discov_num |
notes |
refcode |
DSG 2 |
Kepler 296 = KOI-1422. Derived properties for the A and B components |
|
|
are as follows: |
|
|
Teff (K) 3740 +/- 130 3440 +/- 75 |
|
|
Radius (Rsun) 0.480 +0.066/-0.087 0.322 +0.060/-0.068 |
|
|
Mass (Msun) 0.498 +0.067/-0.087 0.326 +0.070/-0.079 |
|
|
Using statistical and analytical arguments, Barclay et al. (2015) |
|
|
conclude that the five transiting planets associated with this pair |
|
|
orbit the primary star. The two outer planets (Ae and Af) have radii |
|
|
of 1.53 +/- 0.26 and 1.80 +/- 0.31 Rearth, respectively, and receive |
|
|
incident stellar fluxes of 1.40 +/- 0.23 and 0.62 +/- 0.10 times that |
|
|
received from the Sun by the Earth; this level of irradiation places |
|
|
both planets within or close to the circumstellar habitable zone of |
|
|
their parent star. |
Bcy2015 |
refcode |
metd |
author |
reference |
Bcy2015 |
Ag j |
Barclay, T., Quintana, E.V., Adams, F.C., Ciardi, D.R., Huber, D., |
2015ApJ...809....7B |
Bcy2015 |
|
Foreman-Mackey, D., Montet, B.T., & Caldwell, D. |
|
Bcy2015 |
|
ApJ 809, 7, 2015 |
|