K-type star · orange dwarf

HR 6857

HR 6857 is an orange dwarf in the constellation Ophiuchus 153 ly from Earth. Its surface is about 4,550 K, about 0.8 times the Sun's surface temperature, and it shines at 13.07× the Sun's brightness. At magnitude 5.4 it is bright enough to see with the naked eye; the light you see left it 153 years ago.

153 lybrightness mag 5.41K2III

Also catalogued as HD 168387 · HIP 89772

4,550 K
temperature
5.41
apparent magnitude
13.07× ☉
luminosity vs Sun
K2III
spectral type
Distance & comparison with our Sun
153 years
at light speed from Earth
0.79×
as hot as the Sun
13.07×
the Sun's light output
2.06
absolute magnitude
Explore from here · roam the neighborhood
Can you see it tonight?
VISIBLE TO THE NAKED EYE
Brightness mag 5.4To see it no equipment neededLook toward Ophiuchus

Star data from the HYG database v4.2 (Astronexus, CC BY-SA 4.0). Temperature and colour computed by gravityfinder from the B-V colour index; the illustration is generated from that temperature, not a photograph.