - To turn round (an anchor) by the stock, with a motion like turning a gimlet. 2
The word "gimlet" uses 6 letters: E G I L M T.
No direct anagrams for gimlet found in this word list.
Words formed by adding one letter before or after gimlet (in bold), or to egilmt in any order:
n - melting s - gimlets
Shorter words found within gimlet:
el elm em emit et gel gelt gem get gie gilt gimel git glim glime it item leg legit lei let li lie lime lit lite me meg mel melt met mi mig mil mile milt mite teg tel ti tie til tile time
List shorter words within gimlet, sorted by length
Words formed from any letters in gimlet, plus an optional blank or existing letter
List all words starting with gimlet, words containing gimlet or words ending with gimlet
All words formed from gimlet by changing one letter
Other words with the same letter pairs: gi im ml le et
Browse words starting with gimlet by next letter
Previous word in list: gimels
Next word in list: gimleted
Some random words: bhakta epoch eft chablis kuchen mirier eerie
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Many of the town's medical facilities were destroyed, including the area's largest hospital
JOPLIN, Mo. (AP) -- Families whose children get some of the best autism services available are scrambling for help after a prominent treatment facility was destroyed in the tornado that ravaged the city of Joplin last month.
The Ozark Center for Autism, which has a national reputation and draws families to the area, offers hands-on, intensive therapy at an early age. The program had recently added a diagnostic team and was slated to expand with services for adults, including vocational training. But the May 22 tornado that pummeled the city, killing more than 150 people and injuring hundreds, demolished the center.
It has relocated to an indoor skate park on the outskirts of town until it can move to another temporary facility closer to its previous location. But fewer families can easily reach the current location, and while Ozark Center staff members have increased their number of home visits, they are concerned that some children could see their progress halted.
"The children will lose some of the skills they've gained if they're not seen immediately," said Paula Baker, chief clinical officer for Freeman Health System, which owns and operates the autism center.
The destroyed Ozark Center included not just the autism school but residential and outpatient psychiatric care and substance abuse treatment units, collectively serving more than 13,000 patients in a four-state region. Baker said that Freeman plans to completely rebuild, and is especially committed to its autism program, which serves a dozen preschool students, four in a new K-12 program and 40 other families receiving in-home care
"Obviously, it's been devastating," Baker said. "But we are committed to rebuilding the program. The tornado will never blow away our commitment to helping these children."
As news of the damage to the Ozark Center spread on Facebook and through word of mouth, pledges of support and financial donations have poured in from across the country. A Kentucky autism center contacted Baker out of the blue. The Cleveland Clinic, which helped get the Joplin facility started, is raising money to help. So are local and regional agencies in Kansas City, Springfield and elsewhere in Missouri.
"It has been exciting to see the autism community rally behind them," said Dayna Busch, a Springfield activist. "Their quick rally is testimony to their determination that these kiddos not fall through the cracks and fall behind."
The center had opened in October 2007 after a local family that had moved to Ohio for treatment opportunities unavailable in southwest Missouri came to the attention of the Cleveland Clinic Center for Autism. The Cleveland Clinic selected Joplin as the first community in the country where it would replicate its model of using what's known as applied behavioral analysis, or ABA treatment.
"They were very committed to starting something in their community," said Aletta Sinot, director of the Cleveland Clinic program. "They were really forward-thinking, and very community-oriented."
The Ozark Center's footprint remains small, but its reputation extends well beyond Joplin.
Jennifer Kirby, the center's clinical director, had worked at well-regarded autism clinics in the Boston area and London before she joined the Joplin site. The Mississippi native said the Ozark Center for Autism it has a reputation as the "gold standard" in autism treatment.
One family commuted more than 100 miles daily from Springfield so their daughter could attend the preschool. The Associated Press interviewed another family in the tornado's immediate aftermath that had moved from Oregon to Joplin just one month earlier to tap into the community's resources. Their phone number has since been disconnected, and the Ozark Center was not aware of their status.
Jennifer Smith and her husband had their choice of job offers and places to live after he completed a medical fellowship last year in Louisville, Ky. They chose Joplin to get their 5-year-old twin sons the autism services. Smith's sons will attend kindergarten in the fall at a Joplin public school, with autism therapists to ease the transition.
"The first priority was to find a place for them to get help," she said. "It's been the right move."
About 50 families remain on the center's waiting list. In March, the center added a diagnostic team consisting of a pediatrician, clinical psychologist, behavior analyst, speech pathologist and pediatric nurse. That team is now without a home until the center's renovated space becomes available, which Baker expects to happen within the next 90 days.
We have everybody we need sitting around that table," she said. "Families were losing a year of precious time just waiting to get a diagnosis."
Shaine Jordan, 30, said he saw almost immediate improvement in the behavior of his 5-year old daughter, Brielle, who is non-verbal. Years of traditional occupational and speech therapy got her "virtually nowhere."
"We do something for years and got nothing," he said "Within three months, my daughter was able to tell me what she wanted."
Alan Scher Zagier can be reached at http://twitter.com/azagier
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Asteroid, also called minor planet or planetoid, any of a host of small bodies, about 1,000 km (600 miles) or less in diameter, that orbit the Sun primarily between the orbits of Mars and Jupiter in a nearly flat ring called the asteroid belt. It is because of their small size and large numbers relative to the major planets that asteroids are also called minor planets. The two designations have been used interchangeably, though the term asteroid is more widely recognized by the general public. Among scientists, those who study individual objects with dynamically interesting orbits or groups of objects with similar orbital characteristics generally use the term minor planet, whereas those who study the physical properties of such objects usually refer to them as asteroids. The distinction between asteroids and meteoroids having the same origin is culturally imposed and is basically one of size. Asteroids that are approximately house-sized (a few tens of metres across) and smaller are often called meteoroids, though the choice may depend somewhat on context—for example, whether they are considered objects orbiting in space (asteroids) or objects having the potential to collide with a planet, natural satellite, or other comparatively large body or with a spacecraft (meteoroids).
Major milestones in asteroid research
Early discoveries
The first asteroid was discovered on January 1, 1801, by the astronomer Giuseppe Piazzi at Palermo, Italy. At first Piazzi thought he had discovered a comet; however, after the orbital elements of the object had been computed, it became clear that the object moved in a planetlike orbit between the orbits of Mars and Jupiter. Because of illness, Piazzi was able to observe the object only until February 11. Although the discovery was reported in the press, Piazzi only shared details of his observations with a few astronomers and did not publish a complete set of his observations until months later. With the mathematics then available, the short arc of observations did not allow computation of an orbit of sufficient accuracy to predict where the object would reappear when it moved back into the night sky, so some astronomers did not believe in the discovery at all.
