(Q17631429)

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

Transit-timing variations in the system Kepler-410Ab

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

unconfirmed exoplanet

2 references

SIMBAD

Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months)

1 reference

HD 175289b

Henry Draper Catalogue

1 reference

SIMBAD

KOI-42b

Kepler object of interest

2 references

TOI-4589b

TESS Object of Interest

1 reference

Kepler-410 Ab

Kepler Confirmed Names

2 references

KOI-42.01

Kepler object of interest

2 references

TOI-4589.01

imported from Wikimedia project

TESS Object of Interest

1 reference

TIC 164458714b

1 reference

discoverer or inventor

Kepler

1 reference

Spanish Wikipedia

time of discovery or invention

2013

1 reference

February 2014

1 reference

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

2 references

inferred from equatorial coordinates

constellation

Lyra

1 reference

based on heuristic

parent astronomical body

3 references

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

object stated in reference as

Kepler-410 A

object stated in reference as

Kepler-410 A

argument of periapsis

270 degree

1 reference

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

orbital eccentricity

0.17±0.32

1 reference

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

0.17±0.1

1 reference

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

orbital inclination

87.744±0.003 degree

1 reference

Transit-timing variations in the system Kepler-410Ab

87.72±0.15 degree

1 reference

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

orbital period

17.83365704±0.00000224 day

1 reference

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

17.83368211±0.0000115 day

1 reference

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

17.8336313±0.0000043 day

1 reference

Transit-timing variations in the system Kepler-410Ab

17.833648±0.000054 day

1 reference

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

semi-major axis of an orbit

0.1226±0.0047 astronomical unit

2 references

Transit-timing variations in the system Kepler-410Ab

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

declination component of proper motion

parallax

6.7495±0.0224 milliarcsecond

2 references

61.846±0.048 milliarcsecond per year

2 references

right ascension component of proper motion

61.515±0.042 milliarcsecond per year

2 references

2.5±0.05 Earth radius

1 reference

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

2.647±0.02 Earth radius

1 reference

Transit-timing variations in the system Kepler-410Ab

2.742±0.117 Earth radius

1 reference

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

0.253±0.005 Jupiter radius

1 reference

What asteroseismology can do for exoplanets: Kepler-410A b is a small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

diameter

34,600±497 kilometre

1 reference

Fundamental properties of Kepler planet-candidate host stars using asteroseismology

3 references