WASP-36

(تم التحويل من WASP-36b)
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 الطيفيG2V[4]
B-V دليل الألوان0.4[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
المسافةس ض
( ف ن)
التـفـاصـيل[5]
الكتلة1.03+0.033−0.036 M
نصف القطر0.966+0.013−0.014 R
الضياء1.202+0.089−0.081 L
جاذبية السطح (ج)4.4807+0.0086−0.0085 س.ج.ث.
درجة الحرارة6150+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
العمر1.01+1.1−0.68 م.س.
تسميات أخرى
TOI-567، TIC 13349647، WASP-36، 2MASS J08461929-0801370، DENIS J084619.3-080136[3]
مراجع قواعد البيانات
SIMBADdata

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]


نظام WASP-36 [5]
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

  1. ^ قالب:Cite constellation
  2. ^ أ ب ت ث قالب:Cite Gaia DR3
  3. ^ أ ب "WASP-36". SIMBAD. Centre de données astronomiques de Strasbourg.
  4. ^ 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.
  5. ^ 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:10.3847/1538-4365/ac0835, Bibcode2021ApJS..255...15W 
  6. ^ 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.
  7. ^ "Wasp-36b". NASA Exoplanet Exploration. NASA. 2 October 2017. Retrieved 21 May 2020.
  8. ^ 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.
  9. ^ 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.
  10. ^ 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.
  11. ^ WASP-36 b Solar analogue 1.5 day orbital period 2.4 Jupiter masses 1.4 Jupiter radii
  12. ^ 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.
  13. ^ 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:10.3847/1538-3881/ababad, Bibcode2020AJ....160..155W 

قراءات إضافية

قالب:Stars of Hydra