KELT-11b
In today's world, KELT-11b is a topic of interest that sparks various opinions and debates. Whether on a personal, social or professional level, KELT-11b has captured the attention of millions of people around the world. This phenomenon has generated a wide range of research, discussions and reflections that seek to understand and analyze the different aspects that make it up. From its origins to its possible future impacts, KELT-11b has been evolving and transforming over time, becoming a topic of constant interest for modern society. In this article, we will delve into the complexity of KELT-11b, exploring its many facets and analyzing the different positions that exist on the matter.
| Discovery | |
|---|---|
| Discovery date | July 6, 2016 |
| transit | |
| Orbital characteristics | |
| 0.06229 AU (9,318,000 km) | |
| 4.736529[1] d | |
| Star | HD 93396 |
| Physical characteristics | |
| 1.37+0.15 −0.12[1] RJ | |
| Mass | 0.195+0.019 −0.018[1] MJ |
Mean density | 0.093+0.028 −0.024 g/cm3[1] |
| 2.55 m/s2; 0.260 g0[1] | |
| Temperature | 1712+51 −46[1] |
KELT-11b is an exoplanet orbiting around the yellow subgiant star KELT-11 (HD 93396) about 320 light-years away from Earth. It is an inflated planet, one of the "puffiest planets" (lowest-density) known, as a result of its close orbiting distance with its parent star. It has a radius 1.37 times that of Jupiter, but only 19% of its mass. It was discovered in 2016.[1]
The transmission spectrum study in 2020 have revealed the KELT-11b atmosphere containing sub-solar amount of water vapor, but significant amounts of hydrogen cyanide, together with oxides of titanium and aluminum. Also, the nightside flux do indicate a generally cloud-free atmosphere with an effective heat redistribution between dayside and nightside.[2] Later studies have indicated the hydrogen cyanide spectral features are not well distinguished from spectral lines of carbon dioxide and carbon monoxide, although carbon dioxide seems to be present in larger amounts, indicating a high carbon/oxygen ratio of the planet.[3]
References
- ^ a b c d e f g Pepper, Joshua; Rodriguez, Joseph E.; Collins, Karen A.; Johnson, John Asher; Fulton, Benjamin J.; Howard, Andrew W.; Beatty, Thomas G.; Stassun, Keivan G.; Isaacson, Howard; Colón, Knicole D.; Lund, Michael B.; Kuhn, Rudolf B.; Siverd, Robert J.; Gaudi, B. Scott; Tan, T. G.; Curtis, Ivan; Stockdale, Christopher; Mawet, Dimitri; Bottom, Michael; James, David; Zhou, George; Bayliss, Daniel; Cargile, Phillip; Bieryla, Allyson; Penev, Kaloyan; Latham, David W.; Labadie-Bartz, Jonathan; Kielkopf, John; Eastman, Jason D.; et al. (2017). "KELT-11b: A Highly Inflated Sub-Saturn Exoplanet Transiting the V = 8 Subgiant HD 93396". The Astronomical Journal. 153 (5): 215. arXiv:1607.01755v1. Bibcode:2017AJ....153..215P. doi:10.3847/1538-3881/aa6572. S2CID 30219578.
- ^ Colón, Knicole D.; Kreidberg, Laura; Line, Michael; Welbanks, Luis; Madhusudhan, Nikku; Beatty, Thomas; Tamburo, Patrick; Stevenson, Kevin B.; Mandell, Avi; Rodriguez, Joseph E.; Barclay, Thomas; Lopez, Eric D.; Stassun, Keivan G.; Angerhausen, Daniel; Fortney, Jonathan J.; James, David J.; Pepper, Joshua; Ahlers, John P.; Plavchan, Peter; Awiphan, Supachai; Kotnik, Cliff; McLeod, Kim K.; Murawski, Gabriel; Chotani, Heena; LeBrun, Danny; Matzko, William; Rea, David; Vidaurri, Monica; Webster, Scott; et al. (2020). "An Unusual Transmission Spectrum for the Sub-Saturn KELT-11b Suggestive of a Subsolar Water Abundance". The Astronomical Journal. 160 (6): 280. arXiv:2005.05153. Bibcode:2020AJ....160..280C. doi:10.3847/1538-3881/abc1e9. S2CID 218581200.
- ^ Changeat, Q.; Edwards, B.; Al-Refaie, A. F.; Morvan, M.; Tsiaras, A.; Waldmann, I. P.; Tinetti, G. (2020), "KELT-11 b: Abundances of Water and Constraints on Carbon-bearing Molecules from the Hubble Transmission Spectrum", The Astronomical Journal, 160 (6): 260, arXiv:2010.01310, Bibcode:2020AJ....160..260C, doi:10.3847/1538-3881/abbe12, S2CID 222132941
