HR 4458

{{Short description|Binary star system in the constellation Hydra}}

{{Starbox begin}}

{{Starbox observe 2s

| constell = Hydra

| epoch = J2000

| component1 = A

| ra1 = {{RA|11|34|29.48644}}

| dec1 = {{DEC|-32|49|52.8228}}

| appmag_v1 = 5.97

| component2 = B

| ra2 = {{RA|11|34|30.47776}}

| dec2 = {{DEC|-32|50|02.4048}}

| appmag_v2 = 15

}}

{{Starbox character

| class = K0 V + DC8

| r-i = 0.40{{cn|date=March 2025}}

| v-r = 0.44{{cn|date=March 2025}}

| b-v = 0.80

| u-b = 0.325

| variable =

}}

{{Starbox astrometry

| component1 = A

| radial_v = {{val|-22.09|0.12}}

| prop_mo_ra = –670.230

| prop_mo_dec = +822.399

| pm_footnote =

| parallax = 104.6133

| p_error = 0.0277

| parallax_footnote =

| absmag_v = 6.05

| component2 = B

| radial_v2 =

| prop_mo_ra2 = –701.802

| prop_mo_dec2 = +828.928

| pm_footnote2 =

| parallax2 = 104.6570

| p_error2 = 0.0267

| parallax_footnote2 =

| absmag_v2 = 15

}}

{{Starbox detail

| component1=HR 4458 A

| mass = 0.87

| radius = 0.84

| temperature = 5,241

| gravity = 4.59

| metal_fe = −0.37

| rotational_velocity = 6.79

| luminosity_bolometric = 0.368

| age_gyr = 4.6–5.8

| component2=HR 4458 B

| mass2 = 0.58

| radius2 =

| temperature2 = 5,000

| gravity2 = 8.12

| 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

{{notelist|refs=

{{efn|name=cooling|Cooling age}}

}}

References

{{Reflist|refs=

{{Cite Gaia DR3|3478127463341507072}}

{{cite Gaia DR3|3478127467639543296}}

{{cite simbad | title=HD 100623 | access-date=May 6, 2019 }}

{{cite journal |bibcode=1995AJ....110.1838R |title=The Palomar/MSU Nearby-Star Spectroscopic Survey. I. The Northern M Dwarfs -Bandstrengths and Kinematics |last1=Reid |first1=I. Neill |last2=Hawley |first2=Suzanne L. |last3=Gizis |first3=John E. |journal=The Astronomical Journal |date=1995 |volume=110 |page=1838 |doi=10.1086/117655 }}

{{cite journal

| url=http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=V%2F135%2Fcatalog

| last=Gould | first=Benjamin Apthorp | date=1879

| title=Uranometria Argentina catalog of bright southern stars

| journal=Resultados del Observatorio Nacional Argentino en Cordoba

| volume=1 | publication-place=Buenos Aires

| bibcode=1879RNAO....1.....G | access-date=2012-05-08

}}

{{cite journal |bibcode=2018MNRAS.480.3942H |title=The Gaia 20 pc white dwarf sample |last1=Hollands |first1=M. A. |last2=Tremblay |first2=P. -E. |last3=Gänsicke |first3=B. T. |last4=Gentile-Fusillo |first4=N. P. |last5=Toonen |first5=S. |journal=Monthly Notices of the Royal Astronomical Society |date=2018 |volume=480 |issue=3 |page=3942 |doi=10.1093/mnras/sty2057 |doi-access=free |arxiv=1805.12590 }}

{{cite journal

| display-authors=1 | last1=Holmberg | first1=J.

| last2=Nordström | first2=B. | last3=Andersen | first3=J.

| title=The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics

| volume=501 | issue=3 |date=July 2009 | pages=941–947

| journal=Astronomy and Astrophysics

| doi=10.1051/0004-6361/200811191 | bibcode=2009A&A...501..941H

| arxiv=0811.3982 | s2cid=118577511 }}

{{cite journal |bibcode=2021MNRAS.507.5902B |title=New insight into the magnetism of degenerate stars from the analysis of a volume-limited sample of white dwarfs |last1=Bagnulo |first1=S. |last2=Landstreet |first2=J. D. |journal=Monthly Notices of the Royal Astronomical Society |date=2021 |volume=507 |issue=4 |page=5902 |doi=10.1093/mnras/stab2046 |doi-access=free |arxiv=2106.11109 }}

