Wolf 489: Difference between revisions

Coordinates: Sky map 13h 36m 31.81s, +03° 40′ 45.9″
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{{Short description|Star in the constellation Virgo}}
{{Sky|13|36|31.81|+|03|40|45.9|26.9}}
{{Starbox begin
[[es:|name=Wolf 489]]}}
|name=[[Gliese–Jahreiß catalogue|Gliese]] 518}}
{{Starbox observe
|epoch=[[J2000]]<ref name="Simbad">{{cite web
Line 7 ⟶ 8:
| title =GJ 518 -- White Dwarf
| publisher=[[Centre de Données astronomiques de Strasbourg]]
| accessdateaccess-date=2011-11-02}}</ref>
|equinox=[[J2000]]<ref name="Simbad"/>
|constell={{Constel[[Virgo (constellation)|Vir}}Virgo]]
|ra={{RA|13|36|31.81}}<ref name="Simbad"/>
|dec={{DEC|+03|40|45.}}<ref name="Simbad"/>
Line 15 ⟶ 16:
{{cite journal
| last=Holberg |first=J. B.
| coauthorsauthor2=Sion; |author3=Oswalt; |author4=McCook; |author5=Foran; |author6= Subasavage
|title=A New Look at the Local White Dwarf Population
| year=2008
| title=A NEW LOOK AT THE LOCAL WHITE DWARF POPULATION
| journal=[[The Astronomical Journal]]
| volume=135 |issue=4
| pages=1225–1238
| bibcode=2008AJ....135.1225H
| doi=10.1088/0004-6256/135/4/1225
|s2cid=122855486
}}</ref>}}
| url=https://commons.erau.edu/cgi/viewcontent.cgi?article=1948&context=publication}}</ref>}}
{{Starbox character
|class=DZ10.0<ref name="Holberg2008"/><ref name="Sion2009">
{{cite journal
| last=Sion |first=Edward M.
|coauthorsauthor2=Holberg; |author3=Oswalt; |author4=McCook; |author5= Wasatonic
|title=The White Dwarfs within 20 Parsecs of the Sun: Kinematics and Statistics
| year=2009
| title=THE WHITE DWARFS WITHIN 20 PARSECS OF THE SUN: KINEMATICS AND STATISTICS
| journal=[[The Astronomical Journal]]
| volume=138 |issue=6
| pages=1681–1689
| bibcode=2009AJ....138.1681S
| doi=10.1088/0004-6256/138/6/1681
|arxiv = 0910.1288 |s2cid=119284418
}}</ref>
}}</ref>}}
|appmag_1_passband=B
|appmag_1=15.59<ref name="Simbad"/>
Line 50 ⟶ 55:
|appmag_7=12.69<ref name="Simbad"/>}}
{{Starbox astrometry
|prop_mo_ra=-37063735.839<ref name="Sion2009"EDR3>{{Cite Gaia EDR3|3713594960831605760}}</ref>
|prop_mo_dec=-11491113.581<ref name="Sion2009"EDR3/>
|parallax=121119.47566
|p_error=30.40304
|parallax_footnote=<ref name=EDR3/>
|parallax_footnote=<ref name="Yale">[http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=I/238 Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)]</ref>
| absmag_v=15.08<ref name="Holberg2008"/><ref name="Yale">[http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=I/238 Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)]</ref><ref name="note 1" group="note">From apparent magnitude and parallax.</ref>}}
{{Starbox detail
| mass=0.55 ± 0.03<ref name="Holberg2008"/>
Line 63 ⟶ 68:
| age_gyr=5.19<ref name="Sion2009"/><ref name="note 3" group="note">White dwarf cooling age, i. e. age as degenerate star (not including lifetime as main sequence star and as giant star)</ref>}}
{{Starbox catalog
|names=WD 1334+039,<ref name="Holberg2008"/><ref name="Sion2009"/> [[Max Wolf|Wolf]]&nbsp;489,<ref name="Simbad"/> [[Gliese catalogue|Gliese]]&nbsp;518,<ref name="Simbad"/> [[Luyten Half-Second catalogue|LHS]]&nbsp;46,<ref name="Holberg2008"/> [[Luyten Five-Tenths catalogue|LFT]]&nbsp;1023,<ref name="Simbad"/> [[Luyten Two-Tenths catalogue|LTT]]&nbsp;13961,<ref name="Simbad"/> [[New Luyten Two-Tenths catalogue|NLTT]]&nbsp;34618,<ref name="Simbad"/> [[Giclas|G]]&nbsp;062-053,<ref name="Yale"/> [[Giclas|G]]&nbsp;62-53,<ref name="Simbad"/> [[Giclas|G]]&nbsp;64-4,<ref name="Simbad"/> EGGR 100,<ref name="Simbad"/> [[Two Micron All-Sky Survey|2MASS]]&nbsp;J13363181+0340458,<ref name="Simbad"/> USNO-B1.0 0936-00229354<ref name="Simbad"/>}}
{{Starbox reference
| Simbad=Gliese+518
Line 69 ⟶ 74:
{{Starbox end}}
 
