HR 4458
{{Short description|Binary star system in the constellation Hydra}}
{{Starbox begin}}
{{Starbox observe 2s
| constell = Hydra
| epoch = J2000
| component1 = A
| dec1 = {{DEC|-32|49|52.8228}}
| component2 = B
| dec2 = {{DEC|-32|50|02.4048}}
}}
{{Starbox character
| class = K0 V + DC8
| r-i = 0.40{{cn|date=March 2025}}
| v-r = 0.44{{cn|date=March 2025}}
| variable =
}}
{{Starbox astrometry
| component1 = A
| radial_v = {{val|-22.09|0.12}}
| prop_mo_ra = –670.230
| prop_mo_dec = +822.399
| parallax = 104.6133
| p_error = 0.0277
| component2 = B
| radial_v2 =
| prop_mo_ra2 = –701.802
| prop_mo_dec2 = +828.928
| parallax2 = 104.6570
| p_error2 = 0.0267
}}
{{Starbox detail
| component1=HR 4458 A
| luminosity_bolometric = 0.368
| component2=HR 4458 B
| radius2 =
| metal_fe2 =
| rotational_velocity2 =
| luminosity_bolometric2 = 0.000088
| age_gyr2 = 5.69{{efn|name=cooling}}
}}
{{Starbox catalog
| names = {{odlist | name=289 G. Hya | F=20 Crt | GJ=432 | CD=−32°8179 | HD=100623 | HIP=56452 | HR=4458 | SAO=202583 | PLX=2678.00 | LHS=308 | LTT=4280 }}
| component2=B
| names2={{odlist | WD=1132-325}}, VB 4
}}
{{Starbox reference
| Simbad=HD+100623 |sn=A
| Simbad2=HD+100623B |sn2=B
| ARICNS=00888
}}
{{Starbox end}}
HR 4458 (HD 100623) is a binary star system 31.18 light-years away in the equatorial constellation of Hydra. It has the Flamsteed designation 20 Crateris and the Gould designation 289 G. Hydrae; the former refers to the constellation Crater, but when the IAU formally defined constellation boundaries, it was placed in Hydra. This object is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.97. It is moving closer to the Earth with a heliocentric radial velocity of −22 km/s.
The primary component is a K-type main-sequence star with a stellar classification of K0 V. It is around five billion years old with 84% of the Sun's radius. The star is radiating 37% of the Sun's luminosity from its photosphere at an effective temperature of 5,241 K. It has been examined for the presence of an infrared excess, but none was detected.
There is a 15th-magnitude common proper motion companion at an angular separation of {{val|16.2|ul=″}}, corresponding to a projected separation of {{Val|162.5|ul=AU}}. This is a white dwarf star with a classification of DC8. The orbital period of the pair is estimated as {{Convert|406000|days|years|disp=out|abbr=off}}.
Notes
References
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External links
- {{cite web
| url =http://www.solstation.com/stars/hr4458ab.htm
| title =CD-32 8179 / HR 4458 AB
| publisher =SolStation
| access-date =2007-06-06
| archive-url =https://web.archive.org/web/20121013003737/http://www.solstation.com/stars/hr4458ab.htm
| archive-date =2012-10-13
| url-status =dead
}}
{{Stars of Hydra}}
{{DEFAULTSORT:HR 4458}}
Category:K-type main-sequence stars