There matters might have stood had it not been for the fact that that object was located at the heliocentric distance predicted by Bode's law of planetary distances, proposed in 1766 by the German astronomer Johann D. Titius and popularized by his compatriot Johann E. Bode, who used the scheme to advance the notion of a "missing" planet between Mars and Jupiter. The discovery of the planet Uranus in 1781 by the British astronomer William Herschel at a distance that closely fit the distance predicted by Bode's law was taken as strong evidence of its correctness. Some astronomers were so convinced that they agreed during an astronomical conference in 1800 to undertake a systematic search. Ironically, Piazzi was not a party to that attempt to locate the missing planet. Nonetheless, Bode and others, on the basis of the preliminary orbit, believed that Piazzi had found and then lost it. That led German mathematician Carl Friedrich Gauss to develop in 1801 a method for computing the orbit of minor planets from only a few observations, a technique that has not been significantly improved since. The orbital elements computed by Gauss showed that, indeed, the object moved in a planetlike orbit between the orbits of Mars and Jupiter. Using Gauss's predictions, German Hungarian astronomer Franz von Zach (ironically, the one who had proposed making a systematic search for the "missing" planet) rediscovered Piazzi's object on December 7, 1801. (It was also rediscovered independently by German astronomer Wilhelm Olbers on January 2, 1802.) Piazzi named that object Ceres after the ancient Roman grain goddess and patron goddess of Sicily, thereby initiating a tradition that continues to the present day: asteroids are named by their discoverers (in contrast to comets, which are named for their discoverers).
The discovery of three more faint objects in similar orbits over the next six years—Pallas, Juno, and Vesta—complicated that elegant solution to the missing-planet problem and gave rise to the surprisingly long-lived though no longer accepted idea that the asteroids were remnants of a planet that had exploded.
Following that flurry of activity, the search for the planet appears to have been abandoned until 1830, when Karl L. Hencke renewed it. In 1845 he discovered a fifth asteroid, which he named Astraea.
The name asteroid (Greek for "starlike") had been suggested to Herschel by classicist Charles Burney, Jr., via his father, music historian Charles Burney, Sr., who was a close friend of Herschel's. Herschel proposed the term in 1802 at a meeting of the Royal Society. However, it was not accepted until the mid-19th century, when it became clear that Ceres and the other asteroids were not planets.
There were 88 known asteroids by 1866, when the next major discovery was made: Daniel Kirkwood, an American astronomer, noted that there were gaps (now known as Kirkwood gaps) in the distribution of asteroid distances from the Sun (see below Distribution and Kirkwood gaps). The introduction of photography to the search for new asteroids in 1891, by which time 322 asteroids had been identified, accelerated the discovery rate. The asteroid designated (323) Brucia, detected in 1891, was the first to be discovered by means of photography. By the end of the 19th century, 464 had been found, and that number grew to 108,066 by the end of the 20th century and was more than 750,000 in the second decade of the 21st century. The explosive growth was a spin-off of a survey designed to find 90 percent of asteroids with diameters greater than 1 km that can cross Earth's orbit and thus have the potential to collide with the planet (see below Near-Earth asteroids).
Later advances
In 1918 the Japanese astronomer Hirayama Kiyotsugu recognized clustering in three of the orbital elements (semimajor axis, eccentricity, and inclination) of various asteroids. He speculated that objects sharing those elements had been formed by explosions of larger parent asteroids, and he called such groups of asteroids "families."
In the mid-20th century, astronomers began to consider the idea that, during the formation of the solar system, Jupiter was responsible for interrupting the accretion of a planet from a swarm of planetesimals located about 2.8 astronomical units (AU) from the Sun; for elaboration of this idea, see below Origin and evolution of the asteroids. (One astronomical unit is the average distance from Earth to the Sun—about 150 million km [93 million miles].) About the same time, calculations of the lifetimes of asteroids whose orbits passed close to those of the major planets showed that most such asteroids were destined either to collide with a planet or to be ejected from the solar system on timescales of a few hundred thousand to a few million years. Since the age of the solar system is approximately 4.6 billion years, this meant that the asteroids seen today in such orbits must have entered them recently and implied that there was a source for those asteroids. At first that source was thought to be comets that had been captured by the planets and that had lost their volatile material through repeated passages inside the orbit of Mars. It is now known that most such objects come from regions in the main asteroid belt near Kirkwood gaps and other orbital resonances.
During much of the 19th century, most discoveries concerning asteroids were based on studies of their orbits. The vast majority of knowledge about the physical characteristics of asteroids—for example, their size, shape, rotation period, composition, mass, and density—was learned beginning in the 20th century, in particular since the 1970s. As a result of such studies, those objects went from being merely "minor" planets to becoming small worlds in their own right. The discussion below follows that progression in knowledge, focusing first on asteroids as orbiting bodies and then on their physical nature.
Geography of the asteroid belt
Geography in its most-literal sense is a description of the features on the surface of Earth or another planet. Three coordinates—latitude, longitude, and altitude—suffice for locating all such features. Similarly, the location of any object in the solar system can be specified by three parameters—heliocentric ecliptic longitude, heliocentric ecliptic latitude, and heliocentric distance. Such positions, however, are valid for only an instant of time, since all objects in the solar system are continuously in motion. Thus, a better descriptor of the "location" of a solar system object is the path, called the orbit, that it follows around the Sun (or, in the case of a planetary satellite [moon], the path around its parent planet).
All asteroids orbit the Sun in elliptical orbits and move in the same direction as the major planets. Some elliptical orbits are very nearly circles, whereas others are highly elongated (eccentric). An orbit is completely described by six geometric parameters called its elements. Orbital elements, and hence the shape and orientation of the orbit, also vary with time because each object is gravitationally acting on, and being acted upon by, all other bodies in the solar system. In most cases such gravitational effects can be accounted for so that accurate predictions of past and future locations can be made and a mean orbit can be defined. Those mean orbits can then be used to describe the geography of the asteroid belt.
Names and orbits of asteroids
Because of their widespread occurrence, asteroids are assigned numbers as well as names. The numbers are assigned consecutively after accurate orbital elements have been determined. Ceres is officially known as (1) Ceres, Pallas as (2) Pallas, and so forth. Of the 757,626 asteroids discovered through 2018, 68 percent were numbered. Asteroid discoverers have the right to choose names for their discoveries as soon as they have been numbered. The names selected are submitted to the International Astronomical Union (IAU) for approval. (In 2006 the IAU decided that Ceres, the largest known asteroid, also qualified as a member of a new category of solar system objects called dwarf planets.)
Prior to the mid-20th century, asteroids were sometimes assigned numbers before accurate orbital elements had been determined, so some numbered asteroids could not later be located. Such objects were referred to as "lost" asteroids. The final lost numbered asteroid, (719) Albert, was recovered in 2000 after a lapse of 89 years. Many newly discovered asteroids still become "lost" because of an insufficiently long span of observations, but no new asteroids are assigned numbers until their orbits are reliably known.
The Minor Planet Center at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, maintains computer files for all measurements of asteroid positions. As of 2018, there were more than 188 million such positions in its database.
