Gum Nebula

The Gum Nebula (Gum 12) is an emission nebula that extends across 36° in the southern constellations Vela and Puppis. It lies approximately 450 parsecs from the Earth.^[1] Hard to distinguish, it was widely believed to be the greatly expanded (and still expanding) remains of a supernova that took place about a million years ago. More recent research suggests it may be an evolved H II region. It contains the 11,000-year-old Vela Supernova Remnant, along with the Vela Pulsar.

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Quick Facts Supernova remnant, Observation data: J2000.0 epoch ...

Gum Nebula
Supernova remnant
The Gum Nebula in H-alpha
Observation data: J2000.0 epoch
Right ascension	08^h 00^m
Declination	−43° 00′
Distance	1470 ly (450 pc)
Apparent magnitude (V)	+12 (infrared only)
Apparent diameter	30°
Constellation	Vela, Puppis
Physical characteristics
Absolute magnitude (V)	3.73 (infrared)

Designations	Gum 12
See also: Lists of nebulae

The Gum Nebula contains about 32 cometary globules.^[2] These dense cloud cores are subject to such strong radiation from O-type stars γ² Vel and ζ Pup and formerly the progenitor of the Vela Supernova Remnant that the cloud cores evaporate away from the hot stars into comet-like shapes. Like ordinary Bok globules, cometary globules are believed to be associated with star formation.^[3] A notable object inside one of these cometary globules is the Herbig-Haro object HH 46/47.

The main ionizing sources are the Vela OB2 association (including Gamma Velorum cluster and the P Puppis cluster), Zeta Puppis and the OB association Trumpler 10.^[4]^[5] The star cluster NGC 2547 formed 100 pc more distant than Vela OB2 and is an interloper.^[5] The Vela OB2 association is surrounded by the so-called "IRAS Vela Shell", located in the south of the Gum Nebula. The star clusters NGC 2547, Trumpler 10, NGC 2451B, Collinder 135 and Collinder 140 all have similar ages of about 30 Myrs. It is suggested that a few stars exploded in supernovae about 30 Myrs ago in the center of the Gum Nebula and triggered the formation of stars in the region.^[6]

It is named after its discoverer, the Australian astronomer Colin Stanley Gum (1924–1960). Gum had published his findings in 1955 in a work called A study of diffuse southern H-alpha nebulae (see Gum catalog). He also published the discovery of the Gum Nebula in 1952 in the journal The Observatory. The observations were made with the Commonwealth Observatory.^[7]

The Gum nebula was photographed during Apollo 16 while the command module was in the double umbra of the Sun and Earth, using high-speed Kodak film.^[8]

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