Van Maanen's Star
- Type
- White dwarf star
- Diameter
- 9,510 miles
- Distance from Sun
- 14.1 light years
- Mass
- 0.67 M☉
- Temperature
- 10,574 °F
- Date of Discovery
- 1917
- As one of the first and one of the closest white dwarfs discovered, Van Maanen's Star is also the closest solitary white dwarf we have found to Earth. It has a high metal content, making it an interesting star for astronomers to study.
- Create a list of some of the nearest white dwarf stars to us.

- Located in
- Pisces
- Though the star has about two-thirds of the mass of the Sun, it is just 1% of its radius.
- It was accidentally found when Adriaan van Maaanen was looking for a companion star of another nearby star.
- The heat they emit is the surviving heat from a long gone nuclear fision process, meaning the star gradually gets colder and colder.
- The star contains metals which likely have come from smaller asteroids or similar objects being absorbed into it.