请输入您要查询的百科知识：

　

词条 WISE 1828+2650
释义

  1. History of observations

      Discovery  

  2. Distance

  3. Proper motion

  4. Physical properties

      Possible binarity    Comparison  

  5. See also

  6. Notes

  7. References

  8. External links

{{Sky|18|28|31.10|+|26|50|37.79|36.5}}{{Starbox begin
| name=WISEPA J182831.08+265037.8}}{{Starbox image
| image =

| caption ={{longitem|WISE 1828+2650 is circled in the centre
(Infrared image from the WISE space telescope).|style=margin:-15px -15px 6px -15px; font-size: 1.2em;}}
}}{{Starbox observe
| epoch=MJD 55467.61{{r|Kirkpatrick2011}}
| equinox=J2000{{r|Kirkpatrick2011}}
| constell=Lyra
| ra={{RA|18|28|31.10}}{{r|Kirkpatrick2011}}
| dec={{DEC|26|50|37.79}}{{r|Kirkpatrick2011}}}}{{Starbox character
|class=>Y2{{r|Beichman2013}}
|appmag_1_passband=J {{small|(MKO filter system)}}
|appmag_1=23.57 ± 0.35{{r|Kirkpatrick2011}}
|appmag_2_passband=H {{small|(MKO filter system)}}
|appmag_2=22.45 ± 0.08{{r|Beichman2013}}}}{{Starbox astrometry
|prop_mo_ra={{nowrap|954 ± 11{{r|Beichman2013}}}}
|prop_mo_dec={{nowrap|153 ± 12.5{{r|Beichman2013}}}}
|parallax=70
|p_error=14
|parallax_footnote={{r|Dupuy2013}}
}}{{Starbox detail
|mass_mj={{nowrap|3–6 or 0.5–20{{r|Beichman2013}}}}
|temperature=250–400{{r|Beichman2013}}
|age_gyr={{nowrap|2–4 or 0.1–10{{r|Beichman2013}}}}
}}{{Starbox catalog
| names=WISEPA J182831.08+265037.8{{r|Kirkpatrick2011}}
WISEP J182831.08+265037.8{{r|Beichman2013}}
WISEP J1828+2650{{r|Cushing2011}}
WISE J1828+2650{{r|Kirkpatrick2011}}
WISE 1828+2650{{r|Kirkpatrick2011}}}}{{Starbox reference
|Simbad=NAME+WISEP+J1828%2B2650
}}{{Starbox end}}

WISE 1828+2650 (full designation WISEPA J182831.08+265037.8) is a brown dwarf or rogue planet{{r|Beichman2013}} of spectral class >Y2,{{r|Beichman2013}} located in constellation Lyra at approximately 47 light-years from Earth.{{r|Dupuy2013}} It is the "archetypal member" of the Y spectral class.{{r|Cushing2011}}

History of observations

Discovery

WISE 1828+2650 was discovered in 2011 from data collected by NASA's 40 cm (16 in) Wide-field Infrared Survey Explorer (WISE) space telescope at infrared wavelength. WISE 1828+2650 has two discovery papers: Kirkpatrick et al. (2011) and Cushing et al. (2011), however, basically with the same authors and published nearly simultaneously.{{r|Kirkpatrick2011|Cushing2011}}

  • Kirkpatrick et al. presented discovery of 98 new found by WISE brown dwarf systems with components of spectral types M, L, T and Y, among which also was WISE 1828+2650 — coolest of them.{{r|Kirkpatrick2011}}[1]
  • Cushing et al. presented discovery of seven brown dwarfs — one of T9.5 type, and six of Y-type — first members of the Y spectral class, ever discovered and spectroscopically confirmed, including "archetypal member" of the Y spectral class — WISE 1828+2650.{{r|Cushing2011}} These seven objects are also the faintest seven of 98 brown dwarfs, presented in Kirkpatrick et al. (2011).{{r|Kirkpatrick2011}}

Distance

Currently the most accurate distance estimate of WISE 1828+2650 is a trigonometric parallax, measured using Spitzer Space Telescope and published in 2013 by Trent Dupuy and Adam Kraus: 0.070 ± 0.014 arcsec, corresponding to a distance 14.3{{±|3.6|2.4}} pc, or 46.6{{±|11.6|7.8}} ly.{{r|Dupuy2013}}

 WISE 1828+2650 distance estimates
Source Parallax
(mas) 		Distance
(pc) 		Distance
(ly) 		Ref
Kirkpatrick et al. (2011)
 {{small|(Table 6)}}		 – <9.4 <30.7 Kirkpatrick2011}}
Beichman et al. (2013)
 {{small|(according to Kirkpatrick et al. (2012))}}		 122 ± 13 1.0|0.8}}3.2|2.6}}Kirkpatrick2012}}
Beichman et al. (2013) 90 ± 9.5[2] 1.3|1.0}}4.2|3.3}}Beichman2013}}
Dupuy & Kraus (2013) 70 ± 14[3] 14.3{{±>3.6|2.4}}46.6{{±>11.6|7.8}}Dupuy2013}}
Non-trigonometric distance estimates are marked in italic. The most precise estimate is marked in bold.

