Wolf 489: Difference between revisions
m Fixing section headings (task 5) |
Kwamikagami (talk | contribs) m sp. using AWB |
||
Line 1: | Line 1: | ||
{{Sky|13|36|31.81|+|03|40|45.9|26.9}} |
{{Sky|13|36|31.81|+|03|40|45.9|26.9}} |
||
{{Starbox begin |
{{Starbox begin |
||
|name=[[ |
|name=[[Gliese–Jahreiß catalogue|Gliese]] 518}} |
||
{{Starbox observe |
{{Starbox observe |
||
|epoch=[[J2000]]<ref name="Simbad">{{cite web |
|epoch=[[J2000]]<ref name="Simbad">{{cite web |
||
Line 19: | Line 19: | ||
| title=A NEW LOOK AT THE LOCAL WHITE DWARF POPULATION |
| title=A NEW LOOK AT THE LOCAL WHITE DWARF POPULATION |
||
| journal=[[The Astronomical Journal]] |
| journal=[[The Astronomical Journal]] |
||
| volume=135 | |
| volume=135 | pages=1225–1238 |
||
| bibcode=2008AJ....135.1225H |
| bibcode=2008AJ....135.1225H |
||
| doi=10.1088/0004-6256/135/4/1225 |
| doi=10.1088/0004-6256/135/4/1225 |
||
Line 31: | Line 31: | ||
| title=THE WHITE DWARFS WITHIN 20 PARSECS OF THE SUN: KINEMATICS AND STATISTICS |
| title=THE WHITE DWARFS WITHIN 20 PARSECS OF THE SUN: KINEMATICS AND STATISTICS |
||
| journal=[[The Astronomical Journal]] |
| journal=[[The Astronomical Journal]] |
||
| volume=138 | |
| volume=138 | pages=1681–1689 |
||
| bibcode=2009AJ....138.1681S |
| bibcode=2009AJ....138.1681S |
||
| doi=10.1088/0004-6256/138/6/1681 |
| doi=10.1088/0004-6256/138/6/1681 |
||
Line 63: | Line 63: | ||
| 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>}} |
| 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 |
{{Starbox catalog |
||
|names=WD 1334+039<ref name="Holberg2008"/><ref name="Sion2009"/> |
|names=WD 1334+039,<ref name="Holberg2008"/><ref name="Sion2009"/> [[Max Wolf|Wolf]] 489,<ref name="Simbad"/> [[Luyten Half-Second catalogue|LHS]] 46,<ref name="Holberg2008"/> [[Luyten Five-Tenths catalogue|LFT]] 1023,<ref name="Simbad"/> [[Luyten Two-Tenths catalogue|LTT]] 13961,<ref name="Simbad"/> [[New Luyten Two-Tenths catalogue|NLTT]] 34618,<ref name="Simbad"/> [[Giclas|G]] 062-053,<ref name="Yale"/> [[Giclas|G]] 62-53,<ref name="Simbad"/> [[Giclas|G]] 64-4,<ref name="Simbad"/> EGGR 100,<ref name="Simbad"/> [[Two Micron All-Sky Survey|2MASS]] J13363181+0340458,<ref name="Simbad"/> USNO-B1.0 0936-00229354<ref name="Simbad"/>}} |
||
{{Starbox reference |
{{Starbox reference |
||
| Simbad=Gliese+518 |
| Simbad=Gliese+518 |
||
Line 82: | Line 82: | ||
| Woolley (1970) || [http://adsabs.harvard.edu/abs/1970ROAn....5.....W Woolley et al., 1970] || 135 ± 12 || 7.4 ± 0.7 || 24.2 ± 2.1 || <ref name="Wo">[http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=V/32A Stars within 25 pc of the Sun (Woolley+ 1970)]</ref> |
| Woolley (1970) || [http://adsabs.harvard.edu/abs/1970ROAn....5.....W Woolley et al., 1970] || 135 ± 12 || 7.4 ± 0.7 || 24.2 ± 2.1 || <ref name="Wo">[http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=V/32A Stars within 25 pc of the Sun (Woolley+ 1970)]</ref> |
||
|- |
|- |
||
| [[ |
| [[Gliese–Jahreiß catalogue|GJ]], 3rd version || [http://adsabs.harvard.edu/abs/1995yCat.5070....0G Gliese, Jahreiss, 1991] || 122.2 ± 3.9 || 8.18 ± 0.26 || 26.69 ± 0.85 || <ref name="GJ">[http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=V/70A Nearby Stars, Preliminary 3rd Version (Gliese+ 1991)]</ref> |
||
|- |
|- |
||
