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Star HD 94890

Red giant HD 94890 is located 208 light years away from the Sun. It is a single star of spectral class K0III, that has 174 % of solar mass. There are multiple known exoplanets in this system.
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Sun distance
208 light years

HD 94890

Spectral class: K0III

Location +

Ascension iconRight ascension: 10h 56m 43.157s
Declination iconDeclination: -37° 8' 17.954'' (southern hemisphere)
Parallax iconParallax: 15.713
Distance iconSun distance: 207.568 ly | 63.6 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: 174 % M Sun
| 1823 M Jupiter
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Star mass
Mass of the star HD 94890 is 1.74 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: 1071 % R Sun
| 106.6 R Jupiter
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Star size
Radius of the star HD 94890 is 10.71 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: 4867 K | 0.84 T Sun
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Star temperature
Surface temperature of HD 94890 is 4867 K, which is 84 % 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: 58.01 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

Magnitude iconApparent magnitude (V): 4.6
Magnitude iconAbsolute magnitude (V): 0.6
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 94890 system structure

HD 94890
HD 94890 b 2.07 AU 677.1 M⊕ 824.6 days
HD 94890 c 4.33 AU 2829.4 M⊕ 2492.2 days

More about HD 94890

Star HD 94890 is is approximately 11 times bigger than the Sun and temperature on its surface is around 4867 K (4594 °C), which is about 84 % of Sun's temperature.
       HD 94890 can be found in southern celestial hemisphere, and it is possible to see it with naked eye. The star is also observable from Northern America, Europe and Asia. 
Other designations of this star
Iota Antliae, Iot Ant, ι Ant, CD−36 6808, CPD−36 4700, FK5 414, HIP 53502, HR 4273, SAO 201927, PPM 288317, Gaia DR3 5394951821153092864
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Frequently Asked Questions

How far is the HD 94890 system from the Sun?

The HD 94890 system is 208 light years or 63.6 parsecs from the Sun.

What galaxy is the HD 94890 star in?

The HD 94890 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 94890 system?

The HD 94890 is a single star, there are no other known stars in the system.

What type of star is the HD 94890?

The star HD 94890 is a Red giant star.

What temperature is star HD 94890?

The star HD 94890 has an effective temperature of 4867 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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