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 →  ·  How each one was found: the 11 detection methods →

6451 planets found — page 28 of 130.

Planet Host star Method Year Radius (R⊕) Mass (M⊕) Distance (pc)
K2-384 e K2-384 Transit 2022 1.34 — 82.7
K2-384 f K2-384 Transit 2022 2.22 — 82.7
K2-385 b K2-385 Transit 2022 1.54 — 420.8
K2-386 b K2-386 Transit 2022 2.32 — 428.8
K2-387 b K2-387 Transit 2022 7.32 — 266.3
K2-388 b K2-388 Transit 2022 3.90 — 290.5
K2-389 b K2-389 Transit 2022 2.33 — 259.2
K2-389 c K2-389 Transit 2022 2.04 — 259.2
K2-390 b K2-390 Transit 2022 4.66 — 456.1
K2-391 b K2-391 Transit 2022 1.37 — 507.9
K2-392 b K2-392 Transit 2022 1.85 — 407.0
K2-393 b K2-393 Transit 2022 2.35 — 265.9
K2-394 b K2-394 Transit 2022 1.69 — 98.0
K2-395 b K2-395 Transit 2022 2.60 — 286.7
K2-395 c K2-395 Transit 2022 3.40 — 286.7
K2-396 b K2-396 Transit 2022 1.58 — 274.9
K2-396 c K2-396 Transit 2022 3.12 — 274.9
K2-397 b K2-397 Transit 2022 2.42 — 199.4
K2-398 b K2-398 Transit 2022 2.27 — 607.0
K2-398 c K2-398 Transit 2022 5.10 — 607.0
K2-400 b K2-400 Transit 2022 1.16 — 62.4
K2-401 b K2-401 Transit 2022 2.26 — 200.7
K2-402 b K2-402 Transit 2022 2.68 — 523.1
K2-403 b K2-403 Transit 2022 5.33 — 246.6
K2-404 b K2-404 Transit 2022 2.53 — 121.6
K2-405 b K2-405 Transit 2022 4.57 — 197.2
K2-406 b K2-406 Transit 2022 4.60 — 85.4
K2-407 b K2-407 Transit 2022 1.28 — 218.4
K2-407 c K2-407 Transit 2022 1.36 — 218.4
K2-408 b K2-408 Transit 2022 1.68 — 162.3
K2-409 b K2-409 Transit 2022 2.48 — 431.0
K2-411 b K2-411 Transit 2022 0.99 — 298.2
K2-412 b K2-412 Transit 2022 2.12 — 654.1
K2-413 b K2-413 Transit 2022 0.76 — 285.2
K2-413 c K2-413 Transit 2022 1.23 — 285.2
K2-414 b K2-414 Transit 2022 1.22 — 260.0
K2-414 c K2-414 Transit 2022 1.93 — 260.0
K2-99 c K2-99 Radial Velocity 2022 — 2669.76 519.2
KIC 3526061 b KIC 3526061 Radial Velocity 2022 — 5768.59 401.2
KMT-2017-BLG-0673L b KMT-2017-BLG-0673L Microlensing 2022 — 1166.43 5080.0
KMT-2018-BLG-0030L b KMT-2018-BLG-0030L Microlensing 2022 — 460.85 6480.0
KMT-2018-BLG-0087L b KMT-2018-BLG-0087L Microlensing 2022 — 73.10 7020.0
KMT-2018-BLG-0247L b KMT-2018-BLG-0247L Microlensing 2022 — 670.62 6760.0
KMT-2018-BLG-1988L b KMT-2018-BLG-1988L Microlensing 2022 — 5.56 4150.0
KMT-2018-BLG-2602L b KMT-2018-BLG-2602L Microlensing 2022 — 365.50 4310.0
KMT-2019-BLG-0253L b KMT-2019-BLG-0253L Microlensing 2022 — 9.20 4900.0
KMT-2019-BLG-0414L b KMT-2019-BLG-0414L Microlensing 2022 — 1452.48 4410.0
KMT-2019-BLG-0953L b KMT-2019-BLG-0953L Microlensing 2022 — 15.50 7200.0
KMT-2019-BLG-1042L b KMT-2019-BLG-1042L Microlensing 2022 — 60.39 6600.0
KMT-2019-BLG-1552L b KMT-2019-BLG-1552L Microlensing 2022 — 1287.21 4600.0
← Previous Page 28 of 130 Next →

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.