{{cite journal

| last1=Holberg | first1=J. B.

| last2=Oswalt | first2=Terry D.

| last3=Sion | first3=E. M.

| title= A Determination of the Local Density of White Dwarf Stars

| journal=The Astrophysical Journal

| year=2002 | volume=571 | issue=1 | pages=512-518

| bibcode=2002ApJ...571..512H

| doi=10.1086/339842

| doi-access=free| arxiv=astro-ph/0102120

}}

{{cite journal |bibcode=2016MNRAS.462.2295H |title=The 25 parsec local white dwarf population |last1=Holberg |first1=J. B. |last2=Oswalt |first2=T. D. |last3=Sion |first3=E. M. |last4=McCook |first4=G. P. |journal=Monthly Notices of the Royal Astronomical Society |date=2016 |volume=462 |issue=3 |page=2295 |doi=10.1093/mnras/stw1357 |doi-access=free |arxiv=1606.01236 }}

{{cite journal

| last1=Johnson | first1=H. M.

| last2=Wright | first2=C. D.

| title=Predicted infrared brightness of stars within 25 parsecs of the sun

| journal=Astrophysical Journal Supplement Series

| year=1983 | volume=53 | issue=2 | pages=643–711

| bibcode=1983ApJS...53..643J

| doi=10.1086/190905

| doi-access=free}}

{{cite journal

| last1=Mamajek | first1=Eric E.

| last2=Hillenbrand | first2=Lynne A.

| title=Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics

| journal=The Astrophysical Journal | volume=687 | issue=2

| pages=1264–1293 |date=November 2008

| doi=10.1086/591785 | bibcode=2008ApJ...687.1264M |arxiv = 0807.1686

| s2cid=27151456

}}

{{cite journal

| display-authors=1

| last1=Gray | first1=R. O.

| last2=Corbally | first2=C. J.

| last3=Garrison | first3=R. F.

| last4=McFadden | first4=M. T.

| last5=Bubar | first5=E. J.

| last6=McGahee | first6=C. E.

| last7=O'Donoghue | first7=A. A.

| last8=Knox | first8 = E. R.

| title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample

| journal=The Astronomical Journal

| volume=132 | issue=1 | pages=161–70 | date=2006

| doi=10.1086/504637

| bibcode=2006AJ....132..161G

| arxiv=astro-ph/0603770

| s2cid=119476992 }}

{{cite journal

| display-authors=1

| last1=Nidever | first1=David L.

| last2=Marcy | first2=Geoffrey W.

| last3=Butler | first3=R. Paul

| last4=Fischer | first4=Debra A.

| last5=Vogt | first5=Steven S.

| title=Radial Velocities for 889 Late-Type Stars

| journal=The Astrophysical Journal Supplement Series | volume=141 | issue=2

| pages=503–522 | date=August 2002

| doi=10.1086/340570 | bibcode=2002ApJS..141..503N | arxiv=astro-ph/0112477

| s2cid=51814894 }}

{{cite journal

| display-authors=1

| last1=Ramírez | first1=I.

| last2=Fish | first2=J. R.

| last3=Lambert | first3=D. L.

| last4=Allende Prieto | first4=C.

| title=Lithium Abundances in nearby FGK Dwarf and Subgiant Stars: Internal Destruction, Galactic Chemical Evolution, and Exoplanets

| journal=The Astrophysical Journal | volume=756 | issue=1

| page=46 | date=September 2012

| doi=10.1088/0004-637X/756/1/46 | bibcode=2012ApJ...756...46R | arxiv=1207.0499

| s2cid=119199829 }}

{{cite journal | display-authors=1 | last1=Martínez-Arnáiz | first1=R. | last2=Maldonado | first2=J. | last3=Montes | first3=D. | last4=Eiroa | first4=C. | last5=Montesinos | first5=B. | title=Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter | journal=Astronomy and Astrophysics | volume=520 | page=A79 | date=September 2010 | doi=10.1051/0004-6361/200913725 | bibcode=2010A&A...520A..79M | arxiv=1002.4391 | s2cid=43455849 | url=http://eprints.ucm.es/37826/1/davidmontes17libre.pdf | access-date=2018-11-04 | archive-date=2017-09-22 | archive-url=https://web.archive.org/web/20170922031257/http://eprints.ucm.es/37826/1/davidmontes17libre.pdf | url-status=dead }}

