Skip to main content

HD 107914








HD 107914


From Wikipedia, the free encyclopedia

Jump to navigation
Jump to search




































































HD 107914

Observation data
Epoch J2000.0      Equinox J2000.0

Constellation

Centaurus

CCDM J12242-3855A

Right ascension
12h 24m 13.0s[1]

Declination
–38° 54′ 50″[1]

Apparent magnitude (V)
7.0[1]

CCDM J12242-3855B

Right ascension
12h 24m 13.2s[1]

Declination
–38° 54′ 47″[1]

Apparent magnitude (V)
12.8[1]
Characteristics

Spectral type
A7/8III[2]
B−V color index
0.272[3]
Astrometry
Proper motion (μ) RA: +0.55[4] mas/yr
Dec.: –0.02[4] mas/yr
Parallax (π) 12.77 ± 0.46 mas
Distance 255 ± 9 ly
(78 ± 3 pc)
Other designations
CCDM J12242-3855AB, CD−38° 7710, HIP 60503, HD 107914, SAO 203431
Database references
SIMBAD data

HD 107914 is a binary star in the constellation Centaurus, with an estimated distance of 255.5 light-years (78.3 pc)[5] from the Solar System. The primary has a stellar classification of A7-8 III, making it a giant star.


Measurement of the proper motion of this system show that it has a low transverse velocity relative to the Sun. For this reason, it has been compared to the hypothetical "Nemesis" star since it may pass through the Oort cloud in the future.[5] The star is too far away to be a companion to the Sun. However, preliminary measurements of the H-alpha line in the star's spectrum show a radial velocity in the range from –13 to +3 km/s. (This result was obtained by M. Muterspaugh and M. Williamson at a robotic spectroscopic telescope in Arizona.[6]) Such values for the radial velocity are too small to produce a likely collision course with the Solar System. For example, if Vr = –10 km/s, then the distance from the Sun to HD 107914 at closest approach will be about 5.2 ly (1.6 pc).



References[edit]





  1. ^ abcdef "CCDM J12242-3855. Vizier detailed page". Vizier. Centre de Données astronomiques de Strasbourg. Retrieved 2010-04-13..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}


  2. ^ "CCDM J12242-3855AB". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-04-13.


  3. ^ "HIP 60503. VizieR detailed page". Vizier. Centre de Données astronomiques de Strasbourg. Retrieved 2010-04-13.


  4. ^ ab "Detailed description of I/311". Hipparcos. Centre de Données astronomiques de Strasbourg. Retrieved 2010-04-13.


  5. ^ ab Potemine, Igor Yu. (2010-04-13). "Giant Nemesis candidate HD 107914 / HIP 60503 for the perforation of Oort cloud". arXiv:1003.5308 [astro-ph.SR].


  6. ^ Eaton, J. A.; Williamson M. H. (2007). "The Tennessee State University Automatic Spectroscopic Telescope: Data Processing and Velocity Variation of Cool Giants". Publications of the Astronomical Society of the Pacific. 119: 886–897. Bibcode:2007PASP..119..886E. doi:10.1086/521231.












Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_107914&oldid=832113493"





Navigation menu

























(window.RLQ=window.RLQ||).push(function(){mw.config.set({"wgPageParseReport":{"limitreport":{"cputime":"0.308","walltime":"0.386","ppvisitednodes":{"value":1144,"limit":1000000},"ppgeneratednodes":{"value":0,"limit":1500000},"postexpandincludesize":{"value":60727,"limit":2097152},"templateargumentsize":{"value":2153,"limit":2097152},"expansiondepth":{"value":14,"limit":40},"expensivefunctioncount":{"value":3,"limit":500},"unstrip-depth":{"value":1,"limit":20},"unstrip-size":{"value":16925,"limit":5000000},"entityaccesscount":{"value":3,"limit":400},"timingprofile":["100.00% 310.604 1 -total"," 50.29% 156.200 1 Template:Reflist"," 29.99% 93.139 4 Template:Cite_web"," 11.68% 36.271 1 Template:Starbox_observe_2s"," 10.36% 32.187 5 Template:Navbox"," 10.18% 31.617 2 Template:Convert"," 10.11% 31.392 1 Template:Cite_arXiv"," 9.01% 27.975 1 Template:Starbox_astrometry"," 8.33% 25.879 1 Template:Stars_of_Centaurus"," 7.45% 23.139 2 Template:DEC"]},"scribunto":{"limitreport-timeusage":{"value":"0.149","limit":"10.000"},"limitreport-memusage":{"value":4327838,"limit":52428800}},"cachereport":{"origin":"mw1333","timestamp":"20181027015029","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