'''GlieseWolf 518489''' ('''WD 1334+039''', '''LHS 46''', '''G 062-053''', '''WolfGliese 489518''') is a nearby degenerate star ([[white dwarf]]) of spectral class DZ10.0<ref name="Holberg2008"/><ref name="Sion2009"/>), the single known component of the system, located in the constellation {{Constel[[Virgo (constellation)|Vir}}Virgo]].
 
==Distance==
 
GlieseWolf 518489, probably, is the 12th closest white dwarf, or, possibly, 9th–14th (see [[Gliese 293]], [[GJ 1087]], [[Gliese 915]], [[GJ 1276]] and [[Gliese 318]]). Its [[parallax|trigonometric parallax]] from YPC (Yale Parallax Catalog) is 121.4 ± 3.4 [[milliarcsecond|mas]],<ref name="Yale"/> corresponding to a distance 8.24 ± 0.23 [[parsec|pc]], or 26.87 ± 0.75 [[light-year|ly]].
 
'''Gliese 518 parallax data'''
{| class="wikitable"
'''Gliese|+ 518Wolf 489 parallax data'''
|-
! Source !! Paper !! Parallax, [[milliarcsecond|mas]] !! Distance, [[parsec|pc]] !! Distance, [[light-year|ly]] !! Ref.
Line 85 ⟶ 90:
|-
| YPC, 4th edition|| [http://adsabs.harvard.edu/abs/1995GCTP..C......0V van Altena et al., 1995] || 121.4 ± 3.4 || 8.24 ± 0.23 || 26.87 ± 0.75 || <ref name="Yale"/>
|-
| Gaia EDR3, 2020|| - || 119.7566±0.0304 || 8.3503±0.0002 || 27.235±0.007|| <ref name=EDR3/>
|}
 
==Physical parameters==
 
GlieseWolf 518489's mass is 0.55 ± 0.03 [[Solar mass]]es,<ref name="Holberg2008"/> its [[surface gravity]] is 10<sup>7.95 ± 0.02</sup> (8.91 · 10<sup>7</sup>) cm·s<sup>−2</sup>,<ref name="Holberg2008"/> or approximately 91 000 of [[Earth's gravity|Earth's]], corresponding to a radius 9089&nbsp;km, or 143 % of [[Earth's radius|Earth's]].
 
GlieseWolf 518489's temperature is 5030 ± 120 [[Kelvin degree|K]]<ref name="Holberg2008"/> (comparable with that of early [[K-type main sequence star]]s); its cooling age, i. e. age as degenerate star (not including lifetime as main sequence star and as giant star) is 5.19 [[Gigayear|Gyr]].<ref name="Sion2009"/> DespiteWolf Gliese489 518and isshould classifiedappear as "white dwarf",with ita isslight notshade actuallyof whiteyellow, due low temperature, and should appearnealy the same color as a K-type main sequence stars, sometimes referred to as "[[orange dwarf]]s"star.
 
==Notes==
<references group="note"/>
 
==See also==
* [[List of star systems within 25–30 light-years]]
 
==References==
{{reflist|colwidth=30em}}
 
{{Nearest star systems|6}}
{{Stars of Virgo}}
 
{{DEFAULTSORT:Wolf 489}}
[[Category:White dwarf starsdwarfs]]
[[Category:Virgo (constellation)]]
[[Category:Gliese and GJ objects|0518]]
[[Category:2MASS objects|J13363181+0340458]]
 
[[es:Wolf 489]]
[[it:Gliese 518]]

