Confirmed Exoplanet Discovered 2014

Kepler-260 c

A super-earth orbiting the g-type yellow (sun-like) Kepler-260, located approximately 2,046.2 light-years from Earth.

Key parameters at a glance

  • A radius of 1.74 Earth radii
  • A mass of 3.68 Earth masses
  • Surface gravity around 1.22 g
  • An orbital period of 76.050 days
  • Semi-major axis 0.3320 AU
  • Equilibrium temperature 372 K (99 °C)
  • Distance from Earth 2,046.19 light-years
  • Earth Similarity Index 0.724
  • Travel time at Voyager 1 speed 36,084,534 years

1 sibling around Kepler-260

Kepler-260 c shares its host star with 1 other confirmed planet. Side-by-side measurements below.

Planet Type Radius (R⊕) Mass (M⊕) Period (d) Eq. T (K) Year
Kepler-260 b Sub-Neptune 2.01 4.70 8.187 782 2014
Kepler-260 c this Super-Earth 1.74 3.68 76.050 372 2014

Kepler-260 c Planet Profile

Physical Specs

Radius
1.74 R⊕
Radius (Jupiter)
0.155 R♃
Mass
3.68 M⊕
Mass (Jupiter)
0.012 M♃
Density
3.84 g/cm³
Surface Gravity
1.22 g (Earth)

Classification

Planet Type

Super-Earth

ESI Score 0.724
HZ Position Inner
Controversial No

Discovery

Year 2014
Method Transit
Facility Kepler
Telescope 0.95 m Kepler Telescope

Size rank in cohort

Rank by radius

#344of 1176

top 29.2%

This planet

1.74R⊕

Super-Earth median

1.60R⊕

Nearest-size peers

Metric Earth Kepler-260 c Jupiter
Radius (R⊕)1.001.7411.21
Mass (M⊕)1.003.68317.83
Density (g/cm³)5.513.841.33
Surface Gravity (g)1.001.222.53
Insolation (S⊕)1.006.780.037

Star Catalogue Identifiers

TIC

TIC 137348863

Gaia DR2

Gaia DR2 2051907813786770688

Gaia DR3

Gaia DR3 2051907813786770688

System

Kepler-260

Percentile among Super-Earth cohort

Radius 1.740 R⊕ · percentile 70 / cohort 1176
Mass 3.680 M⊕ · percentile 64 / cohort 1176
Orbital period 76.05 d · percentile 98 / cohort 1164
Distance 627.37 pc · percentile 57 / cohort 1171
ESI 0.724 · percentile 86 / cohort 1176

Orbit & Habitability

Orbital Dynamics

Period
76.050 days
Semi-major axis
0.3320 AU
Eccentricity
0.000
Inclination
89.99 °

Year Length

A year here lasts approximately 76.05 Earth days (20.8% of a terrestrial year) on a nearly circular orbit at a mean orbital distance of 0.3320 AU.

Transit Fingerprint

Depth

0.039 %

Duration

6.826 h

Impact parameter b

0.660

Rp / R★

0.017771

Transit midpoint (BJD)

2,454,994.7121

Photometric dip

Transit produces a flux drop of 388 ppm lasting ≈ 6.83 h.

Extended Orbital Architecture

Planet / star radius ratio

0.017771

Semi-major axis / stellar radius

82.690

Impact parameter (b)

0.660

Transit mid-time (BJD)

2,454,994.7121

Angular separation (arcsec)

0.52900

Eq. Temperature

372K

(99 °C)

Insolation (S⊕)

6.78

Earth = 1.00

Earth Similarity (ESI)

0.724

0 = alien, 1 = Earth-identical

Inside the inner HZ boundary (too hot for liquid water) — liquid water is physically possible with adequate atmospheric pressure.

Discovery Paper

Primary reference

Rowe et al. 2014

Instrument

Kepler CCD Array

Publication

2014-03

Observation locale

Space

Host System: Kepler-260

Spectral Class

G-type yellow (Sun-like)

Effective Temperature

5,250 K — cooler than the Sun (5,778 K)

Estimated Age

1.15 Gyr — younger than the Sun (4.6 Gyr)

Stellar Radius

0.862 R☉

Stellar Mass

1.013 M☉

Metallicity [Fe/H]

0.29

Extended Stellar Properties

Surface gravity (log g)

4.494 dex

Stellar density

1.290 g/cm³

Metallicity ratio

[Fe/H]

Distance
627.37 parsec
Light-years 2,046.19 ly
V-band magnitude
14.25 mag
Voyager-speed travel 36,084,534 yr

Multi-band Host Photometry — 17 bands

9.016.416.43U14.65B14.25V14.12Gaia14.14Kepler13.61TESS14.91Sloan g14.84Sloan r14.12Sloan i14.08Sloan z12.90J12.54H12.49K12.41W112.49W212.48W39.05W4

Astrometric Data

Parallax

1.565 mas

Total Proper Motion

13.854 mas/yr

PM Right Ascension

-0.22 mas/yr

PM Declination

-13.85 mas/yr

Galactic Cartesian (pc)

x = 0.294 · y = -0.731 · z = 0.616

Equatorial (J2000)

RA 291.92597° · Dec 38.01405°

Galactic ℓ, b

70.788° · 9.807°

Ecliptic λ, β

304.651° · 58.844°

HTM-20 index

1973200587

Similar Worlds

Explore Related Categories