Geminga

Geminga

Geminga as seen by Chandra and Spitzer
Credit: X-ray: NASA/CXC/PSU/B. Posselt et al; Infrared: NASA/JPLCaltech
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Gemini
Right ascension 06h 33m 54.15s
Declination +17° 46′ 12.9″
Apparent magnitude (V) 25.5
Characteristics
Evolutionary stage Pulsar
Astrometry
Parallax (π)4.0±1.3 mas
Distance~815 ly
(250+120
−62
 pc)
Details
Rotation0.237 s
Age339,000 years
Other designations
SN 437, PSR B0633+17, PSR J0633+1746
Database references
SIMBADdata

Geminga (/ɡəˈmɪŋɡə/ gə-MING-gə) is a gamma ray and x-ray pulsar source thought to be a neutron star approximately 250 parsecs (around 800 light-years) from the Sun in the constellation Gemini.

Its name, attributed by its discoverer Giovanni Bignami, is both a contraction of Gemini gamma-ray source and a transcription of the words gh'è minga (pronounced [ɡɛ ˈmĩːɡa]), meaning "it's not there" in Bignami's native Milanese dialect of Lombard. The name was approved by the International Astronomical Union on 4 April 2022.