Distribution and Kirkwood gaps
The great majority of the known asteroids move in orbits between those of Mars and Jupiter. Most of those orbits, in turn, have semimajor axes, or mean distances from the Sun, between 2.06 and 3.28 AU, a region called the main belt. The mean distances are not uniformly distributed but exhibit population depletions, or "gaps." Those so-called Kirkwood gaps are due to mean-motion resonances with Jupiter's orbital period. An asteroid with a mean distance from the Sun of 2.50 AU, for example, makes three circuits around the Sun in the time it takes Jupiter, which has a mean distance of 5.20 AU, to make one circuit. The asteroid is thus said to be in a three-to-one (written 3:1) resonance orbit with Jupiter. Consequently, once every three orbits, Jupiter and an asteroid in such an orbit would be in the same relative positions, and the asteroid would experience a gravitational force in a fixed direction. Repeated applications of that force would eventually change the mean distance of that asteroid—and others in similar orbits—thus creating a gap at 2.50 AU. Major gaps occur at distances from the Sun that correspond to resonances with Jupiter of 4:1, 3:1, 5:2, 7:3, and 2:1, with the respective mean distances being 2.06, 2.50, 2.82, 2.96, and 3.28. The major gap at the 4:1 resonance defines the nearest extent of the main belt; the gap at the 2:1 resonance, the farthest extent.
Some mean-motion resonances, rather than dispersing asteroids, are observed to collect them. Outside the limits of the main belt, asteroids cluster near resonances of 5:1 (at 1.78 AU, called the Hungaria group), 7:4 (at 3.58 AU, the Cybele group), 3:2 (at 3.97 AU, the Hilda group), 4:3 (at 4.29 AU, the Thule group), and 1:1 (at 5.20 AU, the Trojan groups). (See below Hungarias and outer-belt asteroids and Trojan asteroids for additional discussion of these groups.) The presence of other resonances, called secular resonances, complicates the situation, particularly at the sunward edge of the belt. Secular resonances, in which two orbits interact through the motions of their ascending nodes, perihelia, or both, operate over timescales of millions of years to change the eccentricity and inclination of asteroids. Combinations of mean-motion and secular resonances can either result in long-term stabilization of asteroid orbits at certain mean-motion resonances, as is evidenced by the Hungaria, Cybele, Hilda, and Trojan asteroid groups, or cause the orbits to evolve away from the resonances, as is evidenced by the Kirkwood gaps.
Near-Earth asteroids
Asteroids that can come close to Earth are called near-Earth asteroids (NEAs), although not all NEAs actually cross Earth's orbit. NEAs are divided into several orbital classes. Asteroids belonging to the class most distant from Earth—those asteroids that can cross the orbit of Mars but that have perihelion distances greater than 1.3 AU—are dubbed Mars crossers. That class is further subdivided into two: shallow Mars crossers (perihelion distances no less than 1.58 AU but less than 1.67 AU) and deep Mars crossers (perihelion distances greater than 1.3 AU but less than 1.58 AU).
The next-most-distant class of NEAs is the Amors. Members of that group have perihelion distances that are greater than 1.017 AU, which is Earth's aphelion distance, but no greater than 1.3 AU. Amor asteroids therefore do not at present cross Earth's orbit. Because of strong gravitational perturbations produced by their close approaches to Earth, however, the orbital elements of all Earth-approaching asteroids except the shallow Mars crossers change appreciably on timescales as short as years or decades. For that reason, about half the known Amors—including (1221) Amor, the namesake of the group—are part-time Earth crossers. Only asteroids that cross the orbits of planets—i.e., Earth-approaching asteroids and idiosyncratic objects such as (944) Hidalgo and Chiron (see below Asteroids in unusual orbits)—suffer significant changes in their orbital elements on timescales shorter than many millions of years.
There are two classes of NEAs that deeply cross Earth's orbit on an almost continuous basis. The first of those to be discovered were the Apollo asteroids, named for (1862) Apollo, which was discovered in 1932 but was lost shortly thereafter and not rediscovered until 1978. The mean distances of Apollo asteroids from the Sun are greater than or equal to 1 AU, and their perihelion distances are less than or equal to Earth's aphelion distance of 1.017 AU; thus, they cross Earth's orbit when near the closest points to the Sun in their own orbits. The other class of Earth-crossing asteroids is named Atens for (2062) Aten, which was discovered in 1976. The Aten asteroids have mean distances from the Sun that are less than 1 AU and aphelion distances that are greater than or equal to 0.983 AU, the perihelion distance of Earth; they cross Earth's orbit when near the farthest points from the Sun of their orbits.
The class of NEAs that was the last to be recognized is composed of asteroids with orbits entirely inside that of Earth. Known as Atira asteroids after (163693) Atira, they have mean distances from the Sun that are less than 1 AU and aphelion distances less than 0.983 AU; they do not cross Earth's orbit.
By 2018 the known Atira, Aten, Apollo, and Amor asteroids of all sizes numbered 17, 1,342, 8,972, and 7,618, respectively, although those numbers are steadily increasing as the asteroid survey programs progress. Most of those have been discovered since 1970, when dedicated searches for those types of asteroids were begun. Astronomers have estimated that there are roughly 15 Atiras, 45 Atens, 570 Apollos, and 270 Amors that have diameters larger than about 1 km (0.6 mile).
Because they can approach quite close to Earth, some of the best information available on asteroids has come from Earth-based radar studies of NEAs. In 1968 the Apollo asteroid (1566) Icarus became the first NEA to be observed with radar. By 2018 over 750 NEAs had been so observed. Because of continuing improvements to the radar systems themselves and to the computers used to process the data, the information provided by that technique increased dramatically beginning in the final decade of the 20th century. For example, the first images of an asteroid, (4769) Castalia, were made by using radar data obtained in 1989, more than two years before the first spacecraft flyby of an asteroid—(951) Gaspra by the Galileo spacecraft in 1991 (see below Spacecraft exploration). The observations of Castalia provided the first evidence in the solar system for a double-lobed object, interpreted to be two roughly equal-sized bodies in contact. Radar observations of (4179) Toutatis in 1992 revealed it to be several kilometres long with a peanut-shell shape; similar to Castalia, Toutatis appears predominantly to be two components in contact, one about twice as large as the other. The highest-resolution images show craters having diameters between 100 and 600 metres (roughly 300 and 2,000 feet). Radar images of (1620) Geographos obtained in 1994 were numerous enough and of sufficient quality for an animation to be made showing it rotating.
The orbital characteristics of NEAs mean that some of those objects make close approaches to Earth and occasionally collide with it. In January 1991, for example, an Apollo asteroid (or, as an alternative description, a large meteoroid) with an estimated diameter of 10 metres (33 feet) passed by Earth within less than half the distance to the Moon. Such passages are not especially unusual. On October 6, 2008, the asteroid 2008 TC3, which had a size of about 5 metres (16 feet), was discovered. It crashed in the Nubian Desert of Sudan the next day. However, because of the small sizes of NEAs and the short time they spend close enough to Earth to be seen, it is unusual for such close passages to be observed. An example of an NEA for which the lead time for observation is large is (99942) Apophis. That Aten asteroid, which has a diameter of about 375 metres (1,230 feet), is predicted to pass within 32,000 km (20,000 miles) of Earth—i.e., closer than communications satellites in geostationary orbits—on April 13, 2029; during that passage its probability of hitting Earth is thought to be near zero. The collision of a sufficiently large NEA with Earth is generally recognized to pose a great potential danger to human beings and possibly to all life on the planet. For a detailed discussion of this topic, see Earth impact hazard.
