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词条 HD 188015 b
释义

  1. References

  2. Bibliography

  3. External links

{{Infobox planet
| name = HD 188015 b
| discoverer = Marcy et al.
| discovery_site = {{flag|United States}}
| discovered = January 25, 2005
| discovery_method = Doppler spectroscopy
| apsis = astron
| aphelion = {{convert|1.368|AU|km|abbr=on}}
| perihelion = {{convert|1.038|AU|km|abbr=on}}
| semimajor = {{convert|1.203|±|0.070|AU|km|abbr=on}}
| eccentricity = 0.137 ± 0.026
| period = 461.2 ± 1.7 d
1.263 y
| avg_speed = 28.47
| time_periastron = 2,451,787 ± 17
| arg_peri = 222° ± 10
| semi-amplitude = 37.6 ± 1.2
| star = HD 188015
| mass = >1.50 ± 0.13 {{Jupiter mass|link=y}}
}}

HD 188015 b is an extrasolar planet announced by the California and Carnegie Planet Search team in 2005. Like majority of known planets, it was discovered using the radial velocity method.

The planet has a minimum mass about quarter greater than Jupiter. It orbits the star in a slightly eccentric orbit in a mean distance 20% further than Earth orbits the Sun.

Stability analysis reveals that the orbits of Earth-sized planets in the Trojan points of HD 188015 b would be stable for long periods of time.[1]

References

1. ^{{cite journal |journal=Astronomy & Astrophysics |doi=10.1051/0004-6361:20077994 | volume=474 |issue=3|pages=1023–1029 |title=Survey of the stability region of hypothetical habitable Trojan planets |author1=R. Schwarz |author2=R. Dvorak |author3=Á. Süli |author4=B. Érdi |bibcode=2007A&A...474.1023S |date=November 2007}}: HD 93083, HD 17051, HD 28185, HD 27442, HD 188015, HD 99109, HD 221287

}}

Bibliography

  • {{cite journal | title=Catalog of Nearby Exoplanets | url=http://iopscience.iop.org/0004-637X/646/1/505/fulltext/ | last1=Butler | first1=R. P. | last2=Wright | first2=J. T. | last3=Marcy | first3=G. W. | last4=Fischer | first4=D. A. | last5=Vogt | first5=S. S. | last6=Tinney | first6=C. G. | last7=Jones | first7=H. R. A. | last8=Carter | first8=B. D. | last9=Johnson | first9=J. A. | last10=McCarthy | first10=C. | last11=Penny | first11=A. J. | display-authors=1 | journal=The Astrophysical Journal | volume=646 | issue=1 | pages=505–522 | date=2006 | doi=10.1086/504701 | bibcode=2006ApJ...646..505B | arxiv=astro-ph/0607493 }}
  • {{cite journal | url=http://www.iop.org/EJ/article/0004-637X/646/1/523/64035.html | author=Raghavan | title=Two Suns in The Sky: Stellar Multiplicity in Exoplanet Systems | journal=The Astrophysical Journal | volume=646 | issue=1 | pages=523–542 | date=2006 | doi=10.1086/504823 | last2=Henry | first2=Todd J. | last3=Mason | first3=Brian D. | last4=Subasavage | first4=John P. | last5=Jao | first5=Wei‐Chun | last6=Beaulieu | first6=Thom D. | last7=Hambly | first7=Nigel C. | bibcode=2006ApJ...646..523R|arxiv = astro-ph/0603836 }}

External links

  • {{cite web | url=http://exoplanet.eu/planet.php?p1=HD+188015&p2=b | title=Notes for planet HD 188015 b | work=The Extrasolar Planets Encyclopaedia}}
  • {{cite web | url=http://media4.obspm.fr/exoplanets/base/etoile.php?nom=HD+188015 | title=HD 188015 | work=Exoplanets}}
{{DEFAULTSORT:Hd 188015 B}}{{extrasolar-planet-stub}}HD 188015#Sistema planetarioHD 188015#Планета

5 : Exoplanets discovered in 2006|Giant planets|Giant planets in the habitable zone|Vulpecula|Exoplanets detected by radial velocity

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