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Coordinates: Sky map 05h 48m 33.5938s, −63° 59′ 18.3868″
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{{Short description|Star in the constellation Dorado}}
{{Short description|Star in the constellation Dorado}}

{{Starbox begin
{{Starbox begin
| name = [[Wide Angle Search for Planets|WASP]]-62
| name = WASP-62 / Naledi
}}
}}
{{Starbox observe
{{Starbox observe
| epoch = J2000.0
| epoch = J2000.0
| constell = [[Dorado (constellation)|Dorado]]
| constell = [[Dorado (constellation)|Dorado]]
| ra = {{RA|05|48|33.5938}}<ref name=simbad/>
| ra = {{RA|05|48|33.59333}}<ref name=GaiaDR3/>
| dec = {{DEC|-63|59|18.3868}}<ref name=simbad/>
| dec = {{DEC|-63|59|18.3884}}<ref name=GaiaDR3/>
| appmag_v = 10.21
| appmag_v = 10.21<ref name=simbad/>
}}
}}
{{Starbox character
{{Starbox character
Line 15: Line 14:
| class = F
| class = F
| appmag_1_passband = B
| appmag_1_passband = B
| appmag_1 = 10.73 <ref name=simbad/>
| appmag_1 = 10.73<ref name=simbad/>
| appmag_2_passband = G
| appmag_2_passband = G
| appmag_2 = 10.0721 <ref name=simbad/>
| appmag_2 = {{val|10.077|0.003}}<ref name=GaiaDR3/>
| appmag_3_passband = R
| appmag_3_passband = R
| appmag_3 = 9.93 <ref name=simbad/>
| appmag_3 = 9.93<ref name=simbad/>
| variable =
| variable =
}}
}}
{{Starbox astrometry
{{Starbox astrometry
| radial_v = 15.47
| radial_v = {{val|15.24|0.25}}<ref name=GaiaDR3/>
| prop_mo_ra = -15.641<ref name=dr2/>
| prop_mo_ra = -15.439
| prop_mo_dec = 26.046<ref name=dr2/>
| prop_mo_dec = 26.151
| pm_footnote = <ref name=GaiaDR3/>
| parallax = 5.6649
| p_error = 0.0189
| parallax = 5.6910
| p_error = 0.0113
⚫
| parallax_footnote = <ref name=dr2>{{cite DR2|4756649415309914240}}</ref>
| parallax_footnote = <ref name=GaiaDR3/>
| absmag_v =
| absmag_v =
}}
}}
{{Starbox detail
{{Starbox detail
| source = <ref name="Bonomo2017"/>
⚫
| source =<ref name=Kilpatrick2016>{{citation|arxiv=1611.08708|title=Spitzer secondary eclipse depths with multiple intrapixel sensitivity correction methods observations of WASP-13b, WASP-15b, WASP-16b, WASP-62b, and HAT-P-22b|year=2016|doi=10.3847/1538-3881/153/1/22|last1=Kilpatrick|first1=Brian M.|last2=Lewis|first2=Nikole K.|last3=Kataria|first3=Tiffany|last4=Deming|first4=Drake|last5=Ingalls|first5=James G.|last6=Krick|first6=Jessica E.|last7=Tucker|first7=Gregory S.|journal=The Astronomical Journal|volume=153|page=22|s2cid=12168984}}</ref>
| mass = 1.250{{±|0.05}}
| mass = {{val|1.250|0.050}}
| radius = 1.280{{±|0.05}}
| radius = {{val|1.280|0.050}}
| luminosity =
| luminosity =
| gravity = 4.45{{±|0.1}}
| gravity = 4.45{{±|0.1}}
| temperature = 6230{{±|80}}
| temperature = {{val|6230|80}}
| metal_fe = 0.04{{±|0.06}}
| metal_fe = {{val|0.040|0.060}}
| rotation =
| rotation =
| rotational_velocity = 8.7{{±|0.4}}
| rotational_velocity = {{val|8.70|0.40}}
| age_gyr = 0.8{{±|0.6}}<ref name=Brown2016/>
| age_gyr = {{val|2.60|0.50|0.70}}
}}
}}
{{Starbox catalog
{{Starbox catalog
| names = Naledi, {{odlist |2MASS=J05483359-6359183|GSC=08900-00874|Gaia DR2=4756649415309914240|TYC=8900-874-1|CPD=-64 484|TOI=102}}<ref name=simbad/>
| names = {{odlist | name=Naledi | 2MASS=J05483359-6359183 | CPD=-64 484 | GSC=08900-00874 | TIC=149603524 | TOI=102 |TYC=8900-874-1 | WASP=62}}<ref name=simbad/>
}}
}}
{{Starbox reference
{{Starbox reference
| Simbad = CPD-64 484
| Simbad = CPD-64+484
}}
}}
{{Starbox end
{{Starbox end}}