| 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"/> |
| 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"/> |
||
Line 89: | Line 89: | ||
==Physical parameters== |
==Physical parameters== |
||
Gliese 518'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> |
Gliese 518'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 km, or 143 % of [[Earth's radius|Earth's]]. |
||
Gliese 518'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"/> Despite Gliese 518 is classified as "white dwarf", it is not actually white, due low temperature, and should appear the same color as K-type main sequence stars, sometimes referred to as "[[orange dwarf]]s". |
Gliese 518'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"/> Despite Gliese 518 is classified as "white dwarf", it is not actually white, due low temperature, and should appear the same color as K-type main sequence stars, sometimes referred to as "[[orange dwarf]]s". |
Revision as of 17:02, 21 February 2012
Observation data Epoch J2000[1] Equinox J2000[1] | |
---|---|
Constellation | Template:Constel |
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: -3706[3] mas/yr Dec.: -1149[3] mas/yr |
Parallax (π) | 121.4 ± 3.4 mas[4] |
Distance | 26.9 ± 0.8 ly (8.2 ± 0.2 pc) |
Absolute magnitude (MV) | 15.08[2][4][note 1] |
Details | |
Mass | 0.55 ± 0.03[2] M☉ |
Radius | 0.013[2][note 2] R☉ |
Surface gravity (log g) | 7.95 ± 0.02[2] cgs |
Temperature | 5030 ± 120[2] K |
Age | 5.19[3][note 3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Gliese 518 (WD 1334+039, LHS 46, G 062-053, Wolf 489) 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 Template:Constel.
Distance
Gliese 518, 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,[4] corresponding to a distance 8.24 ± 0.23 pc, or 26.87 ± 0.75 ly.
Gliese 518 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 | [5] |
GJ, 3rd version | Gliese, Jahreiss, 1991 | 122.2 ± 3.9 | 8.18 ± 0.26 | 26.69 ± 0.85 | [6] |
YPC, 4th edition | van Altena et al., 1995 | 121.4 ± 3.4 | 8.24 ± 0.23 | 26.87 ± 0.75 | [4] |
Physical parameters
Gliese 518'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.
Gliese 518'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] Despite Gliese 518 is classified as "white dwarf", it is not actually white, due low temperature, and should appear the same color as K-type main sequence stars, sometimes referred to as "orange dwarfs".
Notes
References
- ^ a b c d e f g h i j k l m n o p q r s t "GJ 518 -- White Dwarf". Centre de Données astronomiques de Strasbourg. Retrieved 2011-11-02.
- ^ a b c d e f g h i j k l m
Holberg, J. B. (2008). "A NEW LOOK AT THE LOCAL WHITE DWARF POPULATION". The Astronomical Journal. 135: 1225–1238. Bibcode:2008AJ....135.1225H. doi:10.1088/0004-6256/135/4/1225.
{{cite journal}}
: Unknown parameter|coauthors=
ignored (|author=
suggested) (help) - ^ a b c d e f g
Sion, Edward M. (2009). "THE WHITE DWARFS WITHIN 20 PARSECS OF THE SUN: KINEMATICS AND STATISTICS". The Astronomical Journal. 138: 1681–1689. Bibcode:2009AJ....138.1681S. doi:10.1088/0004-6256/138/6/1681.
{{cite journal}}
: Unknown parameter|coauthors=
ignored (|author=
suggested) (help) - ^ a b c d e Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
- ^ Stars within 25 pc of the Sun (Woolley+ 1970)
- ^ Nearby Stars, Preliminary 3rd Version (Gliese+ 1991)