Kepler-37 d
Sign in to saveKepler-37d is an exoplanet discovered by the Kepler space telescope in February 2013. It is located 209 light years away, in the constellation Lyra. With an orbital period of 39.8 days, it is the largest of the three known planets orbiting its parent star Kepler-37.
In the Vinony graph
Within Vinony's link graph, Kepler-37 d is referenced by 199 other articles, and connects out to list of planet types, outer space and kelvin.
It is catalogued under topics including Exoplanets discovered by the Kepler space telescope, Exoplanets discovered in 2013 and Kepler-37.
Its subject is documented across 14 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- Pl
- Distance
- 209 light-years
- Coordinates
- RA 284.0596° · Dec 44.5182°
via SIMBAD · CDS Strasbourg
Key facts
- Planet.name
- Kepler-37d
- Planet.discovery_site
- Kepler space telescope
- Planet.discovered
- 2013
- Planet.discovery_method
- Transit
- Planet.apsis
- astron
- Planet.eccentricity
- <0.10
- Planet.star
- Kepler-37
- Planet.mass
- or
- Planet.density
- or
- Planet.single_temperature
- (, equilibrium)
via Wikipedia infobox
Exoplanet data
- Host star
- Kepler-37
- Discovered
- 2013
- Discovered by
- Kepler
- Orbital period
- 39.79 days
- Radius
- 2.03 × Earth
- Mass
- 2 × Earth
- Equilibrium temp
- 499 K
- Distance
- 63.92 pc
via NASA Exoplanet Archive
Wikidata facts
- Diameter
- 4540
- Radius
- 0.173
- Mass
- 0.017
- Orbital period
- 39.7922
Show 11 more facts
- catalog code
- Kepler-37d
- time of discovery or invention
- 2013-02-00
- right ascension
- 284.05961573573080
- declination
- 44.51816367760333
- orbital inclination
- 89.335
- semi-major axis of an orbit
- 0.2109
- orbital eccentricity
- 0
- right ascension component of proper motion
- -60.520
- declination component of proper motion
- 48.694
- parallax
- 15.6155
- Commons category
- Kepler-37 d
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
3 sectionsContents
- Host star
- See also
- References
Kepler-37d is an exoplanet discovered by the Kepler space telescope in February 2013. It is located 209 light years away, in the constellation Lyra. With an orbital period of 39.8 days, it is the largest of the three known planets orbiting its parent star Kepler-37.
A 2021 study detected Kepler-37d via radial velocity, finding a mass of about , but a 2023 study instead found an upper limit on its mass of only . In either case, it is not a rocky planet, but a low-density planet rich in volatiles.
Excerpted from Wikipedia’s “Kepler-37 d” article, available under the CC BY-SA 4.0 licence.