Illustration of a star with several orbiting exoplanets of different sizes, one transiting in front of the star

Exoplanet Archive

Search and filter every confirmed exoplanet in NASA's Exoplanet Archive — refreshed daily from the source. Sort by distance, radius, or mass to explore what's out there.

Host star statistics: how many stars, planets per system →

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16 planets found — page 1 of 1.

Planet Host star Method Year Radius (R⊕) Mass (M⊕) Distance (pc)
Kepler-80 g Kepler-80 Transit 2017 1.13 369.5
Kepler-80 f Kepler-80 Transit 2016 1.21 369.5
Kepler-800 b Kepler-800 Transit 2016 2.85 1019.3
Kepler-801 b Kepler-801 Transit 2016 2.00 440.4
Kepler-802 b Kepler-802 Transit 2016 3.54 780.6
Kepler-803 b Kepler-803 Transit 2016 3.79 639.8
Kepler-804 b Kepler-804 Transit 2016 1.94 649.6
Kepler-804 c Kepler-804 Transit 2016 1.14 649.6
Kepler-805 b Kepler-805 Transit 2016 2.89 638.5
Kepler-806 b Kepler-806 Transit 2016 1.14 361.9
Kepler-808 b Kepler-808 Transit 2016 1.46
Kepler-809 b Kepler-809 Transit 2016 3.01 961.4
Kepler-80 d Kepler-80 Transit 2014 1.53 6.75 369.5
Kepler-80 e Kepler-80 Transit 2014 1.60 4.13 369.5
Kepler-80 b Kepler-80 Transit 2012 2.67 6.93 369.5
Kepler-80 c Kepler-80 Transit 2012 2.74 6.74 369.5

ℹ️ About this data
  • Sourced from NASA's Exoplanet Archive (Caltech/IPAC), refreshed daily. Only confirmed planets are included — candidates awaiting confirmation aren't in this list.
  • A blank field means that measurement hasn't been published for that planet — not every planet has a known mass, for instance, especially ones found only by the transit method (which measures radius directly, but needs a separate technique like radial velocity to get mass).
📏 Units and symbols legend
Symbol Means In metric
R⊕Earth radii — planet size relative to Earth (Earth = 1)1 R⊕ ≈ 6,371 km
M⊕Earth masses — planet mass relative to Earth (Earth = 1)1 M⊕ ≈ 5.972 × 10²⁴ kg
R☉Solar radii — host star size relative to the Sun (Sun = 1)1 R☉ ≈ 696,000 km
M☉Solar masses — host star mass relative to the Sun (Sun = 1)1 M☉ ≈ 1.989 × 10³⁰ kg
KKelvin — temperature (star surface or planet equilibrium)°C = K − 273.15 (shown alongside on each planet's page)
pcParsecs — distance from Earth1 pc ≈ 3.086 × 10¹³ km ≈ 3.26 light-years
daysOrbital period — time for one full orbit around the host star, always in Earth days regardless of the planetEarth's own orbital period is 365.25 days — divide by that to get Earth years
RA / DecRight ascension / declination — the star's position on the skyBoth in degrees — the sky's equivalent of longitude/latitude
EccentricityHow elongated the orbit isUnitless: 0 = perfect circle, closer to 1 = more elongated ellipse

Astronomy uses Earth/Sun/Jupiter as yardsticks instead of kg or km because the numbers involved (10²⁴–10³⁰) are unwieldy otherwise — for scale, a gas giant like Jupiter is about 11 R⊕ and 318 M⊕.

💻 Show API usage example (cURL)
curl -sS "https://devops.majbase.com/exoplanets/api?q=kepler&method=Transit&sort=distance&page=1"

Returns {"rows": [...], "total", "page", "pages"}, or {"error": "..."} if temporarily unavailable. All query params are optional.