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WISE 0350−5658: Difference between revisions

Coordinates: Sky map 03h 50m 00.32s, −56° 58′ 30.2″
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|name=WISE J035000.32−565830.2}}
|name=WISE J035000.32−565830.2}}
{{Starbox observe
{{Starbox observe
⚫
|epoch=[[J2000]]<ref name="Kirkpatrick2012">{{cite journal | authorlink=J. Davy Kirkpatrick | last1=Kirkpatrick | last2=Gelino |first1=J. D. | first2=C. R. | last3=Cushing | first3=M. C. | last4=Mace | first4=G. N. | last5=Griffith | first5=R. L. | last6=Skrutskie | first6=M. F. | last7=Marsh | first7=K. A. | last8=Wright | first8=E. L. | last9=Eisenhardt | first9=P. R. | last10=McLean | first10=I. S. | last11=Mainzer | first11=A. K. | last12=Burgasser | first12=A. J. | last13=Tinney | first13=C. G. | last14=Parker | first14=S. | last15=Salter | first15=G. | title=Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function | year=2012 | journal=[[The Astrophysical Journal]] | volume=753 | issue=2 | pages=156 | arxiv=1205.2122 | doi=10.1088/0004-637X/753/2/156 | bibcode=2012ApJ...753..156K}}</ref>
|epoch=[[J2000]]{{r|Kirkpatrick2012}}
|equinox=[[J2000]]{{r|Kirkpatrick2012}}
|equinox=[[J2000]]{{r|Kirkpatrick2012}}
|constell=[[Reticulum]]
|constell=[[Reticulum]]
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}}
}}
{{Starbox astrometry
{{Starbox astrometry
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|prop_mo_ra={{val|-125|97}}<ref name="Marsh2013">{{cite journal | last=Marsh |first=Kenneth A. | author2=Wright, Edward L. | author3=Kirkpatrick, J. Davy | author4=Gelino, Christopher R. | author5=Cushing, Michael C. | author6=Griffith, Roger L. | author7=Skrutskie, Michael F. | author8=Eisenhardt, Peter R. | date=2013 | title=Parallaxes and Proper Motions of Ultracool Brown Dwarfs of Spectral Types Y and Late T | journal=[[The Astrophysical Journal]] | volume=762 | issue=2 | pages=119 | arxiv=1211.6977 | bibcode=2013ApJ...762..119M | doi=10.1088/0004-637X/762/2/119}}</ref>
|prop_mo_ra={{val|-125|97}}{{r|Marsh2013}}
|prop_mo_dec={{val|-865|76}}
|prop_mo_dec={{val|-865|76}}{{r|Marsh2013}}
|prop_mo_dec={{val|-865|76}}{{r|Marsh2013}}
|parallax=291
|parallax=291
|p_error=50
|p_error=50
|parallax_footnote={{r|Marsh2013}}
|parallax_footnote={{r|Marsh2013}}
|dist_pc={{val|3.44|+0.71|-0.50}}<ref name="Paterson2015"> Paterson, David.A. [http://www.keepandshare.com/doc15/6950/topicsinastronomytopic8 "Topics in Astronomy: Topic 8. Inappropriateness of the Lutz-Kelker equation for brown dwarfs"]. Retrieved on 24 September 2015.</ref>
|dist_pc={{val|3.7|+1.6|-0.4}}{{r|Marsh2013}}
|dist_ly={{val|12.1|+5.2|-1.3}}{{r|Marsh2013}}}}
|dist_ly={{val|11.2|+2.3|-1.6}}{{r|Paterson2015}}}}{{Starbox catalog
{{Starbox catalog
|names=[[Wide-field Infrared Survey Explorer|WISE]] J035000.32−565830.2,{{r|Kirkpatrick2012}}<br />[[Wide-field Infrared Survey Explorer|WISE]] 0350−5658{{r|Kirkpatrick2012}}}}
|names=[[Wide-field Infrared Survey Explorer|WISE]] J035000.32−565830.2,{{r|Kirkpatrick2012}}<br />[[Wide-field Infrared Survey Explorer|WISE]] 0350−5658{{r|Kirkpatrick2012}}}}
{{Starbox reference
{{Starbox reference
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{{Starbox end}}
{{Starbox end}}


