This is the spectroscopic transit of a #planet with an orbital period of 1.5 YEARS !! #HIP41378 ๐ช
In case you missed the great paper led by @sgrouffal (#ProudAdvisor), arXived over the summer, here is a recap'.
The planet HIP41378 f is a Saturn-sized transiting planet with an orbital period of 542 days. It means we can observe its transit only once every 1.5 years - it's actually once every 3 years from the ground as the host star is too close to the Sun (as seen from the Earth) every other transits.
With such a long orbital period and a nearly circular orbit, the transit event lasts 19 hours (!). Hence, from the ground, any observer could only observe a tiny fraction of the transit. To overcome this issue, back in 2022, we set up a worldwide collaboration of almost all high-resolution radial-velocity spectrographs across the globe. Over the same night, all the instruments observed the target HIP41378 at the time of planet'f transit, allowing us to detect the Rossiter-McLaughlin (RM) effect.
The RM effect is measuring the planet's orbital obliquity, i.e. the angle between the orbital plane and the spin axis of the star. While this angle is ~0ยบ in the solar system, for HIP41378 it reaches ฮจ=~52ยบ.
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#Science #Space #Exoplanet #Astrophysics #Astronomy #telescope