Main-belt asteroid families
Within the main belt are groups of asteroids that cluster with respect to certain mean orbital elements (semimajor axis, eccentricity, and inclination). Such groups are called families and are named for the lowest numbered asteroid in the family. Asteroid families are formed when an asteroid is disrupted in a catastrophic collision, the members of the family thus being pieces of the original asteroid. Theoretical studies indicate that catastrophic collisions between asteroids are common enough to account for the number of families observed. About 40 percent of the larger asteroids belong to such families, but as high a proportion as 90 percent of small asteroids (i.e., those about 1 km in diameter) may be family members, because each catastrophic collision produces many more small fragments than large ones and smaller asteroids are more likely to be completely disrupted.
The three largest families in the main asteroid belt are named Eos, Koronis, and Themis. Each family has been determined to be compositionally homogeneous; that is, all the members of a family appear to have the same basic chemical makeup. If the asteroids belonging to each family are considered to be fragments of a single parent body, then their parent bodies must have had diameters of 200, 90, and 300 km (124, 56, and 186 miles), respectively. The smaller families present in the main belt have not been as well studied, because their numbered members are fewer and smaller (and hence fainter when viewed telescopically). It is theorized that some of the Earth-crossing asteroids and the great majority of meteorites reaching Earth's surface are fragments produced in collisions similar to those that produced the asteroid families. For example, the asteroid Vesta, whose surface appears to be basaltic rock, is the parent body of the meteorites known as basaltic achondrite HEDs, a grouping of the related howardite, eucrite, and diogenite meteorite types. (For additional discussion of the HED meteorites and Vesta, see meteorite: Achondrites.)
Hungarias and outer-belt asteroids
Only one known concentration of asteroids, the Hungaria group, occupies the region between Mars and the inner edge of the main belt. The orbits of all the Hungarias lie outside the orbit of Mars, whose aphelion distance is 1.67 AU. Hungaria asteroids have nearly circular (low-eccentricity) orbits but large orbital inclinations to Earth's orbit and the general plane of the solar system.
Four known asteroid groups fall beyond the main belt but within or near the orbit of Jupiter, with mean distances from the Sun between about 3.28 and 5.3 AU, as mentioned above in the section Distribution and Kirkwood gaps. Collectively called outer-belt asteroids, they have orbital periods that range from more than one-half that of Jupiter to approximately Jupiter's period. Three of the outer-belt groups—the Cybeles, the Hildas, and Thule—are named after the lowest-numbered asteroid in each group. Members of the fourth group are called Trojan asteroids. By 2015 there were about 1,894 Cybeles, 1,197 Hildas, 3 Thules, and 6,179 Trojans. Those groups should not be confused with asteroid families, all of which share a common parent asteroid. However, some of those groups—e.g., the Hildas and Trojans—contain families.
Trojan asteroids
In 1772 the French mathematician and astronomer Joseph-Louis Lagrange predicted the existence and location of two groups of small bodies located near a pair of gravitationally stable points along Jupiter's orbit. Those are positions (now called Lagrangian points and designated L4 and L5) where a small body can be held, by gravitational forces, at one vertex of an equilateral triangle whose other vertices are occupied by the massive bodies of Jupiter and the Sun. Those positions, which lead (L4) and trail (L5) Jupiter by 60° in the plane of its orbit, are two of the five theoretical Lagrangian points in the solution to the circular restricted three-body problem of celestial mechanics (see celestial mechanics: The restricted three-body problem). The other three points are located along a line passing through the Sun and Jupiter. The presence of other planets, however—principally Saturn—perturbs the Sun-Jupiter-Trojan asteroid system enough to destabilize those points, and no asteroids have been found actually at them. In fact, because of that destabilization, most of Jupiter's Trojan asteroids move in orbits inclined as much as 40° from Jupiter's orbit and displaced as much as 70° from the leading and trailing positions of the true Lagrangian points.
In 1906 the first of the predicted objects, (588) Achilles, was discovered near the Lagrangian point preceding Jupiter in its orbit. Within a year two more were found: (617) Patroclus, located near the trailing Lagrangian point, and (624) Hektor, near the leading Lagrangian point. It was later decided to continue naming such asteroids after participants in the Trojan War as recounted in Homer's epic work the Iliad and, furthermore, to name those near the leading point after Greek warriors and those near the trailing point after Trojan warriors. With the exception of the two "misplaced" names already bestowed (Hektor, the lone Trojan in the Greek camp, and Patroclus, the lone Greek in the Trojan camp), that tradition has been maintained.
As of 2015, of the more than 6,200 Jupiter Trojan asteroids discovered, about two-thirds are located near the leading Lagrangian point, L4, and the remainder are near the trailing one, L5. Astronomers estimate that 1,800–2,200 of the total existing population of Jupiter's Trojans have diameters greater than 10 km (6 miles).
Since the discovery of Jupiter's orbital companions, the term Trojan has been applied to any small object occupying the equilateral Lagrangian points of other pairs of relatively massive bodies. Astronomers have searched for Trojan objects of Earth, Mars, Saturn, Uranus, and Neptune as well as of the Earth-Moon system. It was long considered doubtful whether truly stable orbits could exist near those Lagrangian points because of gravitational perturbations by the major planets. However, in 1990 an asteroid later named (5261) Eureka was discovered librating (oscillating) about the trailing Lagrangian point of Mars, and since then three others have been found, two at the trailing point and one at the leading point. Twelve Trojans of Neptune, all but three associated with the leading Lagrangian point, have been discovered since 2001. The first Earth Trojan asteroid, 2010 TK7, which librates around L4, was discovered in 2010. The first Uranus Trojan, 2011 QF99, which librates around L4, was discovered in 2011. Although Trojans of Saturn have yet to be found, objects librating about Lagrangian points of the systems formed by Saturn and its moon Tethys and Saturn and its moon Dione are known.