}}
'''WASP-62''' is a single star about 575 light-years away. It is an F class [[main-sequence star]], orbited by a planet, WASP-62b. The age of WASP-62 is much younger than the Sun at 0.8{{±|0.6}} billion years,<ref name=Brown2016/> and it has a metal abundance similar to the Sun. WASP-62 was named '''Naledi''' in 2019.<ref name="Methodology"/>
'''WASP-62''', formally named '''Naledi''', is a single star about {{convert|573|ly|pc|lk=on|abbr=off}} away. It is an F class [[main-sequence star]], orbited by a planet, WASP-62b. The age of WASP-62 is much younger than the Sun at 0.8{{±|0.6}} billion years,<ref name=Brown2016/> and it has a metal abundance similar to the Sun.

==Nomenclature==
The designation ''WASP-62'' indicates that this was the 62nd star found to have a planet by the [[Wide Angle Search for Planets]].

⚫
In December 2019, WASP-62 was named Naledi and its planet was named [[Krotoa]] by amateur astronomers from [[South Africa]] as part of the second [[NameExoWorlds]] campaign.<ref name="NEW2019"/><ref name="Methodology"/>


==Planetary system==
==Planetary system==
A [[Astronomical transit|transiting]] [[hot Jupiter]] [[exoplanet]] orbiting WASP-62 was discovered by [[Wide Angle Search for Planets|WASP]] in 2012.<ref name=Hellier2012>{{citation|arxiv=1204.5095|title=Seven transiting hot-Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b & WASP-67b|year=2012|doi=10.1111/j.1365-2966.2012.21780.x|last1=Hellier|first1=Coel|last2=Anderson|first2=D. R.|last3=Collier Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Fumel|first5=A.|last6=Gillon|first6=M.|last7=Jehin|first7=E.|last8=Lendl|first8=M.|last9=Maxted|first9=P. F. L.|last10=Pepe|first10=F.|last11=Pollacco|first11=D.|last12=Queloz|first12=D.|last13=Ségransan|first13=D.|last14=Smalley|first14=B.|last15=Smith|first15=A. M. S.|last16=Southworth|first16=J.|last17=Triaud|first17=A. H. M. J.|last18=Udry|first18=S.|last19=West|first19=R. G.|journal=Monthly Notices of the Royal Astronomical Society|volume=426|issue=1 |pages=739–750|bibcode=2012MNRAS.426..739H |s2cid=54713354}}</ref> The planet's equilibrium temperature is 1440{{±|30}} [[Kelvin|K]], but the measured average temperature is colder at 1329.6{{±|44.8}} K.<ref name=Kilpatrick2016/> In 2020, a transmission spectrum indicated the atmosphere of WASP-62b is free of clouds. It contains sodium and possibly silicon hydrides.<ref>{{citation|arxiv=2011.06424|title=Evidence of a Clear Atmosphere for WASP-62b: The Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone|year=2021|last1=Alam|first1=Munazza K.|last2=Lopez-Morales|first2=Mercedes|last3=MacDonald|first3=Ryan J.