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Gerard van Belle

From Wikipedia, the free encyclopedia
American astronomer (born 1968)
Gerard Theodore van Belle
Born (1968-10-30)30 October 1968 (age 57)
Tallahassee, Florida
Alma materUniversity of Wyoming,Johns Hopkins University,Whitman College
Known forThe use ofinterferometry in studies of thestellar structure and detection ofextrasolar planets.
Awards2002 Edward Stone Award for Outstanding Research Publication
Scientific career
FieldsAstronomy
InstitutionsLowell,ESO,Caltech,JPL,St. Mary's College of Maryland
ThesisAngular Size Measurements of Highly Evolved Stars (1996)
Doctoral advisorH. Mel Dyck

Gerard Theodore van Belle (born October 30, 1968) is an Americanastronomer. He is anexpert in optical (visible and near-infrared) astronomical interferometry. He currently works at theLowell Observatory as the Director of Science.[1]

Education

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van Belle received a bachelor's degree in physics fromWhitman College in 1990, a master's degree in physics from TheJohns Hopkins University in 1993, and a Ph.D. in physics from theUniversity of Wyoming in 1996. While at Whitman College, he initiated as a member of theSigma Chi fraternity.

Career

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After schooling, van Belle took a position at theJet Propulsion Laboratory as an instrument architect forNASA'sKeck Interferometer, and later joined the Michelson Science Center (nowNASA Exoplanet Science Institute) atCaltech in 2003. He has participated in the commissioning of thePalomar Testbed Interferometer, and theCHARA Array. In 2007, he became a member of the astronomy faculty at theEuropean Southern Observatory (ESO), and instrument scientist for the PRIMA instrument of ESO'sVLTI facility; later in early 2011 he was also appointed instrument scientist for the MATISSE instrument of the VLTI. Since August 2011 he has been a member of the astronomer faculty atLowell Observatory. In May 2017 he was appointed the Director of theNavy Precision Optical Interferometer (NPOI), and after a one-year tenure became Chief Scientist for the facility, until 2022. In May 2024 he was appointed the Director for Science at Lowell Observatory.

Research

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van Belle has utilizednear-infraredastronomical interferometers to measure the sizes of hundreds of nearby stars.[2][3][4][5][6][7][8]The first direct measurement of stellar shape was carried out by a team led by him using the Palomar Testbed Interferometer to make observations of the rapidly rotating starAltair.[9] He also contributed to practical considerations of operating astronomical interferometers, particularly regarding considerations of calibration of these complicated instruments.[10][11][12]

Leadership

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van Belle served as President of theInternational Astronomical Union's Commission 54 on Optical and Infrared Interferometry, for 2012–2015, after terms as Vice President (2009–2012) and Secretary (2006–2009).

Honors, awards and accolades

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Asteroid25155 van Belle is named for him.[13]In 2018 Dr. van Belle was named a recipient of the Significant Sig Award of the Sigma Chi fraternity.[14]

References

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  1. ^https://lowell.edu/people/gerard-van-belle/
  2. ^Dyck, H. M., van Belle, G. T., & Benson, J. A. (1996). "Angular Diameters and Effective Temperatures of Carbon Stars".Astronomical Journal.112: 294.Bibcode:1996AJ....112..294D.doi:10.1086/118014.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  3. ^van Belle; G. T.; et al. (1996). "Angular Size Measurements of 18 Mira Variable Stars at 2.2 microns".Astronomical Journal.112: 2147.Bibcode:1996AJ....112.2147V.doi:10.1086/118170.
  4. ^van Belle; G. T.; et al. (1997)."Angular Size Measurements of Carbon Miras and S-Type Stars".Astronomical Journal.114: 2150.Bibcode:1997AJ....114.2150V.doi:10.1086/118635.
  5. ^van Belle, G.T.; et al. (1999). "Radii and Effective Temperatures for G, K, and M Giants and Supergiants".The Astronomical Journal.117 (1):521–533.Bibcode:1999AJ....117..521V.CiteSeerX 10.1.1.21.9648.doi:10.1086/300677.S2CID 18617983.
  6. ^van Belle, G.T.; et al. (2009)."Supergiant temperatures and linear radii from near-infrared interferometry".Monthly Notices of the Royal Astronomical Society.394 (4):1925–1935.arXiv:0811.4239.Bibcode:2009MNRAS.394.1925V.doi:10.1111/j.1365-2966.2008.14146.x.S2CID 118372600.
  7. ^van Belle, G. T., & von Braun, K. (2009). "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars".Astrophysical Journal.694 (2):1085–1098.arXiv:0901.1206.Bibcode:2009ApJ...694.1085V.doi:10.1088/0004-637X/694/2/1085.S2CID 18370219.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  8. ^van Belle; G. T.; et al. (2021)."Direct Measurements of Giant Star Effective Temperatures and Linear Radii: Calibration against Spectral Types and V - K Color".Astrophysical Journal.922 (2): 163.arXiv:2107.09205.Bibcode:2021ApJ...922..163V.doi:10.3847/1538-4357/ac1687.
  9. ^van Belle; G. T.; et al. (2001). "Altair's Oblateness and Rotation Velocity from Long-Baseline Interferometry".Astrophysical Journal.559 (2): 1155.Bibcode:2001ApJ...559.1155V.doi:10.1086/322340.S2CID 13969695.
  10. ^van Belle; G. T. (1999). "Predicting Stellar Angular Sizes".Publications of the Astronomical Society of the Pacific.111 (766): 1515.arXiv:astro-ph/9904295.Bibcode:1999PASP..111.1515V.doi:10.1086/316462.S2CID 119336489.
  11. ^van Belle, G. T., & van Belle, G. (2005). "Establishing Visible Interferometer System Responses: Resolved and Unresolved Calibrators".Publications of the Astronomical Society of the Pacific.117 (837):1263–1270.arXiv:astro-ph/0508266.Bibcode:2005PASP..117.1263V.doi:10.1086/449603.S2CID 15867046.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  12. ^van Belle; G. T.; et al. (2008). "The Palomar Testbed Interferometer Calibrator Catalog".Astrophysical Journal Supplement Series.176 (1): 276.arXiv:0711.4194.Bibcode:2008ApJS..176..276V.doi:10.1086/526548.S2CID 10713221.
  13. ^Asteroid 25155 van Belle data online at JPL Horizons
  14. ^"Fraternity Announces Recipients of its 2018 Significant Sig Award".sigmachi.org.

External links

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