Learn More in these related Britannica articles:
dinosaur: The asteroid theoryThe discovery of an abnormally high concentration of the rare metal iridium at, or very close to, the K–T boundary provides what has been recognized as one of those rare instantaneous geologic time markers that seem to be worldwide. This iridium anomaly, or…
meteorite: Association of meteorites with asteroidsIf meteoritic material comes from specific regions of the asteroid belt, then the asteroids in such regions should have the chemical and mineralogical composition observed in the meteorites. The surface mineralogical composition of asteroids, in principle, can be determined directly by observations from Earth…
solar system: Asteroids and cometsThe asteroids and comets are remnants of the planet-building process in the inner and outer solar system, respectively. The asteroid belt is home to rocky bodies ranging in size from the largest known asteroid, Ceres (also classified by the IAU as a…
astronomy: Investigations of the smaller bodiesMore than 500,000 asteroids with well-established orbits are known, and thousands of additional objects are discovered each year. Hundreds of thousands more have been seen, but their orbits have not been as well determined. It is estimated that several million asteroids exist, but most are small, and their…
physical science: New discoveriesThe novel properties of the asteroids (nearly 500 of which had been discovered by the end of the century) stimulated star charts of the zodiacal regions and provided the means for improved measurements of solar-system distances.…
More About Asteroid27 references found in Britannica articles
Assorted References
- Bode's law
- Centaur objects
- Chiron
- In Chiron
- comets
- Earth impact hazards
- formation
- Galileo spacecraft
- In Galileo


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We inspire conservation of the world's aquatic treasures. The National Aquarium protects and preserves this blue planet and all of its animal and habitats through its engaging living collections in our ground-breaking Baltimore attraction and the nation's first public aquarium in Washington, DC; our science-based education programs and our hands-on experiences in the field from the Chesapeake Bay to Costa Rica; and partnerships and alliances with like-minded organizations around the world.
J. C. Lore Oyster House, also known as J. C. Lore and Sons, Inc., Seafood Packing Plant, is located at 14430 Solomons Island Road South, in Solomons, Calvert County, Maryland. It is a large two story, rectangular frame industrial building constructed in 1934 as a seafood packing plant. It replaced a 1922 building that was destroyed by the 1933 Chesapeake Potomac hurricane. It is significant for its historical association with the commercial fisheries of Maryland's Patuxent River region, and architecturally as a substantially unaltered example of an early-20th century seafood packing plant. It has been adapted by the Calvert Marine Museum to house exhibits and many of its original spaces, artifacts, and records have been incorporated into them. It was listed on the National Register of Historic Places in 1984, and declared a National Historic Landmark in 2001.
The remains of the Wye Oak supporting its clone The Wye Oak was the largest white oak tree in the United States and the State Tree of Maryland from 1941 until its demise in 2002. Wye Oak State Park preserves the site where the revered tree stood for more than 400 years in the town of Wye Mills, Talbot County, Maryland. The Wye Oak was believed to be over 460 years old at the time of its destruction during a severe thunderstorm on June 6, 2002. It measured in circumference of the trunk at breast height, high, with a crown spread of . It is believed that the acorn that became the oak germinated around the year 1540. The Wye Oak was still bearing a maturing crop of acorns when it was toppled. The Wye Oak drew public attention in 1909, when Maryland State Forester Fred W. Besley made the first official measurement of the tree. Ten years later, in 1919, it was featured in American Forestry magazine as the first tree in the American Forestry Association's "Tree Hall of Fame." The Wye Oak inspired Besley to found the Big Tree Champion Program in 1925; as a result, in 1940 the American Forestry Association named the Wye Oak one of its first National Champion Trees. By the time of its destruction 62 years later, only one other tree named that year remained standing. The tree faced a loss of a large limb in 1956 that sparked concerns, and another limb fell in 1984 that weighed 70,280 lbs. The tree fell during a heavy thunderstorm with high winds on the night of June 6, 2002. The tree's exceptionally long life has been attributed to the efforts of park managers, who applied preventative measures such as fertilizer and insecticide, as well as extensive pruning, cabling, and bracing to the branches.
Assateague State Park is Maryland's only oceanfront park. It is located on Assateague Island, a barrier island bordered by the Atlantic Ocean on the east and the Sinepuxent Bay on the west. Its two miles of ocean beaches offer swimming, beachcombing, sunbathing, surfing and fishing. The bayside offers visitors the chance to explore secluded coves by canoe or kayak. The marsh areas have a variety of wildlife, including deer, waterfowl and feral horses.Visit Assateague State Park
Easy overnight section of AT in Maryland. Begins at overnight parking lot off of 40 and follows the AT South for ~7.5 miles to the Rocky Run shelter. Along the way, trail passes through the South Mountain area (site of a Civil War battle) and the first Washington Monument. There are several camping options along the way. South of the Washington Monument, the trail crosses into Boonsboro at 40. Right on 40 is the South Mountain Inn - we didn't stop in, but apparently they're accomidating of trail hikers. Just south of 40 ( Dahlgren backpackers Campground next to the Application Trail. First come first serve camping. Contains privy with hot water shower, open field for sites, picnic tables, fire rings, and bear pack stand.Visit Dahlgren Backpacker Camp
Parent of brands like Airstream®, Thor Industries owns companies that together represent the world's largest RV manufacturer.
From 1980, when they built their first Camper Van, to today, Road Bear has been on an unquestioning quest to 'be the best for the customer'.
Roadtrippers helps people discover the world around them in an entirely new way by streamlining travel into an engaging and intuitive process.
TH2 is a joint venture created by travel giants: Thor Industries, the world's largest RV manufacturer, and thl, the world's largest RV rental and sales operator.


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Don't miss VH1's Labor Day Weekend Marathon of "Chad Ochocinco: The Ultimate Catch" this Sunday, Sept. 5, from 10 a.m. to 9 p.m.
The series, which ends it's 10-episode run this Labor Day Weekend, is filled with twitter and water cooler fodder. But the reason we're suggesting that you tune-in is to see the LA Galaxy Futboleros in action.
The Galaxy Fuboleros made a special appearance in Episode 4, which is being re-aired this Sunday at 3 p.m. In the episode, the Futboleros, a staple of the Galaxy's pre-game activities in SoccerFest at The Home Depot Center, were invited by Chad to help him pick two girls to take on a special date to San Francisco.
Chad, who had Cincinnati Bengals teammate Terrell Owens and a few other celebrity guest stop by to help him find "The One," relied on the Futboleros to find out which girls were coachable, and which ones were not— which girls were good at juggling balls, and which ones were not.
The season finale of "Chad Ochocinco: The Ultimate Catch" airs Sunday at 9 p.m. (PT) on VH1 (check local listings).
Here are some behind scenes photos from their visit...
And a clip of the Futboleros showing the girls how to do some basic soccer tricks...
Thursday, September 2, 2010
Galaxy Futboleros and Chad Ochocinco on VH1 this Labor Day Weekend
Posted by LA Galaxy at 9:45 AM
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Figure 9–3 shows how JAAS is used by the Message Queue broker. It shows a more complex implementation of the JAAS model shown in Figure 9–2.
The authentication service layer, consisting of one or more login modules (if needed) and corresponding authentication logic, is separate from the broker. The login modules run in the same Java virtual machine as the broker. The broker is represented to the login module as a login context, and communicates with the login module by means of a callback handler that is part of the broker runtime code.
