WASP-36
(Redirected from WASP-36b)
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hydra[1] |
| Right ascension | 08h 46m 19.2977s[2] |
| Declination | −08° 01′ 37.016″[2] |
| Apparent magnitude (V) | 12.7[3] |
| Characteristics | |
| Evolutionary stage | main sequence[4] |
| Spectral type | G2V[4] |
| B−V color index | 0.4[citation needed] |
| J−H color index | 0.256[citation needed] |
| J−K color index | 0.315[citation needed] |
| Astrometry | |
| Radial velocity (Rv) | −12.45±0.97[2] km/s |
| Proper motion (μ) | RA: -4.040 mas/yr[2] Dec.: -8.502 mas/yr[2] |
| Parallax (π) | 2.6493±0.0129 mas[2] |
| Distance | 1,231 ± 6 ly (377 ± 2 pc) |
| Details[5] | |
| Mass | 1.03+0.033 −0.036 M☉ |
| Radius | 0.966+0.013 −0.014 R☉ |
| Luminosity | 1.202+0.089 −0.081 L☉ |
| Surface gravity (log g) | 4.4807+0.0086 −0.0085 cgs |
| Temperature | 6150+110 −100 K |
| Metallicity [Fe/H] | -0.26±0.10[6] dex |
| Rotational velocity (v sin i) | 3.3±1.2[4] km/s |
| Age | 1.01+1.1 −0.68 Gyr |
| Other designations | |
| TOI-567, TIC 13349647, WASP-36, 2MASS J08461929-0801370, DENIS J084619.3-080136[3] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
WASP-36 is a G-type main-sequence star about 1,230 light-years away in the Hydra constellation.
Star characteristics
[edit]WASP-36 is a yellow main sequence star of spectral class G2, similar to the Sun.[7] It has a candidate stellar companion with apparent magnitude 14.03,[8][9] seemingly confirmed in 2019 using Gaia DR2 data.[10]
Planetary system
[edit]In 2010, the SuperWASP survey found the hot Jupiter class planet WASP-36b using the transit method.[11] Its temperature was measured to be 1705±44 K.[12] The planetary transmission spectrum taken in 2016 has turned out to be anomalous: the planet appears to be surrounded by a blue-tinted halo that is too wide to be an atmosphere and may represent a measurement error.[6]
The planetary dayside temperature measured in 2020 is 1440+150
−160 K.[13]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 2.281+0.070 −0.071 MJ |
0.02635+0.00028 −0.00031 |
1.53736533(14) | 0.0087+0.0097 −0.0061 |
83.42+0.12 −0.11° |
1.270+0.018 −0.019 RJ |
References
[edit]- ^ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
- ^ a b c d e 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.
- ^ a b "WASP-36". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c Smith, A. M. S.; Anderson, D. R.; Collier Cameron, A.; Gillon, M.; Hellier, C.; Lendl, M.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Barros, S. C. C.; Jehin, E.; Pepe, F.; Pollacco, D.; Segransan, D.; Southworth, J.; Street, R. A.; Udry, S. (2012). "WASP-36b: A NEW TRANSITING PLANET AROUND a METAL-POOR G-DWARF, AND AN INVESTIGATION INTO ANALYSES BASED ON a SINGLE TRANSIT LIGHT CURVE". The Astronomical Journal. 143 (4): 81. arXiv:1110.5313. Bibcode:2012AJ....143...81S. doi:10.1088/0004-6256/143/4/81. S2CID 67754202.
- ^ a b Wang, Xian-Yu; Wang, Yong-Hao; Wang, Songhu; Wu, Zhen-Yu; Rice, Malena; Zhou, Xu; Hinse, Tobias C.; Liu, Hui-Gen; Ma, Bo; Peng, Xiyan; Zhang, Hui; Yu, Cong; Zhou, Ji-Lin; Laughlin, Gregory (2021), "Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves", The Astrophysical Journal Supplement Series, 255 (1): 15, arXiv:2105.14851, Bibcode:2021ApJS..255...15W, doi:10.3847/1538-4365/ac0835, S2CID 235253975
- ^ a b Mancini, L.; Kemmer, J.; Southworth, J.; Bott, K.; Mollière, P.; Ciceri, S.; Chen, G.; Henning, Th. (2016). "An optical transmission spectrum of the giant planet WASP-36 b". Monthly Notices of the Royal Astronomical Society. 459 (2): 1393–1402. arXiv:1603.08031. Bibcode:2016MNRAS.459.1393M. doi:10.1093/mnras/stw659. S2CID 53411511.
