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词条 Lambda Arae
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{{Starbox begin
| name = Lambda Arae
}}{{Starbox image
| image =

| caption = Location of λ Arae (circled)
}}{{Starbox observe
| epoch = J2000
| ra = {{RA|17|40|23.82481}}
| dec = {{DEC|–49|24|56.1015}}
| appmag_v = 4.77[3]
| constell = Ara
}}{{Starbox character
| class = F4 V[4]
| r-i = 0.22
| v-r =
| b-v = +0.40[3]
| u-b = –0.04[3]
| variable = 3.10[7]
}}{{Starbox astrometry
| radial_v = +3.6[7]
| prop_mo_ra = +103.22
| prop_mo_dec = –176.51
| parallax = 46.62
| p_error = 0.33
| parallax_footnote =
| absmag_v = +3.06[12]
}}{{Starbox detail
| mass =
| radius =
| luminosity = 4.6[13]
| temperature = 6,725[13]
| gravity = 4.15[13]
| metal_fe = –0.24[7]
| rotational_velocity = 15.5[17]
| age_gyr =
}}{{Starbox catalog
| names = CD –49° 11616, GJ 9597, HD 160032, HIP 86486, HR 6569, NSV 23218, NLTT 45187, SAO 228257.[18]
}}{{Starbox reference
| Simbad=lam+Ara
}}{{Starbox end}}

Lambda Arae (λ Ara, λ Arae) is the Bayer designation for a star in the southern constellation of Ara. It is at a distance of {{Convert|70.0|ly|pc|abbr=off|lk=on}} from Earth. The apparent visual magnitude of this star is 4.77,[3] making it bright enough to be seen with the naked eye.

The spectrum of this star matches a stellar classification of F4 V,[4] which places it among the category of F-type main sequence stars. It shines with 4.6 times the luminosity of the Sun. The outer atmosphere is radiating this energy at an effective temperature of 6,725 K,[13] giving it the yellow-white hue of an F-type star. There is some evidence that this may be a binary star system consisting of two stars with identical masses.[17]

Examination of Lambda Arae with the Spitzer Space Telescope shows an excess of infrared emission at a wavelength of 70 μm. This suggests it may be orbited by a disk of dust at a radius of more than 15 astronomical units[24]

References

1. ^{{citation | last1=Ammler-von Eiff | first1=M. | last2=Reiners | first2=A. | title=New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars? | journal=Astronomy & Astrophysics | arxiv=1204.2459 | volume=542 | page=A116 | date=June 2012 | postscript=. | doi=10.1051/0004-6361/201118724 | bibcode=2012A&A...542A.116A }}
2. ^{{citation | last1=Mallik | first1=Sushma V. | title=Lithium abundance and mass | journal=Astronomy and Astrophysics | volume=352 | pages=495–507 |date=December 1999 | bibcode=1999A&A...352..495M }}
3. ^{{citation | 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=161–170 |date=July 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | postscript=. }}
4. ^{{citation | last1=Holmberg | first1=J. | last2=Nordstrom | first2=B. | last3=Andersen | first3=J. | title=The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics | journal=Astronomy and Astrophysics | volume=501 | issue=3 |date=July 2009 | pages=941–947 | doi=10.1051/0004-6361/200811191 | bibcode=2009A&A...501..941H | postscript=. |arxiv = 0811.3982 }}
5. ^{{citation | last1=Johnson | display-authors=1 | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | year=1966 | bibcode=1966CoLPL...4...99J | postscript=. }}
6. ^{{citation | display-authors=1 | last1=Fuhrmann | first1=K. | last2=Chini | first2=R. | last3=Hoffmeister | first3=V. H. | last4=Stahl | first4=O. | title=Evidence for the nearby F4V star λ Ara as a binary system | journal=Monthly Notices of the Royal Astronomical Society | volume=415 | issue=2 | pages=1240–1243 |date=August 2011 | doi=10.1111/j.1365-2966.2011.18764.x | bibcode=2011MNRAS.415.1240F | postscript=. }}
7. ^{{cite simbad | title=lam Ara | accessdate=2010-07-30 | postscript=. }}
8. ^{{citation | display-authors=1 | last1=Lawler | first1=S. M. | last2=Beichman | first2=C. A. | last3=Bryden | first3=G. | last4=Ciardi | first4=D. R. | last5=Tanner | first5=A. M. | last6=Su | first6=K. Y. L. | last7=Stapelfeldt | first7=K. R. | last8=Lisse | first8=C. M. | last9=Harker | first9=D. E. | title=Explorations Beyond the Snow Line: Spitzer/IRS Spectra of Debris Disks Around Solar-type Stars | journal=The Astrophysical Journal | volume=705 | issue=1 | pages=89–111 |date=November 2009 | doi=10.1088/0004-637X/705/1/89 | bibcode=2009ApJ...705...89L |arxiv = 0909.0058 }}
[1][2][3][4][5][6][7][8]
}}

External links

  • HR 6569
  • Image Lambda Arae
{{Stars of Ara}}

8 : Henry Draper Catalogue objects|Bayer objects|Ara (constellation)|F-type subgiants|Hipparcos objects|Gliese and GJ objects|HR objects|Durchmusterung objects

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