Name | Kepler-1708 | ||
Distance | 1667.0 ( -91.0 +102.0 ) pc | ![]() |
|
Spectral type | — | ||
Apparent magnitude V | 16.0 | ||
Mass | 1.088 (± 0.072) MSun | ![]() |
|
Age | 3.16 (± 2.26) Gyr | ![]() |
|
Effective temperature | 6157.0 ( -202.0 +231.0 ) K | ![]() |
|
Radius | 1.117 (± 0.064) RSun | ![]() |
|
Metallicity [Fe/H] | 0.0 | ![]() |
|
Detected Disc | — | ||
Magnetic Field | — | ||
RA2000 | 19:47:18.0 | ||
Dec2000 | +43:37:29 | ||
Alternate Names | |||
Planetary system | 2 planets |
An Exomoon Survey of 70 Cool Giant Exoplanets and the New Candidate Kepler-1708 b-i
2022
KIPPING D., BRYSON S., BURKE Ch., CHRISTIANSEN J., HARDEGREE-ULLMAN K. et al.
Nature Astronomy, in press
paper arxiv
Probing Planets with Exomoons: The Cases of Kepler-1708 b and Kepler-1625 b
2022
TOKADJIAN A. & PIRO A.
ApJ. Letters, 929, L2
paper arxiv
Kepler-1708 b-i is likely undetectable with HST
2022
CASSESE B. & KIPPING D.
MNRAS, submitted
arxiv