- ^ "Wasp-36b". NASA Exoplanet Exploration. NASA. Retrieved 21 May 2020.
- ^ Ngo, Henry; Knutson, Heather A.; Hinkley, Sasha; Bryan, Marta; Crepp, Justin R.; Batygin, Konstantin; Crossfield, Ian; Hansen, Brad; Howard, Andrew W.; Johnson, John A.; Mawet, Dimitri; Morton, Timothy D.; Muirhead, Philip S.; Wang, Ji (2016). "FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION". The Astrophysical Journal. 827 (1): 8. arXiv:1606.07102. Bibcode:2016ApJ...827....8N. doi:10.3847/0004-637X/827/1/8. S2CID 41083068.
- ^ Evans, D. F.; Southworth, J.; Maxted, P. F. L.; Skottfelt, J.; Hundertmark, M.; Jørgensen, U. G.; Dominik, M.; Alsubai, K. A.; Andersen, M. I.; Bozza, V.; Bramich, D. M.; Burgdorf, M. J.; Ciceri, S.; d'Ago, G.; Figuera Jaimes, R.; Gu, S.-H.; Haugbølle, T.; Hinse, T. C.; Juncher, D.; Kains, N.; Kerins, E.; Korhonen, H.; Kuffmeier, M.; Mancini, L.; Peixinho, N.; Popovas, A.; Rabus, M.; Rahvar, S.; Schmidt, R. W.; et al. (2016). "High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP)". Astronomy & Astrophysics. 589: A58. arXiv:1603.03274. Bibcode:2016A&A...589A..58E. doi:10.1051/0004-6361/201527970. S2CID 14215845.
- ^ Mugrauer, M. (December 2019). "Search for stellar companions of exoplanet host stars by exploring the second ESA-Gaia data release". Monthly Notices of the Royal Astronomical Society. 490 (4): 5088–5102. Bibcode:2019MNRAS.490.5088M. doi:10.1093/mnras/stz2673.
- ^ WASP-36 b Solar analogue 1.5 day orbital period 2.4 Jupiter masses 1.4 Jupiter radii
- ^ Garhart, Emily; Deming, Drake; Mandell, Avi; Knutson, Heather A.; Wallack, Nicole; Burrows, Adam; Fortney, Jonathan J.; Hood, Callie; Seay, Christopher; Sing, David K.; Benneke, Björn; Fraine, Jonathan D.; Kataria, Tiffany; Lewis, Nikole; Madhusudhan, Nikku; McCullough, Peter; Stevenson, Kevin B.; Wakeford, Hannah (2020). "Statistical Characterization of Hot Jupiter Atmospheres Using Spitzer's Secondary Eclipses". The Astronomical Journal. 159 (4): 137. arXiv:1901.07040. Bibcode:2020AJ....159..137G. doi:10.3847/1538-3881/ab6cff. S2CID 119209434.
- ^ Wong, Ian; Shporer, Avi; Daylan, Tansu; Benneke, Björn; Fetherolf, Tara; Kane, Stephen R.; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Winn, Joshua N.; Jenkins, Jon M.; Boyd, Patricia T.; Glidden, Ana; Goeke, Robert F.; Sha, Lizhou; Ting, Eric B.; Yahalomi, Daniel (2020), "Systematic phase curve study of known transiting systems from year one of the TESS mission", The Astronomical Journal, 160 (4): 155, arXiv:2003.06407, Bibcode:2020AJ....160..155W, doi:10.3847/1538-3881/ababad, S2CID 212717799
Further reading
[edit]- Zhou, G.; Bayliss, D. D. R.; Kedziora-Chudczer, L.; Tinney, C. G.; Bailey, J.; Salter, G.; Rodriguez, J. (2015). "Secondary eclipse observations for seven hot-Jupiters from the Anglo-Australian Telescope". Monthly Notices of the Royal Astronomical Society. 454 (3): 3002–3019. arXiv:1509.04147. Bibcode:2015MNRAS.454.3002Z. doi:10.1093/mnras/stv2138. S2CID 84835437.
- Maciejewski, G.; Dimitrov, D.; Mancini, L.; Southworth, J.; Ciceri, S.; D'Ago, G.; Bruni, I.; Raetz, St.; Nowak, G.; Ohlert, J.; Puchalski, D.; Saral, G.; Derman, E.; Petrucci, R.; Jofre, E.; Seeliger, M.; Henning, T. (2016). "New transit observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b, and WASP-39 B". Acta Astronomica. 66 (1): 55. arXiv:1603.03268. Bibcode:2016AcA....66...55M.
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