HD 330075
{{Short description|Star in the constellation Norma}}
{{Starbox begin}}
{{Starbox observe
| epoch = J2000.0
| constell = Norma
| dec = {{DEC|–49|57|48.6771}}
}}
{{Starbox character
| type =
| variable =
}}
{{Starbox astrometry
| radial_v = {{Val|61.67|0.24}}
| parallax = 22.0467
| p_error = 0.0443
}}
{{Starbox detail
| radius = {{Val|0.85|0.02|0.03}}
| temperature = {{Val|4967|88|65|fmt=commas}}
| luminosity = {{Val|0.393|0.001}}
| metal_fe = {{Val|0.18|0.04}}
}}
{{Starbox catalog
| names = {{odlist | CD=-49°10033 | HD=330075 | HIP=77517 | SAO=226248 | LTT=6312 | PPM=321068 | NLTT=41237|2MASS=J15493770-4957486|Gaia DR2=5982775854377691136}}
}}
{{Starbox reference
| Simbad = HD+330075
| EPE = HD+330075
}}
{{Starbox end}}
HD 330075 is a star in the southern constellation of Norma. It has a yellow hue and an apparent visual magnitude of 9.36, which makes it too faint to be seen with the naked eye – it is visible only with telescope or powerful binoculars. Parallax measurements provide a distance estimate of 148 light years from the Sun, and it is drifting further away with a radial velocity of 62 km/s. The star is estimated to have come as close as {{Convert|34.20|pc|ly|disp=out|abbr=off}} some 409 million years ago.
This object appears to be a slightly evolved dwarf with a spectral class of G5. That is, it is nearing the end of its main sequence lifetimes and is becoming a subgiant star. The star has very low chromospheric activity and is around five billion years old. It is smaller than the Sun with 86% of the Sun's mass and 85% of the solar radius. As a consequence, it is radiating just 39% of the luminosity of the Sun from its photosphere at an effective temperature of 4,967 K. It has a super-solar metallicity, which means the abundance of elements other than hydrogen and helium appears much higher than in the Sun.
Planetary system
In 2004, the discovery of a hot Jupiter planet orbiting close to the star was announced. This is the first planet discovered by the then-new HARPS spectrograph.
{{OrbitboxPlanet begin}}
{{OrbitboxPlanet
| exoplanet = b
| mass = ≥ 0.76
| period = {{Val|3.369|0.004}}
| semimajor = 0.043
| eccentricity = 0
}}
{{Orbitbox end}}
See also
References
{{Reflist|refs=
{{cite simbad | title=HD 330075 | accessdate=2019-11-18}}
{{Cite Gaia DR2|5982775854377691136}}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | arxiv=1108.4971
| doi=10.1134/S1063773712050015 | s2cid=119257644 }}
| title=Chemical fingerprints of hot Jupiter planet formation
| display-authors=1 | last1=Maldonado | first1=J.
| last2=Villaver | first2=E. | last3=Eiroa | first3=C.
| journal=Astronomy & Astrophysics
| volume=612 | id=A93 | pages=18 | date=May 2018
| arxiv=1712.01035 | bibcode=2018A&A...612A..93M
| doi=10.1051/0004-6361/201732001 | s2cid=119458710 }}
| url=http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full/2004/31/aa0389-04/aa0389-04.html
| title=The HARPS search for southern extra-solar planets I. HD 330075 b: A new "hot Jupiter"
| last1=Pepe | first1=F. | last2=Mayor | first2=M.
| last3=Queloz | first3=D. | last4=Benz | first4=W.
| last5=Bonfils | first5=X. | last6=Bouchy | first6=F.
| last7=Lo Curto | first7=G. | last8=Lovis | first8=C.
| last9=Mégevand | first9=D. | display-authors=1
| journal=Astronomy and Astrophysics
| volume=423 | issue=1 | pages=385–389 | year=2004
| arxiv=astro-ph/0405252 | bibcode=2004A&A...423..385P
| doi=10.1051/0004-6361:20040389 | s2cid=59157984
}}
}}
External links
- {{cite web
| url=http://media4.obspm.fr/exoplanets/base/etoile.php?nom=HD+330075
| title=HD 330075
| work=Exoplanets
| accessdate=2009-05-22
| archive-url=https://web.archive.org/web/20091125000631/http://media4.obspm.fr/exoplanets/base/etoile.php?nom=HD+330075
| archive-date=2009-11-25
| url-status=dead
}}
{{Sky|15|49|37.6913|-|49|57|48.692|163.7}}
{{Stars of Norma}}
Category:G-type main-sequence stars
Category:Planetary systems with one confirmed planet