Starspots, spin-orbit misalignment, and active latitudes in the HAT-P-11 exoplanetary system

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

ApJ, in press [9 pages]

Scientific paper

We present the analysis of 4 months of Kepler photometry of the K4V star HAT-P-11, including 26 transits of its "super-Neptune" planet. The transit data exhibit numerous anomalies that we interpret as passages of the planet over dark starspots. These spot-crossing anomalies preferentially occur at two specific phases of the transit. These phases can be understood as the intersection points between the transit chord and the active latitudes of the host star, where starspots are most abundant. Based on the measured characteristics of spot-crossing anomalies, and previous observations of the Rossiter-McLaughlin effect, we find two solutions for the stellar obliquity (psi) and active latitude (l): either psi = 106 and l = 19.7, or psi = 97 and l = 67 (all in degrees). If the active latitude changes with time in analogy with the "butterfly diagram" of the Sun's activity cycle, future observations should reveal changes in the preferred phases of spot-crossing anomalies.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Starspots, spin-orbit misalignment, and active latitudes in the HAT-P-11 exoplanetary system does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Starspots, spin-orbit misalignment, and active latitudes in the HAT-P-11 exoplanetary system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Starspots, spin-orbit misalignment, and active latitudes in the HAT-P-11 exoplanetary system will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-223992

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.