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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How each one was found: the 11 detection methods →
4709 planets found — page 95 of 95.
| Planet |
Host star |
Method |
Year |
Radius (R⊕) |
Mass (M⊕) |
Distance (pc) |
| SWEEPS-4 b |
SWEEPS-4 |
Transit |
2006 |
9.08 |
1207.70 |
— |
| TrES-2 b |
TrES-2 |
Transit |
2006 |
15.24 |
473.57 |
215.3 |
| XO-1 b |
XO-1 |
Transit |
2006 |
12.78 |
263.80 |
163.6 |
| OGLE-TR-10 b |
OGLE-TR-10 |
Transit |
2004 |
14.01 |
197.05 |
1345.0 |
| OGLE-TR-111 b |
OGLE-TR-111 |
Transit |
2004 |
11.42 |
— |
1068.3 |
| OGLE-TR-113 b |
OGLE-TR-113 |
Transit |
2004 |
12.25 |
400.45 |
566.5 |
| OGLE-TR-132 b |
OGLE-TR-132 |
Transit |
2004 |
13.45 |
375.02 |
2012.6 |
| TrES-1 b |
TrES-1 |
Transit |
2004 |
12.67 |
266.98 |
159.7 |
| OGLE-TR-56 b |
OGLE-TR-56 |
Transit |
2002 |
15.28 |
441.77 |
— |
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 |
| K | Kelvin — temperature (star surface or planet equilibrium) | °C = K − 273.15 (shown alongside on each planet's page) |
| pc | Parsecs — distance from Earth | 1 pc ≈ 3.086 × 10¹³ km ≈ 3.26 light-years |
| days | Orbital period — time for one full orbit around the host star, always in Earth days regardless of the planet | Earth's own orbital period is 365.25 days — divide by that to get Earth years |
| RA / Dec | Right ascension / declination — the star's position on the sky | Both in degrees — the sky's equivalent of longitude/latitude |
| Eccentricity | How elongated the orbit is | Unitless: 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.
