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Star HD 3638

Red giant HD 3638 is located 727 light years away from the Sun. It is a single star of spectral class M0 III, that has 114 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
727 light years

HD 3638

Spectral class: M0 III

Location +

Ascension iconRight ascension: 0h 39m 34.605s
Declination iconDeclination: 49° 34' 23.866'' (northern hemisphere)
Parallax iconParallax: 4.484
Distance iconSun distance: 727.398 ly | 223.0 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 114 % M Sun
| 1194 M Jupiter
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Star mass
Mass of the star HD 3638 is 1.14 solar masses.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
radius icon
Size: 3840 % R Sun
| 382.1 R Jupiter
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Star size
Radius of the star HD 3638 is 38.4 solar radii.

The size of a star refers to its radius — the distance from its center to its surface. Star size is usually measured in solar radii (R☉), where 1 solar radius equals approximately 696,000 kilometers. Depending on their type and life stage, stars can be much smaller or larger than the Sun... icon More about Star size in StellarGuide
temperature icon
Temperature: 3940 K | 0.68 T Sun
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Star temperature
Surface temperature of HD 3638 is 3940 K, which is 68 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide
luminosity icon
Luminosity: 388.28 L Sun
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Star luminosity
Luminosity is the total amount of energy a star gives off every second. Think of it as the star’s true brightness — not just how bright it looks from Earth. This is important because some stars may appear dim simply because they are far away, not because they’re actually faint... icon More about Star luminosity in StellarGuide

Photometry

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
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
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HD 3638 system structure

HD 3638
HD 3638 b 1.3 AU 2098.2 M⊕ 582 days

More about HD 3638

Star HD 3638 is is much bigger than the Sun and temperature on its surface is around 3940 K (3667 °C), which is about 68 % of Sun's temperature.
       HD 3638 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 391435352197580672
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Frequently Asked Questions

How far is the HD 3638 system from the Sun?

The HD 3638 system is 727 light years or 223.0 parsecs from the Sun.

What galaxy is the HD 3638 star in?

The HD 3638 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 3638 system?

The HD 3638 is a single star, there are no other known stars in the system.

What type of star is the HD 3638?

The star HD 3638 is a Red giant star.

What temperature is star HD 3638?

The star HD 3638 has an effective temperature of 3940 K. Find out more about the temperature of stars in Stellar guide
Class of stars Red giant
White dwarfs are the hot, extremely dense stellar remnants left behind by stars that originally had masses between about 0.5 and 8 times the mass of the Sun during their main sequence lifetimes. After exhausting their nuclear fuel, these stars shed their outer layers and leave behind a compact core. Although white dwarfs contain between roughly 0.2 and 1.44 solar masses, this mass is packed into a volume comparable to that of an Earth-sized planet, making them some of the densest objects in the Universe.
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Estimated values
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