WISE 2220−3628

{{Short description|Brown dwarf in the constellation Grus}}

{{Sky|22|20|55.31|-|36|28|17.4|26.4}}

{{Starbox begin

|name=WISE J222055.31−362817.4}}

{{Starbox image

| image = 250px

| caption = WISE 2220-3628

| credit = NASA/ESA/CSA JWST MIRI

}}

{{Starbox observe

|epoch=J2000{{r|Kirkpatrick2012}}

|equinox=J2000{{r|Kirkpatrick2012}}

|constell=Grus

|ra={{RA|22|20|55.31}}{{r|Kirkpatrick2012}}

|dec={{DEC|-36|28|17.4}}{{r|Kirkpatrick2012}}}}

{{Starbox character

|class=Y0{{r|Kirkpatrick2012}}

|appmag_1_passband=J (MKO-NIR filter system)

|appmag_1=20.38 ± 0.17{{r|Kirkpatrick2012}}

|appmag_3_passband=H (MKO-NIR filter system)

|appmag_3=20.81 ± 0.30{{r|Kirkpatrick2012}}

}}

{{Starbox astrometry

| radial_v = {{val|-53.2|2.8}}{{r|Faherty2024}}

| total_v = {{val|55.33|2.82}}{{r|Faherty2024}}

|prop_mo_ra=288.92 ±0.15

|prop_mo_dec=−97.10 ±0.16

| pm_footnote=

|parallax=93.50

|p_error=1.02

|parallax_footnote=

}}

{{Starbox detail

| mass_mj = 6-35{{r|Faherty2024}}

| radius_rj = {{val|0.94|0.14}}{{r|Faherty2024}}

| gravity = {{val|4.7|0.5}}{{r|Faherty2024}}

| temperature = {{val|480|41}}{{r|Faherty2024}}

| age_gyr = {{val|4.5|4.0}}{{r|Faherty2024}}

}}

{{Starbox catalog

|names=WISE J222055.31−362817.4,{{r|Kirkpatrick2012}}
WISE 2220−3628{{r|Kirkpatrick2012}}}}

{{Starbox reference

|Simbad=WISE+J222055.31-362817.4

}}

{{Starbox end}}

WISE J222055.31−362817.4 (designation abbreviated to WISE 2220−3628) is a brown dwarf of spectral class Y0,{{r|Kirkpatrick2012}} located in constellation Grus at approximately 34.2 light-years from Earth.{{r|Kirkpatrick23}}

Discovery

WISE 2220−3628 was discovered in 2012 by J. Davy Kirkpatrick et al. from data, collected by Wide-field Infrared Survey Explorer (WISE) Earth-orbiting satelliteNASA infrared-wavelength 40 cm (16 in) space telescope, which mission lasted from December 2009 to February 2011. In 2012 Kirkpatrick et al. published a paper in The Astrophysical Journal, where they presented discovery of seven new found by WISE brown dwarfs of spectral type Y, among which also was WISE 2220−3628.{{r|Kirkpatrick2012}}

Properties

Y-class dwarfs are among the coldest of all brown dwarfs.{{r|Kirkpatrick2012}} WISE 2220-3628 was observed with JWST and found to be very similar to CWISEP J1935-1546, with the difference of having no signature of an aurora and no temperature inversion in its atmosphere.{{r|Faherty2024}}

Distance

The most accurate distance estimate of WISE 2220−3628 was a trigonometric parallax, published in 2014 by Beichman et al.: 0.136 ± 0.017 arcsec, corresponding to a distance of {{cvt|7.4|±|0.9|pc|ly|lk=on}}.{{r|Beichman2014}} Later the parallax measurement was improved revealing a larger distance of about 34 light years.{{r|Kirkpatrick23}}

==See also==

References

{{reflist|refs=

{{cite journal |author-link=J. Davy Kirkpatrick |last1=Kirkpatrick |first1=J. Davy |last2=Gelino |first2=Christopher R. |last3=Cushing |first3=Michael C. |last4=Mace | first4=Gregory N. |last5=Griffith |first5=Roger L. |last6=Skrutskie |first6=Michael F. |last7=Marsh |first7=Kenneth A. |last8=Wright |first8=Edward L. |last9=Eisenhardt |first9=Peter R. |last10=McLean |first10=Ian S. |last11=Mainzer | first11=Amy K. |last12=Burgasser |first12=Adam J. |last13=Tinney |first13=Chris G. |last14=Parker |first14=Stephen |last15=Salter |first15=Graeme |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 |s2cid=119279752 }}

{{cite journal|first1=C. |last1=Beichman|first2=Christopher R. |last2=Gelino|first3=J. Davy |last3=Kirkpatrick|first4=Michael C. |last4=Cushing|first5=Sally |last5=Dodson-Robinson|first6=Mark S. |last6=Marley|first7=Caroline V. |last7=Morley|first8=E. L. |last8=Wright|year=2014|title=WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection|journal=The Astrophysical Journal|volume=783 |issue=2 |page=68|arxiv=1401.1194v2|bibcode=2014ApJ...783...68B|doi=10.1088/0004-637X/783/2/68|s2cid=119302072 }}

