 Context star field of EPIC 204376071 | |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Scorpius |
| Right ascension | 16h 04m 10.1267s[1] |
| Declination | −22° 34′ 45.5503″[1] |
| Characteristics | |
| Evolutionary stage | M[2] |
| Astrometry | |
| Proper motion (μ) | RA: -11.544[1] mas/yr Dec.: -24.892[1] mas/yr |
| Parallax (π) | 7.3908 ± 0.1944 mas[1] |
| Distance | 440 ± 10 ly (135 ± 4 pc) |
| Details | |
| Mass | 0.161±0.028[2][3] M☉ |
| Radius | 0.631±0.042[3] R☉ |
| Luminosity (bolometric) | 0.0273±0.0020[2] L☉ |
| Temperature | 2960±75[2] K |
| Rotation | 1.63 days[4] |
| Age | 10[5] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
EPIC 204376071 is an M-type star in the constellation of Scorpius. Parallax measurements by the Gaia space observatory put the star at a distance of about 440 light-years (130 parsecs) from Earth.[2][3][5] It is likely a member of the Upper Sco association, and is young enough that it has not yet become a main-sequence star.[2]
Unusual light fluctuations of the star, including up to an 80% dimming in brightness (i.e., "single 80% deep occultation of 1-day duration"), were observed by astronomers.[3][5] The unusual dimming was not only extremely deep, but also substantially asymmetric, with an egress about twice as long as the ingress.[4] Nonetheless, such an unusual dimming for EPIC 204376071 is much greater than the 22% dimming observed for Tabby's star.[6][7] Several explanations have been presented to explain the unusual dimming of the EPIC 204376071 star: one, orbiting dust or small particles; or two, a "transient accretion event of dusty material near the corotation radius of the star".[3] The unusual lightcurve of the star is similar to the lightcurve of a candidate exoplanet, KIC 10403228 b, which may have been caused by a "tilted ring system" orbiting the planet. In the case of EPIC 204376071, an orbiting brown dwarf or large planet, with a ring system, could cause a similar lightcurve, according to the researchers.[5]
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