EPIC 204278916

EPIC 204278916

Observation data ICRS )
Constellation	Scorpius
Right ascension	16h 02m 07.576s[1]
Declination	−22° 57′ 46.89″[1]
Characteristics
Evolutionary stage	Pre-main-sequence
Spectral type	M1[2]
Apparent magnitude (R)	13.7[3]
J−H color index	0.712
J−K color index	1.033
Distance		458 ± 4 ly (140 ± 1 pc)
Details
Myr
USNO -B1.0 0670-00406583, Gaia DR2 6243130106031671168
Database references
SIMBAD	data

EPIC 204278916 is a pre-main-sequence star, about five million years old with a spectral type of M1, implying a red dwarf. It is part of the Upper Scorpius sub-group of the Scorpius–Centaurus association, and is in the constellation Scorpius. The star is approximately the size of the Sun at 0.97 R_☉, but is only half its mass (0.50 M_☉) and a fraction of its luminosity (0.15 L_☉).^[5]

This stellar object was first characterized by the 2nd

space telescope's extended K2 mission Campaign 2 between 23 August and 13 November 2014.

Luminosity

In August 2016, a team of astronomers, led by Simone Scaringi of the Max Planck Institute for Extraterrestrial Physics in Germany, reported that this red dwarf star has a resolved circumstellar disc. Further, the research team observed unusual luminosity dimmings of up to 65% for 25 consecutive days (out of 79 total observation days). The variability in luminosity was highly periodic and attributed to stellar rotation. The researchers hypothesized that the irregular dimmings were caused by either a warped inner-disk edge or transiting cometary-like objects in either circular or eccentric orbits.^[5]

See also

• Disrupted planet
• List of stars that have unusual dimming periods

References

External links

• EPIC Catalog at MAST