|last4=Nikolov|first4=Nikolay|last5=Kirk|first5=James|last6=Goyal|first6=Jayesh M.|last7=Sing|first7=David K.|last8=Wakeford|first8=Hannah R.|last9=Rathcke|first9=Alexander D.|last10=Deming|first10=Drake L.|last11=Sanz-Forcada|first11=Jorge|last12=Lewis|first12=Nikole K.|last13=Barstow|first13=Joanna K.|last14=Mikal-Evans|first14=Thomas|last15=Buchhave|first15=Lars A.|journal=The Astrophysical Journal|volume=906|issue=2|pages=L10|doi=10.3847/2041-8213/abd18e|s2cid=226306572}}</ref>
A [[Astronomical transit|transiting]] [[hot Jupiter]] [[exoplanet]] orbiting WASP-62 was discovered by [[Wide Angle Search for Planets|WASP]] in 2012.<ref name=Hellier2012/> The planet's equilibrium temperature is 1440{{±|30}} [[Kelvin|K]], but the measured average temperature is colder at 1329.6{{±|44.8}} K.<ref name=Kilpatrick2016/> In 2020, a transmission spectrum indicated the atmosphere of WASP-62b is free of clouds. It contains sodium and possibly silicon hydrides.<ref>{{citation|arxiv=2011.06424|title=Evidence of a Clear Atmosphere for WASP-62b: The Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone|year=2021|last1=Alam|first1=Munazza K.|last2=Lopez-Morales|first2=Mercedes|last3=MacDonald|first3=Ryan J.|last4=Nikolov|first4=Nikolay|last5=Kirk|first5=James|last6=Goyal|first6=Jayesh M.|last7=Sing|first7=David K.|last8=Wakeford|first8=Hannah R.|last9=Rathcke|first9=Alexander D.|last10=Deming|first10=Drake L.|last11=Sanz-Forcada|first11=Jorge|last12=Lewis|first12=Nikole K.|last13=Barstow|first13=Joanna K.|last14=Mikal-Evans|first14=Thomas|last15=Buchhave|first15=Lars A.|journal=The Astrophysical Journal|volume=906|issue=2|pages=L10|doi=10.3847/2041-8213/abd18e|bibcode=2021ApJ...906L..10A |s2cid=226306572 |doi-access=free }}</ref>


The planetary orbit is slightly misaligned to the equatorial plane of the star, with the misalignment angle equal to 19.4{{±|5.1|4.9}}°.<ref name=Brown2016/>
⚫
The planetary orbit is slightly misaligned to the equatorial plane of the star, with the misalignment angle equal to 19.4{{±|5.1|4.9}}°.<ref name=Brown2016>{{citation|arxiv=1610.00600|title=Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems|year=2016|doi=10.1093/mnras/stw2316|last1=Brown|first1=D. J. A.|last2=Triaud|first2=A. H. M. J.|last3=Doyle|first3=A. P.|last4=Gillon|first4=M.|last5=Lendl|first5=M.|last6=Anderson|first6=D. R.|last7=Collier Cameron|first7=A.|last8=Hébrard|first8=G.|last9=Hellier|first9=C.|last10=Lovis|first10=C.|last11=Maxted|first11=P. F. L.|last12=Pepe|first12=F.|last13=Pollacco|first13=D.|last14=Queloz|first14=D.|last15=Smalley|first15=B.|journal=Monthly Notices of the Royal Astronomical Society|volume=464|pages=810–839|s2cid=53497449}}</ref>


