Detection of the Rossiter-McLaughlin effect in the 2012 june 6 venus transit

P. Molaro, L. Monaco, M. Barbieri, S. Zaggia

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

Eclipsing bodies on stars produce radial velocity variations on the photospheric stellar lines known as the Rossiter-McLaughlin (RM) effect. The body occults a small area of the stellar disc and, due to the rotation of the star, the stellar line profiles are distorted according to the projected location of the body on to the stellar disc. The effect originally observed in eclipsing binaries was also shown to be produced by extrasolar planets transits. Here we report the detection of the RM effect in the Sun due to the Venus transit of 2012 June 6. We used the integrated sunlight as reflected by the Moon at night time to record part of the transit by means of the high-precision HARPS spectrograph at the 3.6-m La Silla European Southern Observatory (ESO) telescope. The observations show that the partial Venus eclipse of the solar disc in correspondence of the passage in front of the receding hemisphere produced a modulation in the radial velocity with a negative amplitude of ≈-1 m s-1, in agreement with the theoretical model. The radial velocity change is comparable to the solar jitter and more than a factor of 2 smaller than previously detected in extrasolar hot Neptunes. This detection, facilitated by an amplification factor of 3.5 of the Venus radius due to proximity, anticipates the study of transits of Earth-size bodies in solar-type stars by means of a high-resolution spectrograph attached to a 40-m class telescope.

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume429
Issue number1
DOIs
Publication statusPublished - 2013

Fingerprint

Venus (planet)
transit
Venus
radial velocity
stars
spectrographs
sun
Neptune
telescopes
Neptune (planet)
Moon
body size
amplification
eclipses
extrasolar planets
sunlight
planet
observatory
moon
European Southern Observatory

Keywords

  • Planets and satellites:General
  • Planets and satellites:Individual:Venus
  • Sun:General
  • Sun:Oscillations
  • Techniques:Radial velocities

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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title = "Detection of the Rossiter-McLaughlin effect in the 2012 june 6 venus transit",
abstract = "Eclipsing bodies on stars produce radial velocity variations on the photospheric stellar lines known as the Rossiter-McLaughlin (RM) effect. The body occults a small area of the stellar disc and, due to the rotation of the star, the stellar line profiles are distorted according to the projected location of the body on to the stellar disc. The effect originally observed in eclipsing binaries was also shown to be produced by extrasolar planets transits. Here we report the detection of the RM effect in the Sun due to the Venus transit of 2012 June 6. We used the integrated sunlight as reflected by the Moon at night time to record part of the transit by means of the high-precision HARPS spectrograph at the 3.6-m La Silla European Southern Observatory (ESO) telescope. The observations show that the partial Venus eclipse of the solar disc in correspondence of the passage in front of the receding hemisphere produced a modulation in the radial velocity with a negative amplitude of ≈-1 m s-1, in agreement with the theoretical model. The radial velocity change is comparable to the solar jitter and more than a factor of 2 smaller than previously detected in extrasolar hot Neptunes. This detection, facilitated by an amplification factor of 3.5 of the Venus radius due to proximity, anticipates the study of transits of Earth-size bodies in solar-type stars by means of a high-resolution spectrograph attached to a 40-m class telescope.",
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Detection of the Rossiter-McLaughlin effect in the 2012 june 6 venus transit. / Molaro, P.; Monaco, L.; Barbieri, M.; Zaggia, S.

In: Monthly Notices of the Royal Astronomical Society: Letters, Vol. 429, No. 1, 2013.

Research output: Contribution to journalArticle

TY - JOUR

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AU - Monaco, L.

AU - Barbieri, M.

AU - Zaggia, S.

PY - 2013

Y1 - 2013

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AB - Eclipsing bodies on stars produce radial velocity variations on the photospheric stellar lines known as the Rossiter-McLaughlin (RM) effect. The body occults a small area of the stellar disc and, due to the rotation of the star, the stellar line profiles are distorted according to the projected location of the body on to the stellar disc. The effect originally observed in eclipsing binaries was also shown to be produced by extrasolar planets transits. Here we report the detection of the RM effect in the Sun due to the Venus transit of 2012 June 6. We used the integrated sunlight as reflected by the Moon at night time to record part of the transit by means of the high-precision HARPS spectrograph at the 3.6-m La Silla European Southern Observatory (ESO) telescope. The observations show that the partial Venus eclipse of the solar disc in correspondence of the passage in front of the receding hemisphere produced a modulation in the radial velocity with a negative amplitude of ≈-1 m s-1, in agreement with the theoretical model. The radial velocity change is comparable to the solar jitter and more than a factor of 2 smaller than previously detected in extrasolar hot Neptunes. This detection, facilitated by an amplification factor of 3.5 of the Venus radius due to proximity, anticipates the study of transits of Earth-size bodies in solar-type stars by means of a high-resolution spectrograph attached to a 40-m class telescope.

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