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Proper Name	van Maanen's Star
Bayer Designation	None
Flamsteed Number	None
HR (BSC)	None
HD	None
Other Designations	van Maanen 2, Wolf 28, Gliese 35
Constellation	Pisces
Right Ascension	0h 49m 10s
Declination	+5° 23' 19"
Distance	14.1 light years 4.3 parsecs
Magnitude	Apparent: +12.36 Absolute: +14.19
Spectral Class	DZ17.5 white dwarf star
Planets in this system	None known (a possible companion object has been suggested, but remains unconfirmed, and further studies suggest that its existence is unlikely)
Optimum Visibility	October
Notes	The remnant core of a long-expired red giant, van Maanen's Star was discovered by Adrian van Maanen in 1917, and at that time was only the third white dwarf to have been identified. It is an extraordinarily dense object, with an estimated two-thirds of the mass of the Sun compacted into a region only slightly larger than the Earth.

Imagery provided by Aladin sky atlas

van Maanen's Star is a near neighbour of the Sun: it lies just fourteen light years away. After Sirius B and Procyon B, it is the nearest white dwarf to the Solar System, and is the closest known solitary example.

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