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TOI-5628 B
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Star TOI-5628 B

White dwarf TOI-5628 B is located 360 light years away from the Sun. It is a single star, that has 59 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
360 light years
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TOI-5628 B

White dwarf

Location +

Distance iconDistance from the primary: 2500 AU

Basic characteristic

icon weight
Mass: 59 % M Sun
| 618 M Jupiter
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Star mass
Mass of the star TOI-5628 B is 0.59 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
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TOI-5628 B system structure

 TOI-5628 A
TOI-5628 A b 0.04 AU 28.6 M⊕ 8.3 R⊕ 4.3 days
TOI-5628 B 2500 AU

More about TOI-5628 B

       TOI-5628 B can be found in northern celestial hemisphere.
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External sources
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Scientific study, Accepted: 29. 12. 2026
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A Spatial Map of the Atmospheric Limb of a Hot Jupiter
Scientific study, Accepted: 14. 10. 2026
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Peering into the Midplane of the DM Tau Disk using N2H+ and DCO+
Scientific study, Accepted: 13. 10. 2026

News from this star system

Molecular emission in the disk around DM Tauri reveals complex chemical processes
iconToday
Image: Molecular emission in the disk around DM Tauri reveals complex chemical processes
Observations of the disk around DM Tauri reveal how N2H+ and DCO+ molecules are distributed. The data show that external UV radiation and cosmic rays influence the chemical makeup of the disk out to 400 astronomical units, impacting how planets may form....
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Narrow ring of gas found near the young star HD 152384
iconToday
Image: Narrow ring of gas found near the young star HD 152384
A narrow ring of gas has been characterized around the young star HD 152384. Located at the dust sublimation radius, the ring likely formed from the collisions of rocky planetesimals, offering a new look at early planetary system evolution....
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Atmospheric composition of hot Jupiter KELT-2A b reveals chemical history
iconToday
Image: Atmospheric composition of hot Jupiter KELT-2A b reveals chemical history
New observations of hot Jupiter KELT-2A b confirm water vapor in its atmosphere. The planet shows a carbon-to-oxygen ratio similar to its host star but with overall lower metallicity, suggesting a complex migration history from far out in its star system....
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Frequently Asked Questions

How far is the TOI-5628 B system from the Sun?

The TOI-5628 B system is 360 light years or 110.3 parsecs from the Sun.

What galaxy is the TOI-5628 B star in?

The TOI-5628 B is in the Milky Way galaxy just like the Sun.

How many stars are in the TOI-5628 B system?

The TOI-5628 B is a single star, there are no other known stars in the system.

What type of star is the TOI-5628 B?

The star TOI-5628 B is a White dwarf star.

What temperature is the TOI-5628 B?

The primary in the TOI-5628 B system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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exoplanet iconAbout Stellar Catalog

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Estimated values
icon Objects listed in the Stellar Catalog often have values that are estimates. These estimates are determined using their known characteristics, such as spectral type, brightness across different wavelengths, distance from a star, and other factors.
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