NGC 2899
   HOME

TheInfoList



OR:

NGC 2899 is a planetary nebula in the southern
constellation A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object. The origins of the e ...
of Vela. It was discovered by English astronomer
John Herschel Sir John Frederick William Herschel, 1st Baronet (; 7 March 1792 â€“ 11 May 1871) was an English polymath active as a mathematician, astronomer, chemist, inventor, experimental photographer who invented the blueprint and did botanical wor ...
on February 27, 1835. This nebula can be viewed with a moderate-sized amateur telescope, but requires a larger telescope to resolve details. NGC 2899 is located at a distance of from the Sun and from the Galactic Center. This nebula has an overall kidney shape that is elongated along an axis from WNW to ESE. The overall topology is bipolar with a significant equatorial structure. This shape is believed to result from a binary star system. The mean expansion rate is , with high velocity structures expanding at . The core mass of the central star is estimated as . The nebula lies within a large cavity in the surrounding medium. This opening has quadrupolar shape with a physical dimension of . The elongation lies along a position angle of , which is aligned with the minor axis of the planetary nebula. This opening was most likely crafted by a fast
stellar wind A stellar wind is a flow of gas ejected from the upper atmosphere of a star. It is distinguished from the bipolar outflows characteristic of young stars by being less collimated, although stellar winds are not generally spherically symmetric. D ...
coming from the central star during its
asymptotic giant branch The asymptotic giant branch (AGB) is a region of the Hertzsprung–Russell diagram populated by evolved cool luminous stars. This is a period of stellar evolution undertaken by all low- to intermediate-mass stars (about 0.5 to 8 solar masses) lat ...
stage, prior to the formation of a planetary nebula. The shape and filamentary structures suggest the interaction of a binary star system.


References


External links and images

* * * {{DEFAULTSORT:NGC 2899 Planetary nebulae 2899 Vela (constellation) Discoveries by John Herschel