Skip to main content

20 Boötis









20 Boötis


From Wikipedia, the free encyclopedia

Jump to navigation
Jump to search









































































































20 Boötis

Observation data
Epoch J2000      Equinox J2000

Constellation

Boötes

Right ascension
14h 19m 45.23479s[1]

Declination
+16° 18′ 25.0136″[1]

Apparent magnitude (V)
4.85
Characteristics

Spectral type
K3 III
U−B color index
1.4
B−V color index
1.23
R−I color index
0.6
Astrometry
Radial velocity (Rv) –7.64 km/s
Proper motion (μ) RA: –141.56[1] mas/yr
Dec.: +60.48[1] mas/yr
Parallax (π) 17.44 ± 0.22[1] mas
Distance 187 ± 2 ly
(57.3 ± 0.7 pc)
Absolute magnitude (MV)
1.01 ± 0.09[2]
Details
Mass
1.14 ± 0.19[2] M
Radius
11.3 ± 0.5[2] R
Surface gravity (log g)
2.36 ± 0.08[2] cgs
Temperature 4,472[2] K

Metallicity [Fe/H]
0.16[2] dex
Rotation 848 days[3]
Rotational velocity (v sin i) 1.0[3] km/s
Age
5.21 ± 2.28[2] Gyr
Other designations
HR 5370, HD 125560, BD+16°2637, FK5 3135, HIP 70027, SAO 100980, GC 19334.
Database references
SIMBAD data

20 Boötis is a star in the constellation Boötes.


20 Boötis is an orange K-type giant with an apparent magnitude of +4.85. It is approximately 187 light years from Earth.



References[edit]





  1. ^ abcde van Leeuwen, F. (November 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}


  2. ^ abcdefg da Silva, L.; et al. (November 2006), "Basic physical parameters of a selected sample of evolved stars", Astronomy and Astrophysics, 458 (2): 609–623, arXiv:astro-ph/0608160, Bibcode:2006A&A...458..609D, doi:10.1051/0004-6361:20065105


  3. ^ ab Setiawan, J.; et al. (July 2004), "Precise radial velocity measurements of G and K giants. Multiple systems and variability trend along the Red Giant Branch", Astronomy and Astrophysics, 421: 241–254, Bibcode:2004A&A...421..241S, doi:10.1051/0004-6361:20041042-1




External links[edit]



  • HR 5370

  • Image 20 Boötis

















Retrieved from "https://en.wikipedia.org/w/index.php?title=20_Boötis&oldid=799402486"





Navigation menu

























(window.RLQ=window.RLQ||).push(function(){mw.config.set({"wgPageParseReport":{"limitreport":{"cputime":"0.336","walltime":"0.415","ppvisitednodes":{"value":1314,"limit":1000000},"ppgeneratednodes":{"value":0,"limit":1500000},"postexpandincludesize":{"value":101643,"limit":2097152},"templateargumentsize":{"value":2835,"limit":2097152},"expansiondepth":{"value":14,"limit":40},"expensivefunctioncount":{"value":3,"limit":500},"unstrip-depth":{"value":1,"limit":20},"unstrip-size":{"value":11768,"limit":5000000},"entityaccesscount":{"value":3,"limit":400},"timingprofile":["100.00% 271.942 1 -total"," 47.97% 130.463 1 Template:Reflist"," 40.87% 111.133 3 Template:Citation"," 11.42% 31.063 1 Template:Starbox_observe"," 10.03% 27.266 4 Template:Navbox"," 8.99% 24.458 1 Template:Stars_of_Boötes"," 8.79% 23.900 1 Template:Starbox_astrometry"," 7.58% 20.617 1 Template:DEC"," 6.74% 18.316 1 Template:Str_rep"," 6.44% 17.504 1 Template:Starbox_character"]},"scribunto":{"limitreport-timeusage":{"value":"0.113","limit":"10.000"},"limitreport-memusage":{"value":3966258,"limit":52428800}},"cachereport":{"origin":"mw1246","timestamp":"20181121112946","ttl":1900800,"transientcontent":false}}});mw.config.set({"wgBackendResponseTime":128,"wgHostname":"mw1274"});});

Popular posts from this blog

Full-time equivalent

Bicuculline

さくらももこ