The authentication service also supplies a JAAS configuration file containing entries that reference the login modules. The configuration file specifies the order in which the login modules (if more than one) are to be used and any conditions for their use. When the broker starts up, it locates the configuration file by consulting either the Java system property java.security.auth.login.config or the Java security properties file. The broker then selects an entry in the JAAS configuration file according to the value of the broker property imq.user_repository.jaas.name. That entry specifies which login module(s) will be used for authentication. The classes for the login modules are found in the Message Queue external resource files directory, whose location depends on the operating system platform you are using; see Appendix A, Platform-Specific Locations of Message Queue Data for details.
The relation between the configuration file, the login module, and the broker is shown in the following figure. Figure 9–4.
The fact that the broker uses a JAAS plug-in authentication service remains completely transparent to the Message Queue client. The client continues to connect to the broker as it did before, passing a user name and password. In turn, the broker uses a callback handler to pass login information to the authentication service, and the service uses the information to authenticate the user and return the results. If authentication succeeds, the broker grants the connection; if it fails, the client runtime returns a JMS security exception that the client must handle.
After the Message Queue client is authenticated, if there is further authorization to be done, the broker proceeds as it normally would, consulting the access control file to determine whether the authenticated client is authorized to perform the actions it undertakes: accessing a destination, consuming a message, browsing a queue, and so on.


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Design Description:
COMBINED SOLD 300+ T-SHIRTS – Not available in stores. you cant find this anywhere in store. a collector item! 100% statifaction guarantee or your money back! (for ANY reason) TIP Order 2 of more you save on shipping
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Custom Table
To create your own custom table, choose a row variable and column variable, then click on the Go! button.
Presbyterian Panel Survey, May 2001 - The U.S. Congregational Life Survey (Presbyterian Panel Version), Members
Data Archive > U.S. Surveys > Religious Groups > Members or Leaders > Presbyterian > Custom Table


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Welcome one welcome all, my name is Aron.
I want to say thank you and welcome to New York. I will try my best to orginize and help anyone out that I can.
I am not a native New Yorker so feel free to make suggestions or correct me if I am wrong. I know there is so much this state has to offer...
Would anyone be interested in doing a Mid Hudson Bridge photoshoot meetup? It is the bridge that crosses the Hudson connecting Highland and Poughkeepsie. I shot some stuff there today and yesterday, this place has a lot of different photo ops. There is a pedestrian walkway you can cross the bridge...
2008 Altamont Town Garage Sale & Flea Market
Throughout the Village and Fairgrounds
Admission: Free, for spectators and buyers
When: Saturday May 3. 2008
Show hours are from 8:30am to 4:00 pm
The event will be held rain or shine. In the...
Just wondering if they are going to have the Spring show, I haven't heard anything or recieved my post card yet. Thanx in advance for the help.
It's coming up soon anyone going???
Here's a few photos from the NEF Photographer's Party last weekend!! :D
Thanks to everyone for coming out :) :happy We had a great time and enjoyed seeing some old friends and meeting some new ones!!
First, some introductions... from left to right: Robin (Shutterbug758) and her husband...
Come and join us for a NEF Photographers Party!!
You are invited to join us at our home,
I went up to the ADK Balloon Festival early Saturday morning. The balloons started to launch around 6:30am (yes, am! :doh) and it was in the 30s. As the sun came up, I thought the fog would burn off, but it eventually got so thick that all the balloons were grounded. At least I was able to get a...
Aug 11th @ 11:30PM to Aug 12th @ When we finish
Trish and I will be hosting a small get together at our house for viewing/shooting this event if anyone is interested... we have plenty of yard room and the area is fairly dark (better than most actually)... so if you have a tripod... a release......
Tentative date, July 25th. please let me know if there are objections to this date, its the first Saturday i have free unless people want to do it this Saturday. I would be fine with that but figured it would be tough on short notice.
My game plan is sometime around noon at the zoo for 2-3...
Ross and I have been tossing around the idea of having an end of summer photography party at our place. Probably sometime during the very end of August or first couple weeks in September. :pt
It would be a combination of some good food and drinks, a chance to hang out and do some shooting...
I know it's last minute... but Ross and I are going to try out a new butterfly place tomorrow (Sunday). Anyone up for some macro?!! :happy
It's called Popp Butterfly Conservatory and it's located in Oneonta, NY (about 1.5 hours east of Albany via I-88). If anyone from the Albany area wants to...
Who would be interested in a group shoot at the Syracuse Zoo? If we have some interest i will pick a date and figure out the details.
Sunday March 29, 2009, Albany Clarion Inn, 10AM-3PM, buy/sell/trade, new/used, Nikon, Canon, Leica medium format, Biew cameras, Hasselblad, collectable, antique, lenses, microscopes, scientific equipment, books, dark room, film, digital, & more, I90, Exit 5 (Everett Rd), South on...
Trish and I are heading up to the Fort Edward plains Saturday morning to see if we can catch up with the pair of Snowy Owls that have been seen there every day in the past couple weeks... jet me a PM if you are planning on being in the area!!!
Sunday Nov 2, 2008, Albany Clarion Inn, 10AM-3PM, buy/sell/trade, new/used, Nikon, Canon, Leica medium format, Biew cameras, Hasselblad, collectable, antique, lenses, microscopes, scientific equipment, books, dark room, film, digital, & more, I90, Exit 5 (Everett Rd), South on...
Its officially time for our Macro Groupshoot/Workshop!
We are scheduling this for September 14th (Sunday) from 10am - ?... possibly a campfire later on in the evening. Contact myself or Trish if you plan on attending so we can get a good accurate body count and give you...
Who's up for a field trip to Howe Caverns?
I spoke with the good folks there and photography is allowed as long as you don't bring any light stands or monopods/tripods. It's a balmy 52 degrees underground :) . Please check out the site above and let me know what...
this weekend at the state fair grounds, close to 7,000 classic cars. I will be there most of the weekend covering the show for multiple magazines if any one wants to meet up. shoot me a pm if interested.
i know its short notice but i figure since its free maybe somone will want to check it out.
i plan on going on saturday for sure, looks like an awesome time!
Ok, lets see if any one wants to set up a group meet for this place. here are a couple links for info:
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Recovery drinks are expensive. My go-to "branded" recovery drink - Recoverite** - retails for $50/tub. That works out to $1.56 per serving (2 level scoops of powder, mixed in 10 oz water), which might not seem like a lot, but multiplied by 5 workouts/week and 52 weeks/year adds up to $405.
Chocolate milk, of course, is a perfectly acceptable alternative. And at $2.99 per half-gallon, the cost per 10-oz serving goes down to $0.47 ($122/year, a 70% savings). My favorite supermarket-bought recovery drink, though, is Silk Soy chocolate milk - at $3.99/half-gal, still only $0.62 per 10 oz).
Two downsides to chocolate milk: refrigeration and expiration (and therefore, more frequent shopping trips). Powder-based drinks such as Recoverite travel better and, in my opinion, taste better at room temperature.
