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Psi Velorum B
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Star Psi Velorum B

Subgiant Psi Velorum B is located 60 light years away from the Sun. It is a single star of spectral class F3 IV, that has typically about 300 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
60 light years

Psi Velorum B

Subgiant, High proper motion star
Spectral class: F3 IV

Basic characteristic

icon weight
Mass: 130 % M Sun
| 1393.3 M Jupiter
 (estimate)
+
Star mass
The mass of the star Psi Velorum B is unknown. Based on its other characteristics, it is estimated to be about 130 % of the Sun's mass.

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: 160 % R Sun
| 15.7 R Jupiter
(estimate)
+
Star size
Radius of the star Psi Velorum B is not known. Its estimated value based on other similar stars is about 160 % 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 iconTemperature: 6500 K
 (estimate)
+
Star temperature
Surface temperature of Psi Velorum B is estimated to be 6484 K, which is 112 % 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

Photometry

Magnitude iconApparent magnitude (V): 5.1
Magnitude iconAbsolute magnitude (V): 3.8
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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Psi Velorum B system structure

Psi Velorum A
Psi Velorum B

More about Psi Velorum B

       Psi Velorum B 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. 
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External sources
icon study
_empty
Scientific study, Accepted: 29. 12. 2026
icon study
A Spatial Map of the Atmospheric Limb of a Hot Jupiter
Scientific study, Accepted: 14. 10. 2026
icon study
Peering into the Midplane of the DM Tau Disk using N2H+ and DCO+
Scientific study, Accepted: 13. 10. 2026
simbad icon
Simbad database (* psi Vel B)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)

Frequently Asked Questions

How far is the Psi Velorum B system from the Sun?

The Psi Velorum B system is 60 light years or 18.4 parsecs from the Sun.

What galaxy is the Psi Velorum B star in?

The Psi Velorum B is in the Milky Way galaxy just like the Sun.

How many stars are in the Psi Velorum B system?

The Psi Velorum B is a single star, there are no other known stars in the system.

What type of star is the Psi Velorum B?

The star Psi Velorum B is a Subgiant star.

What temperature is the Psi Velorum B?

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