LP 261-75
low-mass star in the constellation Leo Minor
Facts
21 properties- Instance of
- low-mass star, double star, near-infrared source, astrophysical X-ray source, eclipsing binary[2][3][4][5]
- Age estimated by a dating method
- 0.15 gigaannum
- Catalog code
- UCAC2 44308174, LSPM J0951+3558, NLTT 22741, 2MASS J09510459+3558098, WDS J09511+3558A, Gaia DR2 796443724462555904, TOI-1779, Gaia DR3 796443724462555904, TIC 67646988[13][14][15][16][17][18][19][20][21]
- Child astronomical body
- 2MASS J09510549+3558021[11]
- Companion of
- 2MASS J09510549+3558021[12]
- Declination
- 35.96929494728 degree
- Declination component of proper motion
- -171.575 milliarcsecond per year
- Distance from Earth
- 33.995 parsec
- Effective temperature
- 3,692.03 kelvin
- Epoch
- J2000.0
- Imported from
- wholeness_audit_2026-05-02_v2
- Mass
- 0.22 solar mass
- Parallax
- 29.4158 milliarcsecond
- Radial velocity
- 10.2 kilometre per second
- Right ascension
- 147.76906488155 degree
- Right ascension component of proper motion
- -100.901 milliarcsecond per year
- Spectral class
- M5:[7]
- Type of variable star
- rotating variable star, eclipsing binary[22][23]
🏷️ Also known as
sv TOI‑1779
🔖 Identifiers · 3
- Gaia ID
- 796443724462555904
- NASA Exoplanet Archive ID
- LP 261-75 A
- SIMBAD ID
- LP 261-75
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Summary
LP 261-75 is a low-mass star[1].