But powder-based recovery drinks don't have to break the bank - even ones with approximately the same ingredients as a branded recovery drink. The main thing, according to nutrition scientists, is a carbs-to-protein ratio of somewhere around 3:1 or 4:1. The carbs restore muscle glycogen, the protein repairs and builds muscle tissue, and the two act synergistically to help you recover. Some recovery drinks (including Recoverite) are also fortified with electrolytes and extra amino acids.
Turns out, most of these ingredients can be bought separately and combined in the same proportions as "branded" drinks - for substantial cost savings. The main ingredients in Recoverite are maltodextrin (carbs), whey protein, L-glutamine amino acid, and a full-spectrum electrolyte mix. After those, it's just flavoring, sweeteners, and a few extra amino acids in very small quantities.
And guess what? electrolytes are all readily (and cheaply) available at Amazon.com. I found whey protein (Muscle Milk brand) for even cheaper ($28.99 / 6 pounds) at Costco.
And so it's with that in mind that I present the Freshwater Swimmer Generic-but-still-Awesome Powdered Recovery Drink - nutritionally indistinguishable from Recoverite:
- 2 cups maltodextrin
- 2/3 cup whey protein
- 1 rounded Tbsp L-glutamine
- 6 scoops Hammer Endurolytes
The recipe produces 6 servings - combine with 60 oz water in a half-gallon container, shake well, refrigerate, and voila! High-quality powdered recovery drink at $0.58 per serving.
How does it taste? Honestly, with no added flavoring - just the natural vanilla flavors included in the protein powder - it tastes even better than Recoverite.


text: > RPMs or Debian. With Red Hat and descendents (Fedora, Centos) you can > use kickstart, which is a lovely tool for installing clusters. > Kickstart run on top of PXE and DHCP makes installing most systems a > matter of turning them on (after making a single host specific MAC don't forget the zero-install approach - nothing installed on nodes. just export the nodes' root filesystem from a fileserver, and you never have to do anything per-node. yum and rpm both let you install within a separate tree, so the fileserver doesn't need to be running the same config as the nodes. obviously, this results in a certain amount of NFS traffic, as opposed to having those files installed on the node's disk. issues: - diskless nodes are very attractive in many contexts: reliability, price, maintainability, etc. - running NFS-root is a way of tolerating local disk faults; lack of swap may or may not be a problem. - NFS can easily be faster than local disk IO. - in aggregate, a buch of diskless nodes will, in the worst case, create much more traffic than your net and fileserver can handle. - my experience so far with 50-100-node clusters is that a single NFS-connected fileserver is actually pretty good. (our nodes have a local disk used for things like checkpoints of big parallel applications.) - for big MPI clusters, it's extremely attractive to put fileservers directly onto the MPI fabric. suddenly, gigabit is no longer a limiter for file IO and systems like Lustre can give some pretty impressive data rates. - this scheme is probably optimal for very hetrogenous datacenters as well, where you might boot a node in some random OS purely for a particular user/app. that kind of thing seems very dubious to me, but it would only take a few minutes of perl scripting to write a web frontend to select things like IP, distro, kernel, server, etc for a particular node, and propogate the changes. I think that for a small cluster, I'd consider having the nodes with full installs on them. for anything larger than say 4 nodes, I definitely prefer the root-on-fileserver approach with "ephemeral" nodes. it's also pretty sexy to take a node out of the box, plug it in and have it accept jobs in a minute or so with no manual intervention. > course, require knowledge, experience, wisdom, and time to do right, > which is why sysadmins get paid and are worth a very decent salary. hmm. anyone for a cluster-admin salary survey? regards, mark hahn.


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Notification highlight
- RRB Bhopal recruitment 2019-20| Group D, ALP & Technician jobs for 10th pass at www.rrbbpl.nic.in
- RRB Bhopal ALP Technician vacancy 2019 notification
- ALP Technician jobs Eligibility criteria
- RRB Bhopal jobs 2019- Apply online at www.rrbbpl.nic.in
- Upcoming RRB Bhopal recruitment 2019-2020 Latest Jobs notification updates
RRB Bhopal recruitment 2019-20| Group D, ALP & Technician jobs for 10th pass at www.rrbbpl.nic.in
RRB Bhopal recruitment 2019: Bhopal railway recruitment board, invites candidates from eligible candidates for filling bumper vacancies for recruiting the Group D, ALP (Assistant Loco Pilot) & Technician Grade 3 jobs. Candidates have a golden opportunity who are looking for the 10th pass job & ITI diploma holder and want to make their career in railway Jobs. Here candidates get high profile job with attractive pay scale of Rs.19900/- per month. Here you will get step by step procedure and full detail information for the RRB ALP & Technician Jobs. If you are interested in this job we recommended you to keep reading to know about important aspect of eligibility criteria, age limit, how you can apply , formalities required, selection procedure/ method, Application fee important dates, qualification details and most important official notification and apply online link for the Bhopal railway (RRB) Bharti 2019 notification.
Check out latest RRB Group D vacancy (CEN 02/ 2019)
RRB Bhopal ALP Technician vacancy 2019 notification
Every year thousands of candidates apply for the RRB ALP (Assistant Loco Pilot) & Technician Bharti. It is one the biggest post which provides the huge number of vacancies and recruits the candidates who meet their eligibility criteria & selection procedure. So before knowing how to apply, you should know what is the latest eligibility criteria for this jobs.
|Post name: ALP & Technician
|Name of department: RRB
|Location: Bhopal
|vacancies: 1679 Posts
|Qualification Details:
|Age limit
|Selection process
|For ALP post: Applicants must be Matriculation (10th Class) /SSC/ITI from certified Board or Institution.
For Technician post: Applicants must be 10th pass/ SSLC plus ITI/ course completed Act Apprentices OR, 10+2 with Physics and Maths OR Diploma in Engineering (As Applicable).
|Minimum Age: 15 Years
Maximum Age: 30 Years
(as on 01-07-2019)
|Online Exam
Document Verification
Also read: RPF/RPSF recruitment 2019
Check out more upcoming jobs:-
ALP Technician jobs Eligibility criteria
If you are interested in this job and wants to apply online for this job you must know detailed eligibility criteria. In this section, you will come to know about education required, selection procedure and age limit.
check out more similar jobs for 10th pass:
Age limit:- The minimum age & maximum age limit of Jobseeker must be 15 & 30 years respectively as per 01-07-2019.
Application Fee: Candidates have to pay Rs. 500/- through Debit Card, Credit Card, Net Banking or E Challan Offline Payment Mode. Sc/ ST/ Ex-Servicemen/ PWD/ Female/ Transgender/ Minorities/ Economically backward class candidates have to pay Rs. 250/-
Note: For every govt job there is an upper Age Relaxation for the reserved categories. For SC/ST Candidates 05 years, For OBC Candidates 03 years & For PWD Candidates 10 years
- Selection procedure: Once you applied for the post and meet above eligibility criteria then you would be selected or shortlisted for the RRB job. The selection will be made on the basis of 10th/ ITI class marks & documents verification.
