Massive star cluster found in Milky Way
{{date|March 26, 2005}}
[[Image:Pleiades large.jpg|250px|right|thumb|This file image of the [[w:Pleiades|Pleiades]] star cluster does not show the recent Westerlund 1 discovery, but is used to illustrate what a star cluster looks like. ''Source: [[w:NASA|NASA]]'']]
European astronomers discovered a very young and huge [[w:Star cluster|star cluster]] within our [[w:Milky Way|Milky Way]] galaxy using [[w:ESO|European Southern Observatory]] telescopes. The discovery was made at the [[w:La Silla Observatory|La Silla Observatory]] in [[w:Chile|Chile.]]

Hidden behind a veil of dust and gas, the super star cluster, known as Westerlund 1, is
1000 times closer than any other known clusters. These Super star clusters were previously known to exist as pairs or groups of interacting galaxies located at immense intergalactic distances.  It is so close--within 10,000 light years--scientists will be able to examine its structure in detail.  Until now, super clusters were far too distant for individual
stars to be distinguished.

Initial observations have led scientists to conclude the group contains at least 100,000 times the mass of the [[w:Sun|Sun]], with some single stars shining with a power of 1,000,000 suns and 2000 times larger than our own.  All the stars are in a region less than six [[w:Light year|light years]] across.

The existence of Westerlund 1's has been known since 1961. Discovered by Swedish astronomer Bengt Westerlund while in Australia, the cluster is located in the Southern constellation [[w:Ara|Ara]] (the Altar). It was a dimming factor of more than 100,000 caused by the gas and dust between us and the cluster that prevented the actual structure and nature of the phenomenon to be determined.

Using a variety of instruments, including the Wide Field Imager (WFI)
attached to a 2.2 meter scope and the Superb-Seeing Imager 2 (SuSI2) camera
on the ESO 3.5 meter [[w:New Technology Telescope|New Technology Telescope]]
(NTT), 200 cluster member stars were identified. These and other
observations have revealed the cluster contains young stars on the
order of 30-40 times more massive than our own Sun.  The age range has been
determined at 3.5 to five million years old, making this cluster very young
compared to the Galaxy itself at around 13.5 billion years.

The research will appear in the leading research journal ''Astronomy and Astrophysics'', and is titled "On the massive stellar population of the Super Star Cluster
Westerlund 1", by J.S. Clark and colleagues.  A second paper, "Further
Wolf-Rayet stars in the starburst cluster Westerlund 1", by Ignacio
Negueruela and Simon Clark will also be published in the same journal.

==Sources==
*{{source|
url=http://www.eso.org/outreach/press-rel/pr-2005/pr-08-05_pf.html|
title=ESO's Telescopes Uncover Super Star Cluster in the Milky Way| 
author=|pub=ESO|date=March 22, 2005}}

 {{archive}}
[[Category:Space]]
[[Category:Science and technology]]
[[Category:Published]]
[[Category:Astronomy]]
[[Category:European Southern Observatory]]
[[Category:Chile]]
[[Category:South America]]
Pleiades star cluster does not show the recent Westerlund 1 discovery, but is used to illustrate what a star cluster looks like. Source: NASA
European astronomers discovered a very young and huge star cluster within our Milky Way galaxy using European Southern Observatory telescopes. The discovery was made at the La Silla Observatory in Chile.

Hidden behind a veil of dust and gas, the super star cluster, known as Westerlund 1, is
1000 times closer than any other known clusters. These Super star clusters were previously known to exist as pairs or groups of interacting galaxies located at immense intergalactic distances.  It is so close--within 10,000 light years--scientists will be able to examine its structure in detail.  Until now, super clusters were far too distant for individual
stars to be distinguished.

Initial observations have led scientists to conclude the group contains at least 100,000 times the mass of the Sun, with some single stars shining with a power of 1,000,000 suns and 2000 times larger than our own.  All the stars are in a region less than six light years across.

The existence of Westerlund 1's has been known since 1961. Discovered by Swedish astronomer Bengt Westerlund while in Australia, the cluster is located in the Southern constellation Ara (the Altar). It was a dimming factor of more than 100,000 caused by the gas and dust between us and the cluster that prevented the actual structure and nature of the phenomenon to be determined.

Using a variety of instruments, including the Wide Field Imager (WFI)
attached to a 2.2 meter scope and the Superb-Seeing Imager 2 (SuSI2) camera
on the ESO 3.5 meter New Technology Telescope
(NTT), 200 cluster member stars were identified. These and other
observations have revealed the cluster contains young stars on the
order of 30-40 times more massive than our own Sun.  The age range has been
determined at 3.5 to five million years old, making this cluster very young
compared to the Galaxy itself at around 13.5 billion years.

The research will appear in the leading research journal Astronomy and Astrophysics, and is titled "On the massive stellar population of the Super Star Cluster
Westerlund 1", by J.S. Clark and colleagues.  A second paper, "Further
Wolf-Rayet stars in the starburst cluster Westerlund 1", by Ignacio
Negueruela and Simon Clark will also be published in the same journal.
Space Science and technology Published Astronomy European Southern Observatory Chile South America