Transits

Ronald L. Gilliland

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

Transits of the planets Mercury and especially Venus have been exciting events in the development of astronomy over the past few hundred years. Just two years ago the first transiting extra-solar planet, HD 209458b, was discovered, and subsequent studies during transit have contributed fundamental new knowledge. From the photometric light curve during transit one obtains a basic confirmation that the radial velocity detected object is indeed a planet by allowing precise determination of its mass and radius relative to these stellar quantities. From study of spectroscopic changes during transit it has been possible to probe for individual components of the transiting planets atmosphere. Planet transits are likely to become a primary tool for detection of new planets, especially other Earth-like planets with the Kepler Discovery Mission. Looking ahead, the additional aperture of the James Webb Space Telescope promises to allow the first possibility of studying the atmosphere of extra-solar Earth-analogue planets, perhaps even providing the first evidence of direct relevance to the search for signs of life on other planets. Transits in history Transits happen when an obscuring body passes in between us, the observers, and a background luminous source. Historically, both of the planets interior to Earth in the solar system have been observed while transiting the Sun. Mercury transits the Sun from our perspective frequently, Venus transits the Sun from the vantage point of the moving Earth only twice in every 130 years given current orbits.

Original languageEnglish (US)
Title of host publicationAstrophysics of Life
Subtitle of host publicationProceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland May 6-9, 2002
PublisherCambridge University Press
Pages35-40
Number of pages6
Volume9780521824903
ISBN (Electronic)9780511536113
ISBN (Print)0521824907, 9780521824903
DOIs
StatePublished - Jan 1 2005

Fingerprint

transit
planets
sun
Venus (planet)
Earth analogs
atmospheres
James Webb Space Telescope
extrasolar planets
astronomy
solar system
radial velocity
light curve
apertures
histories
orbits
radii
probes

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Gilliland, R. L. (2005). Transits. In Astrophysics of Life: Proceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland May 6-9, 2002 (Vol. 9780521824903, pp. 35-40). Cambridge University Press. https://doi.org/10.1017/CBO9780511536113.005
Gilliland, Ronald L. / Transits. Astrophysics of Life: Proceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland May 6-9, 2002. Vol. 9780521824903 Cambridge University Press, 2005. pp. 35-40
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Gilliland, RL 2005, Transits. in Astrophysics of Life: Proceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland May 6-9, 2002. vol. 9780521824903, Cambridge University Press, pp. 35-40. https://doi.org/10.1017/CBO9780511536113.005

Transits. / Gilliland, Ronald L.

Astrophysics of Life: Proceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland May 6-9, 2002. Vol. 9780521824903 Cambridge University Press, 2005. p. 35-40.

Research output: Chapter in Book/Report/Conference proceedingChapter

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Gilliland RL. Transits. In Astrophysics of Life: Proceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland May 6-9, 2002. Vol. 9780521824903. Cambridge University Press. 2005. p. 35-40 https://doi.org/10.1017/CBO9780511536113.005