{{cite journal

| author=Mermilliod, J.-C.

| title=Compilation of Eggen's UBV data, transformed to UBV (unpublished)

| journal=Catalogue of Eggen's UBV Data | date=1986

| bibcode=1986EgUBV........0M

}}

{{cite journal

| display-authors=1

| last1=Holberg | first1=J. B.

| last2=Oswalt | first2=T. D.

| last3=Sion | first3=E. M.

| last4=Barstow | first4=M. A.

| last5=Burleigh | first5=M. R.

| title=Where are all the Sirius-like binary systems?

| journal=Monthly Notices of the Royal Astronomical Society

| volume=435 | issue=3 | pages=2077–2091 |date=November 2013

| doi=10.1093/mnras/stt1433 | doi-access=free | bibcode=2013MNRAS.435.2077H | arxiv=1307.8047

}}

{{cite journal

| display-authors=1

| last1=Eiroa | first1=C.

| last2=Marshall | first2=J. P.

| last3=Mora | first3=A.

| last4=Montesinos | first4=B.

| last5=Absil | first5=O.

| last6=Augereau | first6=J. Ch.

| last7=Bayo | first7=A.

| last8=Bryden | first8=G.

| last9=Danchi | first9=W.

| last10=del Burgo | first10=C.

| last11=Ertel | first11=S.

| last12=Fridlund | first12=M.

| last13=Heras | first13=A. M.

| last14=Krivov | first14=A. V.

| last15=Launhardt | first15=R.

| last16=Liseau | first16=R.

| last17=Löhne | first17=T.

| last18=Maldonado | first18=J.

| last19=Pilbratt | first19=G. L.

| last20=Roberge | first20=A.

| last21=Rodmann | first21=J.

| last22=Sanz-Forcada | first22=J.

| last23=Solano | first23=E.

| last24=Stapelfeldt | first24=K.

| last25=Thébault | first25=P.

| last26=Wolf | first26=S.

| last27=Ardila | first27=D.

| last28=Arévalo | first28=M.

| last29=Beichmann | first29=C.

| last30=Faramaz | first30=V.

| last31=González-García | first31=B. M.

| last32=Gutiérrez | first32=R.

| last33=Lebreton | first33=J.

| last34=Martínez-Arnáiz | first34=R.

| last35=Meeus | first35=G.

| last36=Montes | first36=D.

| last37=Olofsson | first37=G.

| last38=Su | first38=K. Y. L.

| last39=White | first39=G. J.

| last40=Barrado | first40=D.

| last41=Fukagawa | first41=M.

| last42=Grün | first42=E.

| last43=Kamp | first43=I.

| last44=Lorente | first44=R.

| last45=Morbidelli | first45=A.

| last46=Müller | first46=S.

| last47=Mutschke | first47=H.

| last48=Nakagawa | first48=T.

| last49=Ribas | first49=I.

| last50=Walker | first50=H.

| title=DUst around NEarby Stars. The survey observational results

| journal=Astronomy & Astrophysics

| volume=555 | page=A11 | date=July 2013

| doi=10.1051/0004-6361/201321050 | bibcode=2013A&A...555A..11E | arxiv=1305.0155

| s2cid=377244 }}

{{cite journal

| display-authors=1 | last1=Rodriguez | first1=David R.

| last2=Duchêne | first2=Gaspard | last3=Tom | first3=Henry

| last4=Kennedy | first4=Grant M. | last5=Matthews | first5=Brenda

| last6=Greaves | first6=Jane | last7=Butner | first7=Harold

| title=Stellar multiplicity and debris discs: An unbiased sample

| journal=Monthly Notices of the Royal Astronomical Society

| volume=449 | issue=3 | pages=3160 | year=2015

| bibcode=2015MNRAS.449.3160R | doi=10.1093/mnras/stv483 | arxiv=1503.01320 | doi-access=free }}

}}