⚫
'''WASP-62b''' was named "Krotoa" in 2019 by amateur astronomers from [[South Africa]] as part of the [[NameExoWorlds]] contest.<ref name="Methodology">{{Cite web
⚫
|url=https://africanews.space/international-astronautical-union-approves-names-for-new-stars-and-exoplanets/
⚫
|title=International Astronomical Union Approves Names For New Stars And Exoplanets
⚫
|access-date=2020-11-12 |website=Space in Africa|date=18 December 2019
⚫
|language=en}}</ref>
{{OrbitboxPlanet begin
{{OrbitboxPlanet begin
| name = WASP-62
| name = WASP-62
| table_ref =<ref name=Kilpatrick2016/>
| table_ref = <ref name=Kilpatrick2016/>
}}
}}
{{OrbitboxPlanet
{{OrbitboxPlanet
| exoplanet = [[WASP-62b|b]]
| exoplanet = b / Krotoa
| mass = 0.562{{±|0.042}}
| mass = {{val|0.562|0.042}}
| semimajor = 0.0567{{±|0.0007}}<ref name=Hellier2012/>
| semimajor = {{val|0.05672|0.00075|0.00079}}<ref name="Bonomo2017"/>
| period = 4.4119530{{±|0.000003}}
| period = {{val|4.4119530|(30)}}
| eccentricity = <0.21<ref name=Hellier2012/>
| eccentricity = <0.075<ref name="Bonomo2017"/>
| inclination = 88.3{{±|0.9|0.6}}
| inclination = {{val|88.30|0.90|0.60}}
| radius = 1.390{{±|0.060}}
| radius = {{val|1.390|0.060}}
}}
}}
{{Orbitbox end}}
{{Orbitbox end}}
Line 80: Line 80:
==References==
==References==
{{Reflist|refs=
{{Reflist|refs=

<ref name=simbad>{{cite simbad |title=CPD-64 484}}</ref>
<ref name=simbad>{{cite simbad |title=CPD-64 484 |access-date=2 November 2023}}</ref>

⚫
<ref name=GaiaDR3>{{Cite Gaia DR3|4756649415309914240}}</ref>

<ref name=Hellier2012>{{citation|arxiv=1204.5095|title=Seven transiting hot-Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b & WASP-67b|year=2012|doi=10.1111/j.1365-2966.2012.21780.x|last1=Hellier|first1=Coel|last2=Anderson|first2=D. R.|last3=Collier Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Fumel|first5=A.|last6=Gillon|first6=M.|last7=Jehin|first7=E.|last8=Lendl|first8=M.|last9=Maxted|first9=P. F. L.|last10=Pepe|first10=F.|last11=Pollacco|first11=D.|last12=Queloz|first12=D.|last13=Ségransan|first13=D.|last14=Smalley|first14=B.|last15=Smith|first15=A. M. S.|last16=Southworth|first16=J.|last17=Triaud|first17=A. H. M. J.|last18=Udry|first18=S.|last19=West|first19=R. G.|journal=Monthly Notices of the Royal Astronomical Society|volume=426|issue=1 |pages=739–750|doi-access=free |bibcode=2012MNRAS.426..739H |s2cid=54713354}}</ref>

⚫
<ref name=Brown2016>{{citation|arxiv=1610.00600|title=Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems|year=2016|doi=10.1093/mnras/stw2316|last1=Brown|first1=D. J. A.|last2=Triaud|first2=A. H. M. J.|last3=Doyle|first3=A. P.|last4=Gillon|first4=M.|last5=Lendl|first5=M.|last6=Anderson|first6=D. R.|last7=Collier Cameron|first7=A.|last8=Hébrard|first8=G.|last9=Hellier|first9=C.|last10=Lovis|first10=C.|last11=Maxted|first11=P. F. L.|last12=Pepe|first12=F.|last13=Pollacco|first13=D.|last14=Queloz|first14=D.|last15=Smalley|first15=B.|journal=Monthly Notices of the Royal Astronomical Society|volume=464|issue=1 |pages=810–839|doi-access=free |s2cid=53497449 |bibcode=2017MNRAS.464..810B}}</ref>

