Nebula | |
---|---|
![]() | |
Observation data: J2000 epoch | |
Right ascension | 09h 12m 26s |
Declination | -42° 25′ 39″ |
Constellation | Vela |
Designations | PK 265+4.1,
ESO 314-PN6, AM 0910-421, CS=13.8, HD 79384, IRAS 09105-4213, WEB 8618, PMN J0912-4225, 2MASS J09122664-4225397 |
NGC 2792 is a planetary nebula located in the constellation Vela.[1] NGC 2792 was discovered by British astronomer John Herschel in 1835.[2]
Observation
[edit]With an apparent visual magnitude of 11.6,[3] you must use a telescope with an aperture of at least 200 mm to observe it.[4]
Characteristics
[edit]Distance, size and speed
[edit]Two very similar distances are indicated on the SIMBAD database: 3.086 ± 0.617 kpc (~10,100 ly) and approximately 3050 pc (~9,950 ly).[5]
The apparent size of the nebula is 0.350′ × 0.315, which, given the distance of 3,086 ± 617 pc and through simple calculation, equates to an actual size of 1.02 ± 0.20 al × 0 .92 ± 0.18 ly.[5]
Two identical speed values are also indicated on SIMBAD, i.e. 14.0 ± 5.0 km/s. According to a more recent publication (2023) the speed of the nebula is 12.7 ± 8 km/s.[5]
Age
[edit]The kinematic age of a planetary nebula can be estimated from its expansion speed. According to González-Santamaría and his colleagues, the expansion speed of NGC 2792 is 20 km/s, which gives it a kinematic age of 3.5 thousand years. According to a more recent publication, its expansion speed is 20.2 km/s.[6]
According to González-Santamaría, it has been approximately 50,860 years since the star left the asymptotic giant branch and the nebula enveloping it reached 1% of the mass of the progenitor.[6]
Central star
[edit]The visual magnitude of this star is equal to 16.74 and its mass is estimated at 1.163 solar masses. The radius of the nebula is estimated at 0.108 pc.[7]
See also
[edit]External links
[edit]References
[edit]- ^ "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-06-05.
- ^ "New General Catalog Objects: NGC 2750 - 2799". cseligman.com. Retrieved 2024-06-05.
- ^ "NGC 2792 - Planetary Nebula in Vela | TheSkyLive.com". theskylive.com. Retrieved 2024-06-05.
- ^ astrovalleyfield.ca http://astrovalleyfield.ca//AstronomieCompl/NGC%20et%20autres/WolfgangS/N2700_exc_web.htm. Retrieved 2024-06-05.
{{cite web}}
: Missing or empty|title=
(help) - ^ a b c "NGC 2792". simbad.cds.unistra.fr. Retrieved 2024-06-05.
- ^ a b Skrutskie, M. F.; Cutri, R. M.; Stiening, R.; Weinberg, M. D.; Schneider, S.; Carpenter, J. M.; Beichman, C.; Capps, R.; Chester, T.; Elias, J.; Huchra, J.; Liebert, J.; Lonsdale, C.; Monet, D. G.; Price, S. (February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256.
- ^ Wilson, R. E. (2010-01-01). "VizieR Online Data Catalog: General Catalogue of Stellar Radial Velocities (Wilson, 1953)". VizieR Online Data Catalog. 3021: III/21. Bibcode:2010yCat.3021....0W.
Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
View the detailed Guide of Psilotum nudum: Detailed Study Of Psilotum Nudum (Whisk Fern), Classification, Anatomy, Reproduction