Published in

Cambridge University Press, Proceedings of the International Astronomical Union, S299(8), p. 391-392, 2013

DOI: 10.1017/s1743921313009058

Links

Tools

Export citation

Search in Google Scholar

A Hot Jupiter in a Nearly Polar Orbit

This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

Full text: Download

Green circle
Preprint: archiving allowed
Red circle
Postprint: archiving forbidden
Red circle
Published version: archiving forbidden
Data provided by SHERPA/RoMEO

Abstract

AbstractWe measured the spin-orbit misalignment for WASP-79b, a transiting hot Jupiter from the WASP survey. Using the Rossiter-McLaughlin effect during the transit event, we determined the sky-projected obliquity to be λ = −106+10−8○. This result indicates that the planet is in a nearly polar orbit.