Confirmed Exoplanet Discovered 2015

K2-10 b

A sub-neptune orbiting the f-type yellow-white K2-10, located approximately 888.3 light-years from Earth.

Key parameters at a glance

  • A radius of 3.77 Earth radii
  • A mass of 25.20 Earth masses
  • Surface gravity around 1.77 g
  • An orbital period of 19.306 days
  • Semi-major axis 0.1370 AU
  • Equilibrium temperature 649 K (376 °C)
  • Distance from Earth 888.32 light-years
  • Earth Similarity Index 0.353
  • Travel time at Voyager 1 speed 15,665,496 years

K2-10 b Planet Profile

Physical Specs

Radius
3.77 R⊕
Radius (Jupiter)
0.337 R♃
Mass
25.20 M⊕
Mass (Jupiter)
0.079 M♃
Density
2.36 g/cm³
Surface Gravity
1.77 g (Earth)

Classification

Planet Type

Sub-Neptune

ESI Score 0.353
HZ Position Inner
Controversial No

Discovery

Year 2015
Method Transit
Facility K2
Telescope 0.95 m Kepler Telescope

Size rank in cohort

Rank by radius

#62of 1978

top 3.1%

This planet

3.77R⊕

Sub-Neptune median

2.71R⊕

Nearest-size peers

Metric Earth K2-10 b Jupiter
Radius (R⊕)1.003.7711.21
Mass (M⊕)1.0025.20317.83
Density (g/cm³)5.512.361.33
Surface Gravity (g)1.001.772.53
Insolation (S⊕)1.0042.100.037

Alternative Mass Estimates

Method Value Interpretation
Best measured mass 25.200 M⊕ Direct mass measurement (not derived).

Star Catalogue Identifiers

TIC

TIC 363573185

Gaia DR2

Gaia DR2 3798690151434945280

Gaia DR3

Gaia DR3 3798690151434945280

System

K2-10

Percentile among Sub-Neptune cohort

Radius 3.773 R⊕ · percentile 97 / cohort 1978
Mass 25.200 M⊕ · percentile 96 / cohort 1978
Orbital period 19.31 d · percentile 61 / cohort 1946
Distance 272.36 pc · percentile 33 / cohort 1975
ESI 0.353 · percentile 41 / cohort 1978

Orbit & Habitability

Orbital Dynamics

Period
19.306 days
Semi-major axis
0.1370 AU
Eccentricity
0.310
Inclination
89.50 °

Year Length

A year here lasts approximately 19.31 Earth days (5.3% of a terrestrial year) on a highly eccentric trajectory at a mean orbital distance of 0.1370 AU.

Transit Fingerprint

Depth

0.169 %

Duration

3.806 h

Impact parameter b

0.400

Rp / R★

0.037959

Transit midpoint (BJD)

2,456,819.5794

Photometric dip

Transit produces a flux drop of 1,691 ppm lasting ≈ 3.81 h.

Extended Orbital Architecture

Planet / star radius ratio

0.037959

Semi-major axis / stellar radius

28.700

Impact parameter (b)

0.400

RV semi-amplitude (K)

7.300 m/s

Transit mid-time (BJD)

2,456,819.5794

Angular separation (arcsec)

0.50300

Eq. Temperature

649K

(376 °C)

Insolation (S⊕)

42.10

Earth = 1.00

Earth Similarity (ESI)

0.353

0 = alien, 1 = Earth-identical

Inside the inner HZ boundary (too hot for liquid water) — the surface is too hot to retain surface water.

Detection Signatures

Transit photometry

A transit dip has been observed from at least one telescope.

Radial velocity

Stellar wobble has been measured spectroscopically.

Discovery Paper

Primary reference

Montet et al. 2015

Instrument

Kepler CCD Array

Publication

2015-08

Observation locale

Space

Host System: K2-10

Spectral Class

F-type yellow-white

Effective Temperature

5,533 K — cooler than the Sun (5,778 K)

Estimated Age

Stellar Radius

0.956 R☉

Stellar Mass

0.880 M☉

Metallicity [Fe/H]

-0.07

Extended Stellar Properties

Surface gravity (log g)

4.470 dex

Stellar density

1.508 g/cm³

Systemic radial velocity

8.20 km/s

Rotational v·sin i

1.50 km/s

Activity index (log R'HK)

-5.093

Metallicity ratio

[Fe/H]

Distance
272.36 parsec
Light-years 888.32 ly
V-band magnitude
12.43 mag
Voyager-speed travel 15,665,496 yr

Multi-band Host Photometry — 17 bands

8.914.614.60U13.12B12.43V12.22Gaia12.30Kepler11.74TESS12.91Sloan g13.57Sloan r12.21Sloan i12.53Sloan z11.06J10.75H10.65K10.64W110.69W210.55W38.92W4

Astrometric Data

Parallax

3.643 mas

Total Proper Motion

72.641 mas/yr

PM Right Ascension

-72.60 mas/yr

PM Declination

-2.51 mas/yr

Galactic Cartesian (pc)

x = -0.990 · y = 0.137 · z = 0.030

Equatorial (J2000)

RA 172.12165° · Dec 1.69062°

Galactic ℓ, b

261.428° · 57.717°

Ecliptic λ, β

172.093° · -1.572°

HTM-20 index

-214034828

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