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词条 54 Leonis
释义

  1. References

{{Starbox begin
| name = 54 Leonis
}}{{Starbox observe 2s
| epoch = J2000.0
| equinox =
| constell = Leo
| component1 = 54 Leo A
| ra1 = {{RA|10|55|36.80266}}[1]
| dec1 = {{DEC|+24|44|59.0440}}[1]
| appmag_v1 = 4.477[3]
| component2 = 54 Leo B
| ra2 = {{RA|10|55|37.24836}}[4]
| dec2 = {{DEC|+24|44|56.5478}}[4]
| appmag_v2 = 6.29[6]
}}{{Starbox character
| component1 = 54 Leo A
| class = A0 V[7]
| b-v = +0.001[7]
| component2 = 54 Leo B
| class2 = A2 Vn[7]
| b-v2 = +0.07[6]
}}{{Starbox astrometry
| component1 = 54 Leo A
| radial_v = {{Val|−0.49|0.98}}[11]
| prop_mo_ra = −78.057[1]
| prop_mo_dec = −16.520[1]
| parallax = 9.8275
| p_error = 0.3537
| parallax_footnote = [1]
| absmag_v = –0.29[15]
| component2 = 54 Leo B
| radial_v2 = {{Val|1.30|0.92}}[11]
| prop_mo_ra2 = −75.374[4]
| prop_mo_dec2 = −18.595[4]
| parallax2 = 10.1748
| p_error2 = 0.0569
| parallax_footnote2 = [4]
| absmag_v2 =
}}{{Starbox detail
| source =
| component1 = 54 Leo A
| mass = {{Val|2.4|0.44|0.36}}[20]
| radius = 2.88[21]
| luminosity =
| gravity = {{Val|3.5|0.25}}[20]
| temperature = {{Val|9000|500}}[20]
| metal_fe =
| rotational_velocity = 185[24]
| age_myr = {{Val|411|137|168}}[20]
| component2 = 54 Leo B
| mass2 =
| radius2 = 2.59[21]
| luminosity2 =
| gravity2 =
| temperature2 =
| metal2_fe =
| rotational_velocity2 = {{Val|250|20}}[21]
| age_gyr2 =
}}{{Starbox catalog
| names = 54 Leo, BD+25 2314, CCDM J10556+2445, HIP 53417, Struve 1487
| component1 = 54 Leo A
| names1 = HD 94601, HR 4259, SAO 81583
| component2 = 54 Leo B
| names2 = HD 94602, HR 4260, SAO 81584
}}{{Starbox reference
| Simbad=54+Leo
}}{{Starbox end}}54 Leonis is a binary star[29] system in the zodiac constellation of Leo, located around 321[4] light years from the Sun. It is visible to the naked eye as a faint, white-hued star with a combined apparent visual magnitude of 4.30.[31] As of 2017, the pair had an angular separation of {{val|6.60|ul=arcsecond}} along a position angle of 113°.[32] They have a physical separation of around {{Convert|533|AU|Gm|lk=on|abbr=on}}.[21]

The magnitude 4.477[3] primary, designated component A, is an A-type main-sequence star with a stellar classification of A0 V,[7] which indicates it is generating energy through hydrogen fusion at its core. It has a high rate of spin, showing a projected rotational velocity of 185 km/s. This is giving the star an oblate shape with an equatorial bulge that is an estimated 8% larger than the polar radius.[24] The star

is roughly 411[20] million years old with 2.4[20] times the mass of the Sun and about 2.88[21] times the Sun's radius.

The fainter magnitude 6.29[6] secondary, component B, is a smaller A-type main-sequence star with a class of A2 Vn.[7] The 'n' suffix indicates wide "nebulous" lines due to rapid rotation. It is spinning with an even higher projected rotational velocity of 250[21] km/s. The star has about 2.59[21] times the Sun's radius.

Asteroid 729 Watsonia occulted HIP 53417 on March 3, 2013 at 01:48.[44]

References

1. ^{{cite book|author=Pier Paolo Ricci|title=Almanacco astronomico 2013 Astronomical almanac 2013|url=https://books.google.com/books?id=xG0CBAAAQBAJ&pg=PA322|date=29 November 2012|publisher=Lulu.com|isbn=978-1-291-21157-3|pages=322–}}
2. ^{{cite DR2|3996208310033740160}}
3. ^{{cite DR2|3996208310033739520}}
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9. ^{{citation | last1=Pizzolato | first1=N. | last2=Maggio | first2=A. | last3=Sciortino | first3=S. | title=Evolution of X-ray activity of 1-3 Msun late-type stars in early post-main-sequence phases | journal=Astronomy and Astrophysics | volume=361 | pages=614–628 | date=September 2000 | bibcode=2000A&A...361..614P }}
10. ^{{citation | display-authors=1 | last1=Cowley | first1=A. | last2=Cowley | first2=C. | last3=Jaschek | first3=M. | last4=Jaschek | first4=C. | title=A study of the bright A stars. I. A catalogue of spectral classifications | journal=Astronomical Journal | postscript=. | volume=74 | pages=375–406 | date=April 1969 | doi=10.1086/110819 | bibcode=1969AJ.....74..375C }}
11. ^{{citation | title=The Tycho-2 catalogue of the 2.5 million brightest stars | journal=Astronomy and Astrophysics | postscript=. | last1=Høg | first1=E. | last2=Fabricius | first2=C. | last3=Makarov | first3=V. V. | last4=Urban | first4=S. | last5=Corbin | first5=T. | last6=Wycoff | first6=G. | last7=Bastian | first7=U. | last8=Schwekendiek | first8=P. | last9=Wicenec | first9=A. | display-authors=1 | volume=355 | pages=L27 | year=2000 | doi=10.1888/0333750888/2862 | bibcode=2000A&A...355L..27H }}
12. ^{{citation | title=The Tycho double star catalogue | last1=Fabricius | first1=C. | last2=Høg | first2=E. | last3=Makarov | first3=V. V. | last4=Mason | first4=B. D. | last5=Wycoff | first5=G. L. | last6=Urban | first6=S. E. | display-authors=1 | journal=Astronomy and Astrophysics | volume=384 | pages=180–189 | year=2002 | bibcode=2002A&A...384..180F | doi=10.1051/0004-6361:20011822 }}
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[1][2][3][4][5][6][7][8][9][10][11][12][13][14]
}}{{Stars of Leo}}

8 : A-type main-sequence stars|Binary stars|Leo (constellation)|Durchmusterung objects|Flamsteed objects|Hipparcos objects|Henry Draper Catalogue objects|HR objects

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