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Star HD 281229

HD 281229, also catalogued as TIC 26532226, is a young star in the Perseus Molecular Cloud, about 988.3515 light-years from the Sun. Available data do not specify its mass, radius, temperature, or age.
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Nearby stars catalogue
Sun distance
988 light years

HD 281229

Location +

Ascension iconRight ascension: 3h 49m 14.140s
Declination iconDeclination: 31° 44' 4.400'' (northern hemisphere)
Parallax iconParallax: 3.300
Distance iconSun distance: 988.352 ly | 303.0 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

Photometry

Magnitude iconApparent magnitude (V): 10.4
Magnitude iconAbsolute magnitude (V): 2.9
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 281229 system structure

HD 281229

More about HD 281229

       HD 281229 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
TIC 26532226
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Frequently Asked Questions

How far is the HD 281229 system from the Sun?

The HD 281229 system is 988 light years or 303.0 parsecs from the Sun.

What galaxy is the HD 281229 star in?

The HD 281229 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 281229 system?

The HD 281229 is a single star, there are no other known stars in the system.

What type of star is the HD 281229?

The star HD 281229 is a T Tauri star star.

What temperature is the HD 281229?

The primary in the HD 281229 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide

stellar brief logoStellar Brief

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30. 10. 2026
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The early architecture of planetary systems may be set at birth: a study of Sun-like stars found similar rates of star-planet misalignment across different stages of development. Other findings trace how water and carbon dioxide ice fade around young stars, why white-dwarf debris resists breaking into tiny pieces, and why a reported planet around Gliese 48 remains unconfirmed.
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