The NASA Exoplanet Archive is an online astronomical exoplanet and stellar catalog and data service that collates and cross-correlates astronomical data and information on exoplanets and their host stars and provides tools to work with these data. The Exoplanet Archive is dedicated to collecting and serving important public data sets involved in the search for and characterization of extrasolar planets and their host stars. The data include stellar parameters (such as positions, magnitudes, and temperatures), exoplanet parameters (such as masses and orbital parameters) and discovery/characterization data (such as published radial velocity curves, photometric light curves, images, and spectra).
All data in the Exoplanet Archive are vetted by a team of astronomers and are linked back to the original literature reference. Data are searchable either for an individual star or by stellar and planetary properties. The Exoplanet Archive offers direct access to frequently accessed data sets via an interactive table which allows sorting and filtering of the data. These data sets include:
Additionally, a breakdown of the exoplanet counts by discovery method is available on the Planet Counts page.
The NASA Exoplanet Archive includes several tools for working with exoplanet and stellar host data.
The Exoplanet Archive serves photometric time-series data from surveys that aim to discover transiting exoplanets, such as the Kepler Mission and CoRoT. The database provides access to over 700,000 light curves from space and ground-based exoplanet transit survey programs, including:
Please include the following standard acknowledgment in any published material that makes use of the NASA Exoplanet Archive's Services.
""This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program."
The Exoplanet Archive offers search and filtering capabilities for exolanets, Kepler candidates and time series data sets. All data in the Exoplanet Archive are vetted by a team of astronomers and are linked to the original literature references.
The Exoplanet Archive supports interactive visualization of images, spectra, and time series data. The Exoplanet Archive maintains its own stellar cross-identification to minimize ambiguity in multiple star components.
The Exoplanet Archive offers direct access to frequently accessed tables:
The Exoplanet Archive has a dedicated interface for transit survey data sets. The Exoplanet Archive also serves the public Kepler light curves. The Exoplanet Archive is the U.S. portal to the public CoRoT mission data for both the Exoplanet and Asteroseismology data sets. The Exoplanet Archive also serves ground-based transit survey data including the TrES observations of the Kepler field and KELT observations of the Praesepe field.
| Exoplanet Content | Stellar Parameters |
|---|---|
| Published parameters for known exoplanets | |
| Published Parameters | Published Parameters |
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| Predicted Parameters | Derived Parameters |
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| Associated Data | Associated Data |
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| Examples of Associated Data | |
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The transit survey data currently contained within the Exoplanet Archive include:
| Survey Region | Number of Objects | Time-Series Filter | Additional Static Filters | Time Span (days) | Number of Epochs | Number of Light Curves |
|---|---|---|---|---|---|---|
| XO | 2047 | W (XO) | JHK (2MASS) | 486 | < ~3500 | 2047 |
| HATNet | 2656 | I/R Cousins | JHK (2MASS), BV Johnson, I Cousins | 1996 | ~1100 - ~12000 | 6047 |
| Kepler Field | 195330 | CCD White light | g, r, i, z, J, H, & Ks | 682 | ~500 - ~50000 | 1064815 |
| CoRoT-Exoplanet | 96568 | CCD White light and 3 color Prism | B, V, R, & I | ~900 | 3400 – 396000 | 97971 |
| CoRoT-Seismology | 84 | CCD White light | V | ~900 | 68000 – 420000 | 85 |
| TrES-Lyr1 | 25947 | r, R | B, V | 75 | ~15000 | 25947 |
| KELT-Praesepe | 66637 | RK | 73 | ~3000 | 66637 | |
| NGC 2301 | 3961 | R | B, R | 14 | ~150 | 3961 |
| NGC 3201 | 58666 | V, I | V, I | 700 | ~120 | 58666 |
| M 10 | 43930 | V, I | V, I | 500 | ~50 | 43930 |
| M 12 | 32378 | V, I | V, I | 500 | ~50 | 32378 |