K2-72
Sign in to saveK2-72 (also designated EPIC 206209135) is a cool red dwarf star of spectral class M2V located about away from the Earth in the constellation of Aquarius. It is known to host four planets, all similar in size to Earth, with one of them residing within the habitable zone.
In the Vinony graph
Vinony's link graph records 294 inbound references to K2-72, and connects out to list of stars in Aquarius, list of planet types and year.
It sits within the topics Aquarius (constellation), M-type main-sequence stars and Planetary systems with four confirmed planets.
Vinony links it to 11 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- LM*
- Spectral type
- M2V
- Distance
- 217 light-years
- Redshift
- z = -0.00013213035214920676
- Coordinates
- RA 334.6219° · Dec -9.6123°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Constellation
- Aquarius
- Distance from Earth
- 66.513
- Radius
- 0.33
- Mass
- 0.27
Show 14 more facts
- effective temperature
- 3360.47
- parallax
- 15.0346
- apparent magnitude
- 14.257562
- radial velocity
- -39.6143
- epoch
- J2000.0
- catalog code
- EPIC 206209135
- spectral class
- M2V
- surface gravity
- 151080
- right ascension component of proper motion
- 195.834
- declination component of proper motion
- 74.259
- right ascension
- 334.62189522828
- declination
- -9.61232808001
- stellar rotational velocity
- 6.071
- metallicity
- -0.738
via Wikidata · CC0
~3 min read
Encyclopedic overview
4 sectionsContents
- Nomenclature and history
- Stellar characteristics
- Planetary system
- References
K2-72 (also designated EPIC 206209135) is a cool red dwarf star of spectral class M2V located about away from the Earth in the constellation of Aquarius. It is known to host four planets, all similar in size to Earth, with one of them residing within the habitable zone.
==Nomenclature and history== K2-72 also has the 2MASS catalogue number J22182923-0936444. Its EPIC (Ecliptic Plane Input Catalog) number is 206209135.
Excerpted from Wikipedia’s “K2-72” article, available under the CC BY-SA 4.0 licence.