Skip to main content

HD 111968








HD 111968


From Wikipedia, the free encyclopedia

Jump to navigation
Jump to search














































































n Centauri

Observation data
Epoch J2000.0      Equinox J2000.0

Constellation

Centaurus

Right ascension
12h 53m 26.20s[1]

Declination
−40° 10′ 43.9″[1]

Apparent magnitude (V)
+4.25
Characteristics

Spectral type
A7III
U−B color index
+0.12
B−V color index
+0.22[2]

Variable type
none
Astrometry
Proper motion (μ) RA: 7001708400000000000♠+70.84±0.14[1] mas/yr
Dec.: 2998774600000000000♠−22.54±0.10[1] mas/yr
Parallax (π) 21.95 ± 0.19[1] mas
Distance 149 ± 1 ly
(45.6 ± 0.4 pc)
Absolute magnitude (MV) +0.86[2]
Details
Temperature 7,648[2] K
Rotational velocity (v sin i)
7001924000000000000♠92.4±4.6[2] km/s
Other designations
n Cen, CD−39° 7893, FK5 482, GC 17489, GJ 488.1, HD 111968, HIP 62896, HR 4889, SAO 203907
Database references
SIMBAD data

HD 111968, also known by the Bayer designation n Centauri (n Cen), is a star in the constellation Centaurus.


n Centauri is a white A-type giant with an apparent magnitude of +4.25. It is approximately 149 light years from Earth.



References[edit]





  1. ^ abcde van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357..mw-parser-output cite.citation{font-style:inherit}.mw-parser-output q{quotes:"""""""'""'"}.mw-parser-output code.cs1-code{color:inherit;background:inherit;border:inherit;padding:inherit}.mw-parser-output .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-limited a,.mw-parser-output .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Lock-gray-alt-2.svg/9px-Lock-gray-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Lock-red-alt-2.svg/9px-Lock-red-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration{color:#555}.mw-parser-output .cs1-subscription span,.mw-parser-output .cs1-registration span{border-bottom:1px dotted;cursor:help}.mw-parser-output .cs1-hidden-error{display:none;font-size:100%}.mw-parser-output .cs1-visible-error{font-size:100%}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration,.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left,.mw-parser-output .cs1-kern-wl-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right,.mw-parser-output .cs1-kern-wl-right{padding-right:0.2em}
    Vizier catalog entry



  2. ^ abcd Ammler-von Eiff, M.; Reiners, A. (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv:1204.2459, Bibcode:2012A&A...542A.116A, doi:10.1051/0004-6361/201118724.














Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_111968&oldid=800811826"





Navigation menu

























(window.RLQ=window.RLQ||).push(function(){mw.config.set({"wgPageParseReport":{"limitreport":{"cputime":"0.368","walltime":"0.465","ppvisitednodes":{"value":1402,"limit":1000000},"ppgeneratednodes":{"value":0,"limit":1500000},"postexpandincludesize":{"value":65134,"limit":2097152},"templateargumentsize":{"value":3328,"limit":2097152},"expansiondepth":{"value":14,"limit":40},"expensivefunctioncount":{"value":3,"limit":500},"unstrip-depth":{"value":1,"limit":20},"unstrip-size":{"value":8151,"limit":5000000},"entityaccesscount":{"value":4,"limit":400},"timingprofile":["100.00% 384.854 1 -total"," 32.05% 123.328 1 Template:Reflist"," 23.73% 91.316 1 Template:Cite_journal"," 22.62% 87.059 1 Template:About-distinguish"," 16.95% 65.241 1 Template:Starbox_astrometry"," 11.09% 42.666 3 Template:Val"," 7.34% 28.258 5 Template:Navbox"," 6.21% 23.918 1 Template:Stars_of_Centaurus"," 5.20% 20.008 1 Template:Starbox_observe"," 4.32% 16.609 1 Template:Starbox_character"]},"scribunto":{"limitreport-timeusage":{"value":"0.189","limit":"10.000"},"limitreport-memusage":{"value":5277352,"limit":52428800}},"cachereport":{"origin":"mw1275","timestamp":"20181026180248","ttl":1900800,"transientcontent":false}}});mw.config.set({"wgBackendResponseTime":114,"wgHostname":"mw1324"});});

Popular posts from this blog

Full-time equivalent

Bicuculline

さくらももこ