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A p p e a r a n c e
F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
KELT-21b is an extrasolar planet discovered in 2017. It is a hot Jupiter with radius of about 1.586 M J .[1]
Host star [ edit ]
KELT-21b orbits KELT-21 A (HD 332124). It orbits the primary star in a triple star system , with the other two stars located 1.2 arcseconds away. These two stars, designated KELT-21 B and C, have masses of 0.13 M ☉ and 0.11 M ☉ , respectively.[1] The primary star is heavy at 1.458± 0.029M ☉ , extremely hot at 8210± 771 K and rapidly rotating (equatorial velocity equal to 141 km/s).[2] In comparison, the Sun has a temperature of 5772 K[3] and rotates at an equatorial velocity of 1.997 km/s.[4] The planetary orbit is well aligned with the equatorial plane of the host star, with misalignment equal to −5.6+1.7 −1.9 °.[5]
Transmission planetary spectroscopy was performed in 2021, based on a single transit observation in 2019. High planetary gravity and relatively low planetary temperature made detection of an atmosphere impossible that time.[6]
References [ edit ]
^ a b c d e f g h Johnson, Marshall C; Rodriguez, Joseph E; Zhou, George; Gonzales, Erica J; Cargile, Phillip A; Crepp, Justin R; Penev, Kaloyan; Stassun, Keivan G; Gaudi, B. Scott; Colón, Knicole D; Stevens, Daniel J; Strassmeier, Klaus G; Ilyin, Ilya; Collins, Karen A; Kielkopf, John F; Oberst, Thomas E; Maritch, Luke; Reed, Phillip A; Gregorio, Joao; Bozza, Valerio; Novati, Sebastiano Calchi; d'Ago, Giuseppe; Scarpetta, Gaetano; Zambelli, Roberto; Latham, David W; Bieryla, Allyson; Cochran, William D; Endl, Michael; Tayar, Jamie; et al. (2018). "KELT-21b: A Hot Jupiter Transiting the Rapidly Rotating Metal-poor Late-A Primary of a Likely Hierarchical Triple System" . The Astronomical Journal . 155 (2 ): 100. arXiv :1712.03241 . Bibcode :2018AJ....155..100J . doi :10.3847/1538-3881/aaa5af . S2CID 73559090 .
^ Garai, Z.; Pribulla, T.; Kovács, J.; Szabó, Gy M.; Claret, A.; Komžík, R.; Kundra, E. (2022), "Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era", Monthly Notices of the Royal Astronomical Society , 513 (2 ): 2822–2840, arXiv :2204.09077 , doi :10.1093/mnras/stac1095
^ Williams, D. R. (1 July 2013). "Sun Fact Sheet" . NASA Goddard Space Flight Center . Archived from the original on 15 July 2010. Retrieved 12 August 2013 .
^ "Solar System Exploration: Planets: Sun: Facts & Figures" . NASA. Archived from the original on 2 January 2008.
^ Rice, Malena; Wang, Songhu; Wang, Xian-Yu; Stefánsson, Guđmundur; Isaacson, Howard; Howard, Andrew W.; Logsdon, Sarah E.; Schweiker, Heidi; Dai, Fei; Brinkman, Casey; Giacalone, Steven; Holcomb, Rae (2022), "A Tendency Toward Alignment in Single-star Warm-Jupiter Systems", The Astronomical Journal , 164 (3 ): 104, arXiv :2207.06511 , Bibcode :2022AJ....164..104R , doi :10.3847/1538-3881/ac8153 , S2CID 250526491
^ Stangret, M.; Casasayas-Barris, N.; Pallé, E.; Orell-Miquel, J.; Morello, G.; Luque, R.; Nowak, G.; Yan, F. (2022), "High-resolution transmission spectroscopy study of ultra-hot Jupiters HAT-P-57b, KELT-17b, KELT-21b, KELT-7b, MASCARA-1b, and WASP-189b", Astronomy & Astrophysics , 662 : A101, arXiv :2111.13064 , Bibcode :2022A&A...662A.101S , doi :10.1051/0004-6361/202141799 , S2CID 244709777
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● T h i s p a g e w a s l a s t e d i t e d o n 3 0 J u n e 2 0 2 4 , a t 1 0 : 5 2 ( U T C ) .
● T e x t i s a v a i l a b l e u n d e r t h e C r e a t i v e C o m m o n s A t t r i b u t i o n - S h a r e A l i k e L i c e n s e 4 . 0 ;
a d d i t i o n a l t e r m s m a y a p p l y . B y u s i n g t h i s s i t e , y o u a g r e e t o t h e T e r m s o f U s e a n d P r i v a c y P o l i c y . W i k i p e d i a ® i s a r e g i s t e r e d t r a d e m a r k o f t h e W i k i m e d i a F o u n d a t i o n , I n c . , a n o n - p r o f i t o r g a n i z a t i o n .
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