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HAT-P-67
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Star HAT-P-67

Subgiant HAT-P-67 is located 1214 light years away from the Sun. It is a single star of spectral class F5IV, that has 164 % of solar mass. There is at least one exoplanet in this system.
Sun distance
1214 light years

HAT-P-67

Subgiant (spectral class F5IV)

Location

Ascension iconRight ascension: 17h 6m 26.579s
Declination iconDeclination: 44° 46' 36.776'' (northern hemisphere)
Parallax iconParallax: 2.687
Distance iconSun distance: 1213.86 ly | 372.2 pc

Basic characteristic

icon weight
Mass: 164.2 % M Sun | 1720 M Jupiter
radius icon
Size: 265 % R Sun | 26.4 R Jupiter
temperature iconTemperature: 6406 K | 1.11 T Sun

1 exoplanet

HAT-P-67 b 0.06 AU 101.7 M 23.5 R 4.8 days

Photometry

Magnitude iconApparent magnitude (V): 10.1
Magnitude iconAbsolute magnitude (V): 2.3
5
10
15
20
25
30
35
K
2.1
H
1.6
J
1.2
Grp
0.8
I
0.8
G
0.6
V
0.5
Gbp
0.5
B
0.4
U
0.3
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
More about HAT-P-67
Star HAT-P-67 is is approximately 3 times bigger than the Sun and temperature on its surface is around 6406 K (6133 °C), which is about 111 % of Sun's temperature.
       HAT-P-67 can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia. 
Other designations of this star
Gaia DR3 1358614983131339392
External sources
gaia icon
Gaia database (Gaia DR3 1358614983131339392)
Archive from the Gaia mission
tess icon
TESS database (TOI 2014.01)
Archive from the TESS mission
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
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