Nancy Houk
Alma mater
  • University of Michigan 1962, B.S.
  • Case Institute of Technology 1964, M.S.
  • Case Western Reserve University 1967, Ph.D.
Known forAtlas of Objective Prism Spectra
Scientific career
Fields
InstitutionsUniversity of Michigan

Nancy Houk is an American astronomer who led the effort to establish a comprehensive database of stellar temperatures and luminosities.[1]

Education

After earning her Doctorate in Astronomy from Case Western Reserve University in 1967, Nancy Houk was a postdoctoral student at Case Western and the Kapteyn Laboratory in the Netherlands.

During her undergraduate years at the University of Michigan, Houk researched at the Maria Mitchell Observatory, a memorial to Maria Mitchell, America's first woman professional astronomer.

Career

Houk joined the Astronomy Department at the University of Michigan in 1970 as a Research Associate,[2] followed by promotions to Research Associate in 1973, the Associate Research Scientist in 1977, then Research Scientist in 1985.

Research

Houk led the effort to establish a comprehensive database of stellar temperatures and luminosities. Houk's photographic observations of stars were made using the University of Michigan 0.61-m Curtis Schmidt telescope located at Cerro Tololo Interamerican Observatory (CTIO). CTIO, established in 1960, is a campus of astronomical telescopes located east of La Serena, Chile at an altitude of 2200 meters. CTIO is part of the National Optical Astronomy Observatory (NOAO). The telescope that Houk used was moved from Portage Lake Observatory in Michigan to CTIO in 1966. Houk began her observations in 1971. By 2014, the project had assembled five volumes covering the sky from the south celestial pole to +5° declination, consisting of 162,900 stars in total.[3]

The plates images are spectral images, taken with an objective prism at the front of the telescope. The images provide information about the physical properties of stars such as their composition of atomic elements and molecules, mass, temperature, rotational properties, age, distance, spectra classification and more. Houk used this data to construct the fundamental diagram used in astrophysics called the Hertzsprung-Russell Diagram that forms the basis of modern astrophysics.[4]

Astronomical Photographic Data Archive

Houk retired in 2001 and donated half her plate collection which surveyed the entire southern hemisphere night sky to the Astronomical Photographic Data Archive (APDA) in 2004.[5] The other half of her collection resides in Japan. APDA, located at the Pisgah Astronomical Research Institute, plans to digitize her photographic plates.[6]

Nancy Houk transferring her collection to APDA. Standing next to her is Michael Castelaz, PARI Research Director in 2004 who accepted Nancy Houk's collection on behalf of APDA.

Publications

Her research is published in 5 volumes of the Michigan Spectral Catalog where the first set of HR diagrams are presented from her data. The publications resulting from her research, and conferences where she presented her results are listed below:

References

  1. ↑ "Memoir: Nancy Houk". Faculty History Project. University of Michigan. Archived from the original on 2019-05-04. Retrieved 2017-09-01.
  2. ↑ Hiltner, W. A. (January 1972), "The University of Michigan Observatory report", Bulletin of the Astronomical Society, 4: 119–123, Bibcode:1972BAAS....4..119H.
  3. ↑ Hearnshaw, John B. (2014), The Analysis of Starlight: Two Centuries of Astronomical Spectroscopy (2 ed.), Cambridge University Press, p. 185, ISBN 978-1107782914
  4. ↑ Capaccioli, M., ed. (December 6, 2012), "Astronomy with Schmidt-Type Telescopes", Proceedings of the 78th Colloquium of the International Astronomical Union, Asiago, Italy, August 30–September 2, 1983, Springer Netherlands, p. 42, ISBN 9789400963870.
  5. ↑ Sorg, Lisa. "N.C. astronomy institute aims to archive a treasure trove of celestial photos". Indy Week. Retrieved 2017-09-06.
  6. ↑ "Preserving the Astronomical Past — NOVA Next | PBS". NOVA Next. 2014-12-10. Retrieved 2017-09-06.
  7. ↑ Sowell, J. R.; Trippe, M.; Caballero-Nieves, S. M.; Houk, N. (2007-09-01). "H-R Diagrams Based on the HD Stars in the Michigan Spectral Catalogue and the Hipparcos Catalog". The Astronomical Journal. 134 (3): 1089–1102. Bibcode:2007AJ....134.1089S. doi:10.1086/520060. ISSN 0004-6256.
  8. ↑ Caballero-Nieves, S. M.; Sowell, J. R.; Houk, N. (2007-09-01). "Galactic Distributions and Statistics of the HD Stars in the Michigan Spectral Catalogue". The Astronomical Journal. 134 (3): 1072–1088. Bibcode:2007AJ....134.1072C. doi:10.1086/520059. ISSN 0004-6256.
  9. ↑ Murray, C. A.; Penston, M. J.; Binney, J. J.; Houk, N. (1997-08-01). "The Luminosity Function of Main Sequence Stars within 80 Parsecs". Hipparcos - Venice '97. 402: 485–488. Bibcode:1997ESASP.402..485M.
  10. ↑ Binney, J. J.; Dehnen, W.; Houk, N.; Murray, C. A.; Penston, M. J. (1997-08-01). "The Kinematics of Main Sequence Stars from HIPPARCOS Data". Hipparcos - Venice '97. 402: 473–478. Bibcode:1997ESASP.402..473B.
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