WASP-36
بيانات الرصـد الحقبة J2000 اعتدال J2000 | |
---|---|
الكوكبة | Hydra[1] |
الصعود المستقيم | 08س 46د 19.2977ث[2] |
الميل | −08° 01′ 37.016″[2] |
القدر الظاهري (V) | 12.7[3] |
الخـصـائص | |
النوع الطيفي | G2V[4] |
B-V دليل الألوان | 0.4[بحاجة لمصدر] |
علم القياسات الفلكية | |
السرعة القطرية (Rv) | −12.45±0.97[2] كم/ث |
الحركة الحقيقية (μ) | RA: −4.040 mas/yr Dec.: −8.502 mas/س |
اختلاف المنظر (π) | 2.6493 ± 0.0129[2] mas |
المسافة | س ض ( ف ن) |
التـفـاصـيل[5] | |
الكتلة | 1.03+0.033−0.036 M☉ |
نصف القطر | 0.966+0.013−0.014 R☉ |
الضياء | 1.202+0.089−0.081 L☉ |
جاذبية السطح (ج) | 4.4807+0.0086−0.0085 س.ج.ث. |
درجة الحرارة | 6150+110−100 ك |
المعدنية [Fe/H] | −0.26+0.10−{{{2}}}[6] العشرية |
تسارع الدوران (v sin i) | 3.3+1.2−{{{2}}}[4] كم/ث |
العمر | 1.01+1.1−0.68 م.س. |
تسميات أخرى | |
مراجع قواعد البيانات | |
SIMBAD | data |
WASP-36 is a G-type main-sequence star about 1,230 light-years away in the Hydra constellation.
خصائص النجم
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]
النظام الكوكبي
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−{{{2}}} 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]
المرافق (بالترتيب من النجم) |
الكتلة | نصف المحور الرئيسي (و.ف.) |
الدور المداري (يوم) |
الانحراف | الميل | نصف القطر |
---|---|---|---|---|---|---|
b | 2.281+0.070 −0.071 MJ |
0.02635+0.00028 −0.00031 |
1.53736533(14) | 0.0087+0.0097 −0.0061 |
1.270+0.018 −0.019 RJ |
المصادر
- ^ قالب:Cite constellation
- ^ أ ب ت ث قالب:Cite Gaia DR3
- ^ أ ب "WASP-36". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ أ ب 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.
- ^ أ ب Wang, Xian-Yu; Wang, Yong-Hao; Wang, Songhu; Wu, Zhen-Yu; Rice, Malena; Zhou, Xu; Hinse, Tobias C.; Liu, Hui-Gen; et al. (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, doi: , Bibcode: 2021ApJS..255...15W
- ^ أ ب 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. 2 October 2017. 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; et al. (2020), "Systematic phase curve study of known transiting systems from year one of the TESS mission", The Astronomical Journal 160 (4): 155, doi: , Bibcode: 2020AJ....160..155W
قراءات إضافية
- 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.