Proper motion

WISE 1828+2650 has proper motion of about 966 milliarcseconds per year.{{r|Beichman2013}}

 WISE 1828+2650 proper motion estimates
Source μ
mas/yr 		P. A.
° 		μRA
mas/yr 		μDEC
mas/yr 		Ref
Kirkpatrick et al. (2011) 1084 84 1078 ± 327 118 ± 409 Kirkpatrick2011}}
Beichman et al. (2013) 966 81 954 ± 11 153 ± 12.5 Beichman2013}}
Dupuy & Kraus (2013) 1034 ± 15 80.4 ± 0.9 1020 ± 15 173 ± 16 Dupuy2013}}
The best estimate is marked in bold.

Physical properties

Until the discovery of WISE 0855−0714 in 2014 WISE 1828+2650 was considered as the coldest currently known brown dwarf or the first example of free-floating planet (it is not currently known if it is a brown dwarf or a free-floating planet).{{r|Beichman2013}} It has a temperature in the range {{Convert|250|–|400|K|C F}}{{r|Beichman2013}} and was initially estimated below 300 K,{{r|Cushing2011}} or about {{convert|27|C|F|abbr=on}}. It has been assigned the latest known spectral class (>Y2,{{r|Beichman2013}} initially estimated as >Y0{{r|Cushing2011}}).

The mass of WISE 1828+2650 is in the range {{Jupiter mass|Jup=y|link=y|0.5–20}} for ages of 0.1–10 Gyr.{{r|Beichman2013}}

High tangential velocity of WISE 1828+2650, characteristic of an old disk population, indicates possible age of WISE 1828+2650 in the range 2–4 Gyr, leading to mass estimate of about {{Jupiter mass|Jup=y|link=y|3–6}}.{{r|Beichman2013}}[4]

WISE 1828+2650 is similar in appearance to the other Y-type object WD 0806-661 B. WD 0806-661 B could have formed as a planet close to its primary, WD 0806-661 A, and later, when the primary became a white dwarf and lost most of its mass, have migrated into a larger orbit of 2500 AU, and similarity between WD 0806-661 B and WISE 1828+2650 may indicate that WISE 1828+2650 had formed in the same way.{{r|Beichman2013}}

Possible binarity

Comparison between WISE 1828+2650 and WD 0806-661 B may suggest that WISE 1828+2650 is a system of two equal-mass objects. Observations with Hubble Space Telescope (HST) and Keck-II LGS-AO system had not revealed binarity, suggesting that if any such companion exists, it would have an orbit less than 0.5 AU, and no evidence for binarity yet exists.{{r|Beichman2013}}

Comparison

{{clear}}

See also

The other six discoveries of brown dwarfs, published by Cushing et al. in 2011:{{r|Cushing2011}}

  • WISE 0148−7202 (T9.5)
  • WISE 0410+1502 (Y0)
  • WISE 1405+5534 (Y0 (pec?))
  • WISE 1541−2250 (Y0.5)
  • WISE 1738+2732 (Y0)
  • WISE 2056+1459 (Y0)

