WASP-56: Difference between revisions
Content deleted Content added
Bibcode Bot (talk | contribs) m Adding 1 arxiv eprint(s), 1 bibcode(s) and 0 doi(s). Did it miss something? Report bugs, errors, and suggestions at User talk:Bibcode Bot |
Tom.Reding (talk | contribs) m WP:GenFixes, ref cleanup, parse authN/edN using AWB |
||
| Line 2: | Line 2: | ||
|constell= [[Triangulum (constellation)|Triangulum]] |
|constell= [[Triangulum (constellation)|Triangulum]] |
||
|name= Wasp 56 |
|name= Wasp 56 |
||
|type= G6 <ref name=SIMBAD> |
|type= G6 <ref name=SIMBAD>SIMBAD, [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=wasp+56&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id Cl* Melotte 111 AV 561 -- Star in Cluster] (accessed 9 September 2013)</ref> |
||
|ra= {{RA|12|13|27.906}} <ref name=SIMBAD/> |
|ra= {{RA|12|13|27.906}} <ref name=SIMBAD/> |
||
|dec= {{DEC|+23|03|20.30}} <ref name=SIMBAD/> |
|dec= {{DEC|+23|03|20.30}} <ref name=SIMBAD/> |
||
}} |
}} |
||
'''WASP-56''' is a sun-like star of spectral type G6 in the constellation of [[Triangulum]]. It has an apparent magnitude of 11.48. It has a [[exoplanet|planet]] around 0.6 the mass of [[Jupiter]] that has a period of 4.6 days. The planet possibly has a large core of heavy metals.<ref>{{cite journal|author=Faedi, F. |
'''WASP-56''' is a sun-like star of spectral type G6 in the constellation of [[Triangulum]]. It has an apparent magnitude of 11.48. It has a [[exoplanet|planet]] around 0.6 the mass of [[Jupiter]] that has a period of 4.6 days. The planet possibly has a large core of heavy metals.<ref>{{cite journal|display-authors=4|author=Faedi, F.|author2=Pollacco, D.|author3=Barros, S. C. C.|author4=Brown, D.|author5=Collier Cameron, A.|author6= Doyle,A. P.|author7=Enoch, R.|author8=Gillon, M.|author9=Gómez Maqueo Chew, Y.|author10=Hébrard, G.|author11=Lendl, M.|author12=Liebig, C.|author13=Smalley, B.|author14=Triaud, A. H. M. J.|author15=West, R. G.|author16=Wheatley, P. J.|author17=Alsubai, K. A.|author18=Anderson, D. R.|author19=Armstrong, D.|author20=Bento, J.|author21=Bochinski, J.|author22=Bouchy, F.|author23=Busuttil, R.|author24=Fossati, L.|author25=Fumel, A.|author26=Haswell, C. A.|author27=Hellier, C.|author28=Holmes, S.|author29=Jehin, E.|author30=Kolb, U.|author31=McCormac, J.|author32=Miller, G. R. M.|author33=Moutou, C.|author34=Norton, A. J.|author35=Parley, N.|author36=Queloz, D.|author37=Santerne, A.|author38=Skillen, I.|author39=Smith, A. M. S.|author40=Udry, S.|author41=Watson, C. |date=2013|title=WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP|journal=[[Astronomy and Astrophysics]]|volume=551|url=http://arxiv.org/pdf/1210.2329v2.pdf|pages=A73-90|doi=10.1051/0004-6361/201220520|arxiv = 1210.2329 |bibcode = 2013A&A...551A..73F }}</ref> |
||
==References== |
==References== |
||
| Line 16: | Line 15: | ||
[[Category:Triangulum (constellation)]] |
[[Category:Triangulum (constellation)]] |
||
[[Category:G-type stars]] |
[[Category:G-type stars]] |
||
{{Star-stub}} |
{{Star-stub}} |
||
Revision as of 18:11, 4 May 2015
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Triangulum |
| Right ascension | 12h 13m 27.906s [1] |
| Declination | +23° 03′ 20.30″ [1] |
| Spectral type | G6 [1] |
WASP-56 is a sun-like star of spectral type G6 in the constellation of Triangulum. It has an apparent magnitude of 11.48. It has a planet around 0.6 the mass of Jupiter that has a period of 4.6 days. The planet possibly has a large core of heavy metals.[2]
References
- ^ a b c SIMBAD, Cl* Melotte 111 AV 561 -- Star in Cluster (accessed 9 September 2013)
- ^ Faedi, F.; Pollacco, D.; Barros, S. C. C.; Brown, D.; et al. (2013). "WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP" (PDF). Astronomy and Astrophysics. 551: A73-90. arXiv:1210.2329. Bibcode:2013A&A...551A..73F. doi:10.1051/0004-6361/201220520.
 | This star-related article is a stub. You can help Wikipedia by expanding it. |