Astronomy:PSR B0329+54
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Short description: Pulsar in the constellation Camelopardalis
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Camelopardalis |
| Right ascension | 03h 32m 59.368s[1] |
| Declination | +54° 34′ 43.57″[1] |
| Distance | 3,460 ly (1,060 pc) |
| Spectral type | Pulsar |
| Other designations | |
| Database references | |
| SIMBAD | data |
PSR B0329+54 is a pulsar approximately 3,460 light-years away in the constellation of Camelopardalis. It completes one rotation every 0.71452[2] seconds and is approximately 5 million years old.[2]
The emissions of this pulsar and the Vela Pulsar were converted into audible sound by the French composer Gérard Grisey, and used as such in the piece Le noir de l'étoile (1989–90).[3][4][5]
Planetary system
In 1979, two exoplanets were announced to be orbiting the pulsar (being classified as pulsar planets). Later observations did not support this conclusion.[6][2][7] More recently, a 2017 analysis indicates that a different long-period pulsar planet remains a possibility,[8] and this is treated as a confirmed planet by exoplanet databases.[9]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (years) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 1.97 ± 0.19 M⊕ | 10.26 ± 0.07 | 27.76 ± 0.03 | 0.236 ± 0.011 | — | — |
See also
References
- ↑ 1.0 1.1 Cutri, R. M. et al. (June 2003), 2MASS All Sky Catalog of point sources, NASA/IPAC, Bibcode: 2003tmc..book.....C.
- ↑ 2.0 2.1 2.2 Konacki, Maciej et al. (July 1999), "Are There Planets around the Pulsar PSR B0329+54?", The Astrophysical Journal 519 (1): L81–L84, doi:10.1086/312089, Bibcode: 1999ApJ...519L..81K.
- ↑ Re, Giuseppe del. 2000. Cosmic Dance, pp. 24–25. Templeton Foundation Press, ISBN:9781890151256
- ↑ Luminet, Jean-Pierre. 2011. Illuminations: Cosmos et esthétique, pp. 419–420. Odile Jacob, ISBN:9782738185938
- ↑ Template:IRCAM work
- ↑ Hobbs, G.; Lyne, A. G.; Kramer, M. (February 2010), "An analysis of the timing irregularities for 366 pulsars", Monthly Notices of the Royal Astronomical Society 402 (2): 1027–1048, doi:10.1111/j.1365-2966.2009.15938.x, Bibcode: 2010MNRAS.402.1027H.
- ↑ Shabanova, T. V. et al. (September 2013), "Timing Observations of 27 Pulsars at the Pushchino Observatory from 1978 to 2012", The Astrophysical Journal 775 (1): 24, doi:10.1088/0004-637X/775/1/2, 2, Bibcode: 2013ApJ...775....2S.
- ↑ 8.0 8.1 Starovoit, E. D.; Rodin, A. E. (2017). "On the existence of planets around the pulsar PSR B0329+54". Astronomy Reports 61 (11): 948–953. doi:10.1134/S1063772917110063. Bibcode: 2017ARep...61..948S.
- ↑ "PSR B0329+54". https://exoplanetarchive.ipac.caltech.edu/overview/PSR%20B0329+54.
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