⚫
<ref name=Kilpatrick2016>{{citation|arxiv=1611.08708|title=Spitzer secondary eclipse depths with multiple intrapixel sensitivity correction methods observations of WASP-13b, WASP-15b, WASP-16b, WASP-62b, and HAT-P-22b|year=2016|doi=10.3847/1538-3881/153/1/22|last1=Kilpatrick|first1=Brian M.|last2=Lewis|first2=Nikole K.|last3=Kataria|first3=Tiffany|last4=Deming|first4=Drake|last5=Ingalls|first5=James G.|last6=Krick|first6=Jessica E.|last7=Tucker|first7=Gregory S.|journal=The Astronomical Journal|volume=153|issue=1 |page=22|s2cid=12168984 |bibcode=2017AJ....153...22K |doi-access=free }}</ref>

<ref name="Bonomo2017">{{cite journal |last1=Bonomo |first1=A. S. |last2=Desidera |first2=S. |display-authors=etal |date=June 2017 |title=The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets |journal=[[Astronomy & Astrophysics]] |volume=602 |issue= |pages=A107 |doi=10.1051/0004-6361/201629882 |arxiv=1704.00373 |bibcode=2017A&A...602A.107B|s2cid=118923163 }}</ref>

<ref name="NEW2019">{{cite web |url=https://www.nameexoworlds.iau.org/2019approved-names |title=2019 Approved Names |website=nameexoworlds.iau.org |publisher=[[International Astronomical Union|IAU]] |access-date=2 November 2023}}</ref>

<ref name="Methodology">{{Cite web
⚫
|url=https://africanews.space/international-astronautical-union-approves-names-for-new-stars-and-exoplanets/
⚫
|title=International Astronomical Union Approves Names For New Stars And Exoplanets
⚫
|access-date=2020-11-12 |website=Space in Africa|date=18 December 2019
⚫
|language=en}}</ref>


}}
}}
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{{Dorado}}
{{Dorado}}


⚫
[[Category:Dorado]]
[[Category:F-type main-sequence stars]]
[[Category:F-type main-sequence stars]]
[[Category:Planetary systems with one confirmed planet]]
[[Category:Planetary systems with one confirmed planet]]
[[Category:Planetary transit variables]]
[[Category:Planetary transit variables]]
⚫
[[Category:Dorado]]
[[Category:2MASS objects|J05483359-6359183]]
[[Category:2MASS objects|J05483359-6359183]]
[[Category:Durchmusterung objects]]
[[Category:Durchmusterung objects|PD-64 00484]]
[[Category:Stars with proper names]]
[[Category:TESS Objects of Interest|102]]
[[Category:TIC objects|149603524]]
[[Category:Wide Angle Search for Planets|62]]
[[Category:Stars with proper names|Naledi]]

Latest revision as of 10:18, 22 August 2024

WASP-62 / Naledi
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Dorado
Right ascension 05h 48m 33.59333s[1]
Declination −63° 59′ 18.3884″[1]
Apparent magnitude (V) 10.21[2]
Characteristics
Evolutionary stage main-sequence star
Spectral type F
Apparent magnitude (B) 10.73[2]
Apparent magnitude (G) 10.077±0.003[1]
Apparent magnitude (R) 9.93[2]
Astrometry
Radial velocity (Rv)15.24±0.25[1] km/s
Proper motion (μ) RA: -15.439 mas/yr[1]
Dec.: 26.151 mas/yr[1]
Parallax (π)5.6910 ± 0.0113 mas[1]
Distance573 ± 1 ly
(175.7 ± 0.3 pc)
Details[3]
Mass1.250±0.050 M☉
Radius1.280±0.050 R☉
Surface gravity (log g)4.45±0.1 cgs
Temperature6230±80 K
Metallicity [Fe/H]0.040±0.060 dex
Rotational velocity (v sin i)8.70±0.40 km/s
Age2.60+0.50
−0.70 Gyr
Other designations
Naledi, CPD−64 484, TOI-102, TIC 149603524, WASP-62, TYC 8900-874-1, GSC 08900-00874, 2MASS J05483359-6359183[2]
Database references
SIMBADdata

WASP-62, formally named Naledi, is a single star about 573 light-years (176 parsecs) away. It is an F class main-sequence star, orbited by a planet, WASP-62b. The age of WASP-62 is much younger than the Sun at 0.8±0.6 billion years,[4] and it has a metal abundance similar to the Sun.