Latest revision as of 07:48, 27 February 2023

Wolf 489
Observation data
Epoch J2000[1]      Equinox J2000[1]
Constellation Virgo
Right ascension 13h 36m 31.81s[1]
Declination +03° 40′ 45.″[1]
Apparent magnitude (V) 14.66[2]
Characteristics
Spectral type DZ10.0[2][3]
Apparent magnitude (B) 15.59[1]
Apparent magnitude (V) 14.63[1]
Apparent magnitude (R) 14.0[1]
Apparent magnitude (I) 14.1[1]
Apparent magnitude (J) 13.06[1]
Apparent magnitude (H) 12.82[1]
Apparent magnitude (K) 12.69[1]
Astrometry
Proper motion (μ) RA: -3735.839[4] mas/yr
Dec.: -1113.581[4] mas/yr
Parallax (π)119.7566 ± 0.0304 mas[4]
Distance27.235 ± 0.007 ly
(8.350 ± 0.002 pc)
Absolute magnitude (MV)15.08[2][5][note 1]
Details
Mass0.55 ± 0.03[2] M
Radius0.013[2][note 2] R
Surface gravity (log g)7.95 ± 0.02[2] cgs
Temperature5030 ± 120[2] K
Age5.19[3][note 3] Gyr
Other designations
WD 1334+039,[2][3] Wolf 489,[1] Gliese 518,[1] LHS 46,[2] LFT 1023,[1] LTT 13961,[1] NLTT 34618,[1] G 062-053,[5] G 62-53,[1] G 64-4,[1] EGGR 100,[1] 2MASS J13363181+0340458,[1] USNO-B1.0 0936-00229354[1]
Database references
SIMBADdata

Wolf 489 (WD 1334+039, LHS 46, G 062-053, Gliese 518) is a nearby degenerate star (white dwarf) of spectral class DZ10.0[2][3]), the single known component of the system, located in the constellation Virgo.

Distance[edit]

Wolf 489, probably, is the 12th closest white dwarf, or, possibly, 9th–14th (see Gliese 293, GJ 1087, Gliese 915, GJ 1276 and Gliese 318). Its trigonometric parallax from YPC (Yale Parallax Catalog) is 121.4 ± 3.4 mas,[5] corresponding to a distance 8.24 ± 0.23 pc, or 26.87 ± 0.75 ly.

Wolf 489 parallax data
Source Paper Parallax, mas Distance, pc Distance, ly Ref.
Woolley (1970) Woolley et al., 1970 135 ± 12 7.4 ± 0.7 24.2 ± 2.1 [6]
GJ, 3rd version Gliese, Jahreiss, 1991 122.2 ± 3.9 8.18 ± 0.26 26.69 ± 0.85 [7]
YPC, 4th edition van Altena et al., 1995 121.4 ± 3.4 8.24 ± 0.23 26.87 ± 0.75 [5]
Gaia EDR3, 2020 - 119.7566±0.0304 8.3503±0.0002 27.235±0.007 [4]

Physical parameters[edit]

Wolf 489's mass is 0.55 ± 0.03 Solar masses,[2] its surface gravity is 107.95 ± 0.02 (8.91 · 107) cm·s−2,[2] or approximately 91 000 of Earth's, corresponding to a radius 9089 km, or 143% of Earth's.

Wolf 489's temperature is 5030 ± 120 K[2] (comparable with that of early K-type main sequence stars); its cooling age, i. e. age as degenerate star (not including lifetime as main sequence star and as giant star) is 5.19 Gyr.[3] Wolf 489 and should appear white with a slight shade of yellow, nealy the same color as a K-type main sequence star.

Notes[edit]

  1. ^ From apparent magnitude and parallax.
  2. ^ From surface gravity and mass.
  3. ^ White dwarf cooling age, i. e. age as degenerate star (not including lifetime as main sequence star and as giant star)

See also[edit]

References[edit]

  1. ^ a b c d e f g h i j k l m n o p q r s t u "GJ 518 -- White Dwarf". Centre de Données astronomiques de Strasbourg. Retrieved 2011-11-02.
  2. ^ a b c d e f g h i j k l m Holberg, J. B.; Sion; Oswalt; McCook; Foran; Subasavage (2008). "A New Look at the Local White Dwarf Population". The Astronomical Journal. 135 (4): 1225–1238. Bibcode:2008AJ....135.1225H. doi:10.1088/0004-6256/135/4/1225. S2CID 122855486.
  3. ^ a b c d e Sion, Edward M.; Holberg; Oswalt; McCook; Wasatonic (2009). "The White Dwarfs within 20 Parsecs of the Sun: Kinematics and Statistics". The Astronomical Journal. 138 (6): 1681–1689. arXiv:0910.1288. Bibcode:2009AJ....138.1681S. doi:10.1088/0004-6256/138/6/1681. S2CID 119284418.
  4. ^ a b c d Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  5. ^ a b c d Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
  6. ^ Stars within 25 pc of the Sun (Woolley+ 1970)
  7. ^ Nearby Stars, Preliminary 3rd Version (Gliese+ 1991)