'''WISE J035000.32−565830.2''' (designation abbreviated to '''WISE 0350−5658''') is a [[brown dwarf]] of [[spectral class]] Y1,{{r|Kirkpatrick2012}} located in constellation [[Reticulum]].<ref name="note 1" group="note">The nearest known [[star]]/[[brown dwarf]] in this constellation.</ref> Being approximately 12 [[light-year]]s from [[Earth]],{{r|Marsh2013}} it is one of the [[List of nearest stars|Sun's nearest neighbors]].
'''WISE J035000.32−565830.2''' (designation abbreviated to '''WISE 0350−5658''') is a [[brown dwarf]] of [[spectral class]] Y1,{{r|Kirkpatrick2012}} located in constellation [[Reticulum]], the nearest known [[star]]/[[brown dwarf]] in this constellation. Being approximately 11.2 [[light-year]]s from [[Earth]],{{r|Paterson2015}} it is one of the [[List of nearest stars|Sun's nearest neighbors]].


==Discovery==
==Discovery==
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==Distance==
==Distance==
WISE 0350−5658 is one of the nearest known brown dwarfs: its [[parallax|trigonometric parallax]], published by Marsh et al. (2013), is 0.291 ± 0.050 [[Arcsecond|arcsec]]ond, corresponding to a distance 3.7{{±|1.6|0.4}} [[parsec|pc]] (12.1{{±|5.2|1.3}} [[light-year|ly]]).{{r|Marsh2013}}<ref name="note 2" group="note"/>
WISE 0350−5658 is one of the nearest known brown dwarfs: its [[parallax|trigonometric parallax]] is 0.291 ± 0.050 [[Arcsecond|arcsec]]ond{{r|Marsh2013}}, corresponding to a direct inversion distance{{r|Paterson2015}} of 3.44{{±|0.71|0.5}} [[parsec|pc]] (11.2{{±|2.3|1.6}} [[light-year|ly]]).

{| class="wikitable"
|+ WISE 0350−5658 distance estimates
|-
! Source !! Parallax, [[milliarcsecond|mas]] !! Distance, [[parsec|pc]] !! Distance, [[light-year|ly]] !! Distance, [[petametre|Pm]] !! Ref.
{{πp|Marsh et al. (2013)<br>{{small|(according Kirkpatrick et al. (2012))}}|238|38|{{r|Kirkpatrick2012}}}}
{{πs|Marsh et al. (2013)|291|50|3.7|1.6|0.4|12.1|5.2|1.3|{{r|Marsh2013}}|c2=<ref name="note 2" group="note">In this parallax and distance estimates the most probable distance value does not equal to [[multiplicative inverse|inverse]] maximum likelihood parallax value, as would be in the case of exact parallax and distance values. This is because Marsh et al. used a more sophisticated method of converting maximum likelihood parallaxes into most probable distances, that uses also some [[a priori and a posteriori|prior]] information, and not just the calculation of the inverse value. (The method description see in Marsh et al. (2013), Section 4).</ref>|b=}}
|}

<small>Non-trigonometric distance estimates are marked in ''italic''. The {{abbr|most precise|Distance estimates from preliminary versions of e-prints or published only on web pages are not taken into account.}} estimate is marked in '''bold'''.</small>


==See also==
==See also==
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*[[WISE 0734−7157]] (Y0)
*[[WISE 0734−7157]] (Y0)
*[[WISE 2220−3628]] (Y0)
*[[WISE 2220−3628]] (Y0)