Notes

1. ^These 98 brown dwarf systems are only among first, not all brown dwarf systems, discovered from data, collected by WISE: six discoveries were published earlier (however, also listed in Kirkpatrick et al. (2011)) in Mainzer et al. (2011) and Burgasser et al. (2011), and the other discoveries were published later.
2. ^According to Dupuy & Kraus (2013), this measurement uncertainty is likely underestimated.
3. ^Relative parallax.
4. ^This may indicate that WISE 1828+2650 is more likely a free-floating planet, not a brown dwarf, since it is below the lower mass limit for brown dwarfs ({{Jupiter mass|Jup=y|~13}}, see brown dwarf).
5. ^{{cite journal |last=Cushing |first=Michael C. |title=The Discovery of Y Dwarfs using Data from the Wide-field Infrared Survey Explorer (WISE) |year=2011 |doi=10.1088/0004-637X/743/1/50 |bibcode=2011ApJ...743...50C|journal=The Astrophysical Journal |volume= 743 |pages=50 |number =1 |last2=Kirkpatrick |first2=J. Davy |last3=Gelino |first3=Christopher R. |last4=Griffith |first4=Roger L. |last5=Skrutskie |first5=Michael F. |last6=Mainzer |first6=A. |last7=Marsh |first7=Kenneth A. |last8=Beichman |first8=Charles A. |last9=Burgasser |first9=Adam J. |last10=Prato |first10=Lisa A. |last11=Simcoe |first11=Robert A. |last12=Marley |first12=Mark S. |last13=Saumon |first13=D. |last14=Freedman |first14=Richard S. |last15=Eisenhardt |first15=Peter R. |last16=Wright |first16=Edward L. |arxiv = 1108.4678 }}
6. ^{{cite journal | authorlink=J. Davy Kirkpatrick | last=Kirkpatrick |first=J. Davy |author2=Cushing, Michael C. |author3=Gelino, Christopher R. |author4=Griffith, Roger L. |author5=Skrutskie, Michael F. |author6=Marsh, Kenneth A. |author7=Wright, Edward L. |author8=Mainzer, A. |author9=Eisenhardt, Peter R. |author10=McLean, Ian S. |author11=Thompson, Maggie A. |author12=Bauer, James M. |author13=Benford, Dominic J. |author14=Bridge, Carrie R. |author15=Lake, Sean E. |author16=Petty, Sara M. |author17=Stanford, S. A. |author18=Tsai, Chao-Wei |author19=Bailey, Vanessa |author20=Beichman, Charles A. |author21=Bloom, Joshua S. |author22=Bochanski, John J. |author23=Burgasser, Adam J. |author24=Capak, Peter L. |author25=Cruz, Kelle L. |author26=Hinz, Philip M. |author27=Kartaltepe, Jeyhan S. |author28=Knox, Russell P. |author29=Manohar, Swarnima |author30=Masters, Daniel |author31=Morales-Calderon, Maria |author32=Prato, Lisa A. |author33=Rodigas, Timothy J. |author34=Salvato, Mara |author35=Schurr, Steven D. |author36=Scoville, Nicholas Z. |author37=Simcoe, Robert A. |author38=Stapelfeldt, Karl R. |author39=Stern, Daniel |author40=Stock, Nathan D. |author41=Vacca, William D. | title=The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE) | date=2011 | journal=The Astrophysical Journal Supplement | volume=197 | issue=2 | pages=19 | arxiv=1108.4677v1 | doi=10.1088/0067-0049/197/2/19 | bibcode=2011ApJS..197...19K}}
7. ^{{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}}
8. ^{{cite journal | last=Beichman |first=C. |author2=Gelino, Christopher R. |author3=Kirkpatrick, J. Davy |author4=Barman, Travis S. |author5=Marsh, Kenneth A. |author6=Cushing, Michael C. |author7=Wright, E. L. | title=The Coldest Brown Dwarf (or Free-floating Planet)?: The Y Dwarf WISE 1828+2650 | date=2013 | journal=The Astrophysical Journal | volume=764 | issue=1 | pages=101 | arxiv=1301.1669 | doi=10.1088/0004-637X/764/1/101 | bibcode=2013ApJ...764..101B}}
9. ^{{Cite journal | doi = 10.1126/science.1241917| title = Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects| journal = Science| volume = 341| issue = 6153| pages = 1492–5| year = 2013| last1 = Dupuy | first1 = T. J.| last2 = Kraus | first2 = A. L.|arxiv = 1309.1422 |bibcode = 2013Sci...341.1492D | pmid=24009359}}

References

{{reflist|colwidth=30em|refs=[5][6][7][8][9]
}}

External links

  • {{cite news|last=Choi|first=Charles Q.|title=Y dwarf star? Because they're cool, that's Y!|publisher=Space.com|date=August 26, 2011|url=http://www.space.com/12714-coldest-failed-stars-brown-dwarfs-wise.html|accessdate=August 31, 2011}}
  • NASA news release
  • [https://science.nasa.gov/science-news/science-at-nasa/2011/23aug_coldeststars/ Science news]
  • {{APOD |date=30 August 2011 |title=Infrared image of WISE 1828+2650}}
  • Solstation.com (New Objects within 20 light-years)
{{Stars of Lyra}}

6 : Brown dwarfs|Rogue planets|Y-type stars|Lyra (constellation)|Astronomical objects discovered in 2011|WISE objects
随便看

　

开放百科全书收录14589846条英语、德语、日语等多语种百科知识，基本涵盖了大多数领域的百科知识，是一部内容自由、开放的电子版国际百科全书。

　

Copyright © 2023 OENC.NET All Rights Reserved
京ICP备2021023879号 更新时间：2024/11/13 12:47:11