High Angular Resolution Studies of Young Stars
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
{'SignBlockName': 'Edward G. Schmidt', 'PO_EMAI': None, 'PO_PHON': None}
Much progress has been made during the past decade in                           observations of interstellar clouds of gas and dust and of the                  formation of new stars that takes place in cold, dense clumps in                many of these clouds.  The question that is unanswered is "Do any               of these currently forming stars acquire planetary systems                      similar to our own?"  The question is unanswered because up to                  now observers lacked the angular resolution to detect planets or                planetary precursor object across interstellar distances. The                   Principal Investigator proposes to overcome this difficulty by                  using lunar occultations of star forming regions, which he thinks               will increase the angular resolution sufficiently to allow him to               observe planetary systems in the making.
{'FirstName': 'Michal', 'LastName': 'Simon', 'PI_MID_INIT': None, 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Michal Simon', 'EmailAddress': 'michal.simon@sunysb.edu', 'NSF_ID': '000089645', 'StartDate': '02/01/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'SUNY at Stony Brook', 'CityName': 'STONY BROOK', 'ZipCode': '117940001', 'PhoneNumber': '6316329949', 'StreetAddress': 'W5510 FRANKS MELVILLE MEMORIAL L', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'New York', 'StateCode': 'NY', 'CONGRESSDISTRICT': '01', 'CONGRESS_DISTRICT_ORG': 'NY01', 'ORG_UEI_NUM': 'M746VC6XMNH9', 'ORG_LGL_BUS_NAME': 'THE RESEARCH FOUNDATION FOR THE STATE UNIVERSITY OF NEW YORK', 'ORG_PRNT_UEI_NUM': None}
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{'Code': '1215', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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