{{Cite journal|display-authors=1 |last1= Kirkpatrick |first1= J. Davy |last2= Marocco |first2= Federico |last3= Gelino |first3= Christopher R. |last4= Raghu |first4= Yadukrishna |last5= Faherty |first5= Jacqueline K. |last6= Bardalez Gagliuffi |first6= Daniella C. |last7= Schurr |first7= Steven D. |last8= Apps |first8= Kevin |last9= Schneider |first9= Adam C. |last10= Meisner |first10= Aaron M. |last11= Kuchner |first11= Marc J. |last12= Caselden |first12= Dan |last13= Smart |first13= R. L. |last14= Casewell |first14= S. L. |last15= Raddi |first15= Roberto |last16= Kesseli |first16= Aurora |last17= Stevnbak Andersen |first17= Nikolaj |last18= Antonini |first18= Edoardo |last19= Beaulieu |first19= Paul |last20= Bickle |first20= Thomas P. |last21= Bilsing |first21= Martin |last22= Chieng |first22= Raymond |last23= Colin |first23= Guillaume |last24= Deen |first24= Sam |last25= Dereveanco |first25= Alexandru |last26= Doll |first26= Katharina |last27= Durantini Luca |first27= Hugo A. |last28= Frazer |first28= Anya |last29= Gantier |first29= Jean Marc |last30= Gramaize |first30=Léopold |last31= Grant |first31= Kristin |last32= Hamlet |first32= Leslie K. |last33= Higashimura |first33= Hiro |last34= Hyogo |first34= Michiharu |last35=Jałowiczor |first35= Peter A. |last36= Jonkeren |first36= Alexander |last37= Kabatnik |first37= Martin |last38= Kiwy |first38= Frank |last39= Martin |first39= David W. |last40= Michaels |first40= Marianne N. |last41= Pendrill |first41= William |last42= Pessanha Machado |first42= Celso |last43= Pumphrey |first43= Benjamin |last44= Rothermich |first44= Austin |last45= Russwurm |first45= Rebekah |last46= Sainio |first46= Arttu |last47= Sanchez |first47= John |last48= Sapelkin-Tambling |first48= Fyodor Theo |last49= Schümann |first49= Jörg |last50= Selg-Mann |first50= Karl |last51= Singh |first51= Harshdeep |last52= Stenner |first52= Andres |last53= Sun |first53= Guoyou |last54= Tanner |first54= Christopher |last55= Thévenot |first55= Melina |last56= Ventura |first56= Maurizio |last57= Voloshin |first57= Nikita V. |last58= Walla |first58= Jim |last59= Wedracki |first59= Zbigniew |last60= Adorno |first60= Jose I. |last61= Aganze |first61= Christian |last62= Allers |first62= Katelyn N. |last63= Brooks |first63= Hunter |last64= Burgasser |first64= Adam J. |last65= Calamari |first65= Emily |last66= Connor |first66= Thomas |last67= Costa |first67= Edgardo |last68= Eisenhardt |first68= Peter R. |last69= Gagné |first69= Jonathan |last70= Gerasimov |first70= Roman |last71= Gonzales |first71= Eileen C. |last72= Hsu |first72= Chih-Chun |last73= Kiman |first73= Rocio |last74= Li |first74= Guodong |last75= Low |first75= Ryan |last76= Mamajek |first76= Eric |last77= Pantoja |first77= Blake M. |last78= Popinchalk |first78= Mark |last79= Rees |first79= Jon M. |last80= Stern |first80= Daniel |last81= Suárez |first81= Genaro |last82= Theissen |first82= Christopher |last83= Tsai |first83= Chao-Wei |last84= Vos |first84= Johanna M. |last85= Zurek |first85= David |last86= The Backyard Worlds: Planet 9 Collaboration|date=December 2023 |title=The Initial Mass Function Based on the Full-sky 20-pc Census of ∼3,600 Stars and Brown Dwarfs |journal=The Astrophysical Journal Supplement Series |language=en |arxiv=2312.03639 |bibcode=2023arXiv231203639K}}

{{Cite journal |last1=Faherty |first1=Jacqueline K. |last2=Burningham |first2=Ben |last3=Gagné |first3=Jonathan |last4=Suárez |first4=Genaro |last5=Vos |first5=Johanna M. |last6=Alejandro Merchan |first6=Sherelyn |last7=Morley |first7=Caroline V. |last8=Rowland |first8=Melanie |last9=Lacy |first9=Brianna |last10=Kiman |first10=Rocio |last11=Caselden |first11=Dan |last12=Kirkpatrick |first12=J. Davy |last13=Meisner |first13=Aaron |last14=Schneider |first14=Adam C. |last15=Kuchner |first15=Marc Jason|first16=Daniella Carolina |last16=Bardalez Gagliuffi |first17=Charles |last17=Beichman |first18=Peter |last18=Eisenhardt |first19=Christopher R. |last19=Gelino |first20=Ehsan |last20=Gharib-Nezhad |first21=Eileen |last21=Gonzales |first22=Federico |last22=Marocco |first23=Austin James |last23=Rothermich |first24=Niall |last24=Whiteford |date=2024-04-17 |title=Methane emission from a cool brown dwarf |url=https://www.nature.com/articles/s41586-024-07190-w |journal=Nature |language=en |volume=628 |issue=8008 |pages=511–514 |doi=10.1038/s41586-024-07190-w |issn=1476-4687|arxiv=2404.10977 }}

{{Cite arXiv |eprint=2412.16679 |class=astro-ph |last1=Fontanive |first1=Clémence |title=The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- II. Parallaxes and Proper Motions |date=2024-12-21 |last2=Bedin |first2=Luigi R. |last3=Albert |first3=Loïc |last4=Gagliuffi |first4=Daniella C. Bardalez}}

}}

{{Stars of Grus}}

{{DEFAULTSORT:WISE 2220-3628}}

Category:Brown dwarfs

Category:Y-type brown dwarfs

Category:Grus (constellation)

Category:WISE objects