Nomenclature

[edit]

The designation WASP-62 indicates that this was the 62nd star found to have a planet by the Wide Angle Search for Planets.

In December 2019, WASP-62 was named Naledi and its planet was named Krotoa by amateur astronomers from South Africa as part of the second NameExoWorlds campaign.[5][6]

Planetary system

[edit]

A transiting hot Jupiter exoplanet orbiting WASP-62 was discovered by WASP in 2012.[7] The planet's equilibrium temperature is 1440±30 K, but the measured average temperature is colder at 1329.6±44.8 K.[8] In 2020, a transmission spectrum indicated the atmosphere of WASP-62b is free of clouds. It contains sodium and possibly silicon hydrides.[9]

The planetary orbit is slightly misaligned to the equatorial plane of the star, with the misalignment angle equal to 19.4+5.1
−4.9°.[4]

The WASP-62 planetary system[8]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b / Krotoa 0.562±0.042 MJ 0.05672+0.00075
−0.00079[3] 		4.4119530(30) <0.075[3] 88.30+0.90
−0.60° 		1.390±0.060 RJ

References

[edit]
  1. ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ a b c d "CPD-64 484". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2 November 2023.
  3. ^ a b c Bonomo, A. S.; Desidera, S.; et al. (June 2017). "The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy & Astrophysics. 602: A107. arXiv:1704.00373. Bibcode:2017A&A...602A.107B. doi:10.1051/0004-6361/201629882. S2CID 118923163.
  4. ^ a b Brown, D. J. A.; Triaud, A. H. M. J.; Doyle, A. P.; Gillon, M.; Lendl, M.; Anderson, D. R.; Collier Cameron, A.; Hébrard, G.; Hellier, C.; Lovis, C.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Smalley, B. (2016), "Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems", Monthly Notices of the Royal Astronomical Society, 464 (1): 810–839, arXiv:1610.00600, Bibcode:2017MNRAS.464..810B, doi:10.1093/mnras/stw2316, S2CID 53497449
  5. ^ "2019 Approved Names". nameexoworlds.iau.org. IAU. Retrieved 2 November 2023.
  6. ^ "International Astronomical Union Approves Names For New Stars And Exoplanets". Space in Africa. 18 December 2019. Retrieved 2020-11-12.
  7. ^ Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2012), "Seven transiting hot-Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b & WASP-67b", Monthly Notices of the Royal Astronomical Society, 426 (1): 739–750, arXiv:1204.5095, Bibcode:2012MNRAS.426..739H, doi:10.1111/j.1365-2966.2012.21780.x, S2CID 54713354
  8. ^ a b Kilpatrick, Brian M.; Lewis, Nikole K.; Kataria, Tiffany; Deming, Drake; Ingalls, James G.; Krick, Jessica E.; Tucker, Gregory S. (2016), "Spitzer secondary eclipse depths with multiple intrapixel sensitivity correction methods observations of WASP-13b, WASP-15b, WASP-16b, WASP-62b, and HAT-P-22b", The Astronomical Journal, 153 (1): 22, arXiv:1611.08708, Bibcode:2017AJ....153...22K, doi:10.3847/1538-3881/153/1/22, S2CID 12168984
  9. ^ Alam, Munazza K.; Lopez-Morales, Mercedes; MacDonald, Ryan J.; Nikolov, Nikolay; Kirk, James; Goyal, Jayesh M.; Sing, David K.; Wakeford, Hannah R.; Rathcke, Alexander D.; Deming, Drake L.; Sanz-Forcada, Jorge; Lewis, Nikole K.; Barstow, Joanna K.; Mikal-Evans, Thomas; Buchhave, Lars A. (2021), "Evidence of a Clear Atmosphere for WASP-62b: The Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone", The Astrophysical Journal, 906 (2): L10, arXiv:2011.06424, Bibcode:2021ApJ...906L..10A, doi:10.3847/2041-8213/abd18e, S2CID 226306572
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