==Notes==
{{reflist|colwidth=30em|group=note}}


==References==
==References==
{{reflist|colwidth=30em|refs=
{{reflist}}
⚫
<ref name="Kirkpatrick2012">{{cite journal | authorlink=J. Davy Kirkpatrick | last1=Kirkpatrick | last2=Gelino |first1=J. D. | first2=C. R. | last3=Cushing | first3=M. C. | last4=Mace | first4=G. N. | last5=Griffith | first5=R. L. | last6=Skrutskie | first6=M. F. | last7=Marsh | first7=K. A. | last8=Wright | first8=E. L. | last9=Eisenhardt | first9=P. R. | last10=McLean | first10=I. S. | last11=Mainzer | first11=A. K. | last12=Burgasser | first12=A. J. | last13=Tinney | first13=C. G. | last14=Parker | first14=S. | last15=Salter | first15=G. | title=Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function | year=2012 | journal=[[The Astrophysical Journal]] | volume=753 | issue=2 | pages=156 | arxiv=1205.2122 | doi=10.1088/0004-637X/753/2/156 | bibcode=2012ApJ...753..156K}}</ref>
⚫
<ref name="Marsh2013">{{cite journal | last=Marsh |first=Kenneth A. | author2=Wright, Edward L. | author3=Kirkpatrick, J. Davy | author4=Gelino, Christopher R. | author5=Cushing, Michael C. | author6=Griffith, Roger L. | author7=Skrutskie, Michael F. | author8=Eisenhardt, Peter R. | date=2013 | title=Parallaxes and Proper Motions of Ultracool Brown Dwarfs of Spectral Types Y and Late T | journal=[[The Astrophysical Journal]] | volume=762 | issue=2 | pages=119 | arxiv=1211.6977 | bibcode=2013ApJ...762..119M | doi=10.1088/0004-637X/762/2/119}}</ref>
}}


{{nearest systems|3}}
{{nearest systems|3}}

Revision as of 05:19, 24 September 2015

WISE J035000.32−565830.2
Observation data
Epoch J2000[1]      Equinox J2000[1]
Constellation Reticulum
Right ascension 03h 50m 00.32s[1]
Declination −56° 58′ 30.2″[1]
Characteristics
Spectral type Y1[1]
Apparent magnitude (J (MKO-NIR filter system)) >22.8[1]
Apparent magnitude (H (MKO-NIR filter system)) >21.5[1]
Astrometry
Proper motion (μ) RA: −125±97[2] mas/yr
Dec.: −865±76[2] mas/yr
Parallax (π)291 ± 50 mas[2]
Distance11.2+2.3
−1.6[3] ly
(3.44+0.71
−0.50[3] pc)
Other designations
WISE J035000.32−565830.2,[1]
WISE 0350−5658[1]
Database references
SIMBADdata

WISE J035000.32−565830.2 (designation abbreviated to WISE 0350−5658) is a brown dwarf of spectral class Y1,[1] located in constellation Reticulum, the nearest known star/brown dwarf in this constellation. Being approximately 11.2 light-years from Earth,[3] it is one of the Sun's nearest neighbors.

Discovery

WISE 0350−5658 was discovered in 2012 by J. Davy Kirkpatrick and colleagues from data collected by the Wide-field Infrared Survey Explorer (WISE) in the infrared at a wavelength of 40 cm (16 in), whose mission lasted from December 2009 to February 2011. In 2012 Kirkpatrick et al. published a paper in The Astrophysical Journal, where they presented the discovery of seven new brown dwarfs of spectral type Y that had been found by WISE, among which was WISE 0350−5658.[1]

Distance

WISE 0350−5658 is one of the nearest known brown dwarfs: its trigonometric parallax is 0.291 ± 0.050 arcsecond[2], corresponding to a direct inversion distance[3] of 3.44+0.71
−0.5 pc (11.2+2.3
−1.6 ly).

See also

The other six discoveries of brown dwarfs, published in Kirkpatrick et al. (2012):[1]

References

  1. ^ a b c d e f g h i j k l Kirkpatrick, J. D.; Gelino, C. R.; Cushing, M. C.; Mace, G. N.; Griffith, R. L.; Skrutskie, M. F.; Marsh, K. A.; Wright, E. L.; Eisenhardt, P. R.; McLean, I. S.; Mainzer, A. K.; Burgasser, A. J.; Tinney, C. G.; Parker, S.; Salter, G. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal. 753 (2): 156. arXiv:1205.2122. Bibcode:2012ApJ...753..156K. doi:10.1088/0004-637X/753/2/156.
  2. ^ a b c d Marsh, Kenneth A.; Wright, Edward L.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Cushing, Michael C.; Griffith, Roger L.; Skrutskie, Michael F.; Eisenhardt, Peter R. (2013). "Parallaxes and Proper Motions of Ultracool Brown Dwarfs of Spectral Types Y and Late T". The Astrophysical Journal. 762 (2): 119. arXiv:1211.6977. Bibcode:2013ApJ...762..119M. doi:10.1088/0004-637X/762/2/119.
  3. ^ a b c d Paterson, David.A. "Topics in Astronomy: Topic 8. Inappropriateness of the Lutz-Kelker equation for brown dwarfs". Retrieved on 24 September 2015.
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