- Online Exam
- Interview
- Document Verification
- Candidates have to answer the reasoning MCQ type question related to General Awareness, Arithmetic, General Intelligence, Reasoning, Technical Ability & General Science.
Important Dates
|Tentative dates
|Start date for Submission of applications form
|_-_-2019 (update soon)
|The last date for submission of Applications form
|_-_-2019 (update soon)
|Online Fee submission last date
|_-_-2019 (update soon)
|Offline post office fee submission last date
|_-_-2019 (update soon)
Important Links- Official Notification & Application form
|Official Notification
|Apply online
RRB Bhopal jobs 2019- Apply online at www.rrbbpl.nic.in
Now, if you are interested in the same post and look yourself eligible for this post then firstly you have to read the official advertisement which is given above.Then you have to print application form given at the end of in the official website. If you are wondering & still confused how to apply online? then following the following step as mentioned.
Firstly candidates have to download the official notification.
- Firstly, click here
- Now select your RRB zone.
- Then select important links/ Recruitment option
- Select the desirable jobs.
- Upload your valid details, Photo ID proof, Aadhar no. etc.
- Now click on submit button.
- Check twice before submitting your application form.
- Now pay the fees and print out your application form for further uses.
Note: Always keep the original document with you.
Upcoming RRB Bhopal recruitment 2019-2020 Latest Jobs notification updates
If you are waiting for more RRB Bhopal Jobs then you are at right place. Here our team provide you latest job and keep update you with correct information & latest upcoming government jobs. Others Job website maybe share wrong information with you but our dedicated team with provide always right information. Our team will regularly update this page for the RRB Bhopal vacancy 2019. You are requested to bookmark us by pressing (Ctrl + D) from your keyboard or note down our website for more jobs. You can also subscribe us for daily free job alert on your mobile. We understand how this govt. job assist for you:).


text: On Tue, 2003-03-11 at 16:55, Robert G. Brown wrote: > As I said before, if y'all want to wait 2-3 days before ordering, I'd be > happy to give at least a short report on the device as soon as I receive > it. As in, well made/cheap, works/broken out of box, horribly exciting > or rather dull (but useful) or useless as the case may be. I got one from EFI about 2 months ago. I wanted to understand why my electricity bill was so outrageous in the winter. It worked fine out of the box, you don't even need to read the manual. I used it to check the consumption of almost everything electric in my house. You can use it to check the immediate consumption, but it also accumulates it as long as it is plugged. It's easy to use and it seems robust. The only problem may be the limitation of 3KW (AFAIR) on the measured output. Patrick -- Patrick Geoffray, PhD Myricom, Inc. http://www.myri.com


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In a move that could set a new trend in the industry, Goldman Sachs (NYSE:GS) revealed plans on Wednesday to begin disclosing the value of its money market mutual funds on a daily basis.
Continue Reading Below
The switch comes as investors and regulators push Goldman and other fund managers to increase transparency in the $2.7 trillion fund industry.
"As a leading provider of liquidity solutions, we believe that more frequent disclosure and greater transparency will benefit investors," James McNamara, president of Goldman Sachs Mutual Funds, said in a statement. "It is our belief that this level of transparency will also benefit the ongoing dialogue around potential regulatory changes to money market funds."
Goldman said it will begin disclosing the daily market value for its U.S.-domiciled commercial paper money market funds effective on Wednesday.
The Wall Street heavyweight said it plans to also release similar metrics on government and municipal funds next week and the daily value of non-U.S. money market funds in the "near future."
This marks a big change for Goldman, which currently releases money market fund values monthly, but with a 60-day lag. Still, money funds, which are considered among the safest investments, don't typically see dramatic day-to-day fluctuations.
With an estimated $133 billion in assets under management, Goldman is the No. 8 U.S. money-fund firm, The Wall Street Journal reported, citing research firm Crane Data.
Shares of New York-based Goldman gained 0.26% to $133.40 ahead of Wednesday's opening bell, putting them on pace to maintain their 12-month gain of 35%.


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Cinco de Julio
July 10, 2011
Last Tuesday we went to grab a bite at Don Pedro on Lawrenceville Highway in Lilburn. OMG. Probably the best Mexican food I've had in a long time. A friend discovered their sister restaurant (same name, different location) on Buford Highway recently and has been raving about it. The Lilburn location was a little closer to our house, so we decided to check it out. I'm so glad we did.
Not only is Don Pedro's home to the $.99 taco, but they have all you can drink Horchata, which is one of Jim's favorite summertime drinks. Also, be sure to taste the Jarrito — a fruit flavored Mexican soda. They have an orange/mango flavor (we weren't sure which it was) and pineapple.
Obviously, you can't go wrong with a $.99 taco, but all the varieties we got were delicious and included: Asada (steak), Pastor (a spicy pork) and Picadillo de Pollo (shredded chicken). Our friend also tried the Lengua (tongue) and said it was very yummy.
In addition to the tacos, we tried the Mulitas (two tortillas laid flat with steak, avocado, cheese, onions and cilantro), Chicken Tostadas and the Tortas, a meat and veggie filled sandwich pocket. We also enjoyed a side of Rice and Beans. Between the four of us that went for dinner, we couldn't agree on what we like best, but it was a toss up between the Mulitas and the Tortas. (For the record, my vote is for the Tortas.)
We couldn't stop thinking about their tasty fare, so Jim went back yesterday and picked up a to go order for dinner :0)
One Response to "Cinco de Julio"
July 12, 2011 at 3:32 am
[…] Cinco de Julio […]


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His failed policies are what's to blame
Obama Blames Dem Losses on 'Fox News in Every Bar and Restaurant'
Nov 30, 2016 // 9:20am
President Barack Obama has lashed out at Fox News at various times during his presidency and it's continuing in the final weeks of his time in office.
In an interview with Rolling Stone, Obama was asked if he still believes the U.S. is a "progressive country" following the election of Donald Trump as the 45th president.
He pointed to Democrats' failure to reach working-class white voters, as he did in 2008 and 2012.
He said:
In this election, [they] turned out in huge numbers for Trump. And I think that part of it has to do with our inability, our failure, to reach those voters effectively. Part of it is Fox News in every bar and restaurant in big chunks of the country, but part of it is also Democrats not working at a grassroots level, being in there, showing up, making arguments. That part of the critique of the Democratic Party is accurate. We spend a lot of time focused on international policy and national policy and less time being on the ground. And when we're on the ground, we do well. This is why I won Iowa.It comes after Obama, in a sit-down with Bill Maher before the election, said that "if I watched Fox News, I wouldnt vote for me either."
Reacting this morning on "Fox & Friends," Herman Cain said it's "sad" that Obama doesn't want the American people to know the truth, criticizing the president for repeatedly trying to convince people not to watch Fox News.
Be the change you wish to see in the world." -Mahatma Gandhi
Those who claim perfect mental health are truely insane.
His failed policies are what's to blame
A True America Hero