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Juniper Jupiter

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Stevenson, D. J.; Bodenheimer, P.; Lissauer, J. J.; D'Angelo, G. (2022). "Mixing of Condensable Constituents with H-He during the Formation and Evolution of Jupiter". The Planetary Science Journal. 3 (4): id.74. arXiv: 2202.09476. Bibcode: 2022PSJ.....3...74S. doi: 10.3847/PSJ/ac5c44. S2CID 247011195. The axial tilt of Jupiter is relatively small, only 3.13°, so its seasons are insignificant compared to those of Earth and Mars. [132] Maunder, A. S. D. (August 1934). "The origin of the symbols of the planets". The Observatory. 57: 238–247. Bibcode: 1934Obs....57..238M. In Vedic astrology, Hindu astrologers named the planet after Brihaspati, the religious teacher of the gods, and often called it " Guru", which means the "Teacher". [236] [237] In Central Asian Turkic myths, Jupiter is called Erendiz or Erentüz, from eren (of uncertain meaning) and yultuz ("star"). The Turks calculated the period of the orbit of Jupiter as 11 years and 300 days. They believed that some social and natural events connected to Erentüz's movements on the sky. [238] The Chinese, Vietnamese, Koreans, and Japanese called it the "wood star" ( Chinese: 木星; pinyin: mùxīng), based on the Chinese Five Elements. [239] [240] [241] In China it became known as the "Year-star" (Sui-sing) as Chinese astronomers noted that it jumped one zodiac constellation each year (with corrections). In some ancient Chinese writings the years were named, at least in principle, in correlation with the Jovian zodiac signs. [242] Gallery Interplanetary Seasons". Science@NASA. Archived from the original on October 16, 2007 . Retrieved February 20, 2007.

MacDougal, Douglas W. (2012). "A Binary System Close to Home: How the Moon and Earth Orbit Each Other". Newton's Gravity. Undergraduate Lecture Notes in Physics. Springer New York. pp. 193–211. doi: 10.1007/978-1-4614-5444-1_10. ISBN 978-1-4614-5443-4. the barycentre is 743,000km from the centre of the Sun. The Sun's radius is 696,000km, so it is 47,000km above the surface. Encyclopedia - the brightest bodies". IMCCE. Archived from the original on July 24, 2023 . Retrieved May 29, 2023. Different from cedar: Junipers are not members of the Cedrus genus. The leaves of theseevergreenconifers usually take the form of flattened scales in the mature plants, though they may be needle-like in juvenile plants. a b c Pirani, S.; Johansen, A.; Bitsch, B.; Mustill, A.J.; Turrini, D. (March 2019). "Consequences of planetary migration on the minor bodies of the early solar system". Astronomy & Astrophysics. 623: A169. arXiv: 1902.04591. Bibcode: 2019A&A...623A.169P. doi: 10.1051/0004-6361/201833713. Bobis, Laurence; Lequeux, James (July 2008). "Cassini, Rømer, and the velocity of light". Journal of Astronomical History and Heritage. 11 (2): 97–105. Bibcode: 2008JAHH...11...97B. doi: 10.3724/SP.J.1440-2807.2008.02.02. S2CID 115455540.Murdin, Paul (2000). Encyclopedia of Astronomy and Astrophysics. Bristol: Institute of Physics Publishing. ISBN 978-0-12-226690-4. a b Kunde, V. G.; Flasar, F. M.; Jennings, D. E.; Bézard, B.; Strobel, D. F.; etal. (September 10, 2004). "Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment". Science. 305 (5690): 1582–1586. Bibcode: 2004Sci...305.1582K. doi: 10.1126/science.1100240. PMID 15319491. S2CID 45296656. Archived from the original on December 26, 2018 . Retrieved April 4, 2007. In 1932, Rupert Wildt identified absorption bands of ammonia and methane in the spectra of Jupiter. [160] Three long-lived anticyclonic features called "white ovals" were observed in 1938. For several decades they remained as separate features in the atmosphere, sometimes approaching each other but never merging. Finally, two of the ovals merged in 1998, then absorbed the third in 2000, becoming Oval BA. [161] Radiotelescope research Image of Jupiter and its radiation belts in radio

Brygoo, S.; Loubeyre, P.; Millot, M.; Rygg, J. R.; Celliers, P. M.; Eggert, J. H.; Jeanloz, R.; Collins, G. W. (2021). "Evidence of hydrogen−helium immiscibility at Jupiter-interior conditions". Nature. 593 (7860): 517–521. Bibcode: 2021Natur.593..517B. doi: 10.1038/s41586-021-03516-0. OSTI 1820549. PMID 34040210. S2CID 235217898.

Subprojects

Price, Fred W. (October 26, 2000). The Planet Observer's Handbook. Cambridge University Press. p.140. ISBN 978-0-521-78981-3 . Retrieved March 19, 2023. Tenn, Joe (March 10, 2006). "Edward Emerson Barnard". Sonoma State University. Archived from the original on September 17, 2011 . Retrieved January 10, 2007.

Weitering, Hanneke (January 10, 2018). " 'Totally Wrong' on Jupiter: What Scientists Gleaned from NASA's Juno Mission". space.com. Archived from the original on November 9, 2020 . Retrieved February 26, 2021. Doctor, Rina Marie (October 21, 2015). "Jupiter's Superstorm Is Shrinking: Is Changing Red Spot Evidence Of Climate Change?". Tech Times. Archived from the original on April 14, 2017 . Retrieved April 13, 2017. Michtchenko, T. A.; Ferraz-Mello, S. (February 2001). "Modeling the 5:2 Mean-Motion Resonance in the Jupiter–Saturn Planetary System". Icarus. 149 (2): 77–115. Bibcode: 2001Icar..149..357M. doi: 10.1006/icar.2000.6539.Youssef, A.; Marcus, P. S. (2003). "The dynamics of jovian white ovals from formation to merger". Icarus. 162 (1): 74–93. Bibcode: 2003Icar..162...74Y. doi: 10.1016/S0019-1035(02)00060-X. a b c d Kruijer, Thomas S.; Burkhardt, Christoph; Budde, Gerrit; Kleine, Thorsten (June 2017). "Age of Jupiter inferred from the distinct genetics and formation times of meteorites". Proceedings of the National Academy of Sciences. 114 (26): 6712–6716. Bibcode: 2017PNAS..114.6712K. doi: 10.1073/pnas.1704461114. PMC 5495263. PMID 28607079. Trachenko, K.; Brazhkin, V. V.; Bolmatov, D. (March 2014). "Dynamic transition of supercritical hydrogen: Defining the boundary between interior and atmosphere in gas giants". Physical Review E. 89 (3): 032126. arXiv: 1309.6500. Bibcode: 2014PhRvE..89c2126T. doi: 10.1103/PhysRevE.89.032126. PMID 24730809. S2CID 42559818. 032126. Li, Liming; Jiang, X.; West, R. A.; Gierasch, P. J.; Perez-Hoyos, S.; Sanchez-Lavega, A.; Fletcher, L. N.; Fortney, J. J.; Knowles, B.; Porco, C. C.; Baines, K. H.; Fry, P. M.; Mallama, A.; Achterberg, R. K.; Simon, A. A.; Nixon, C. A.; Orton, G. S.; Dyudina, U. A.; Ewald, S. P.; Schmude, R. W. (2018). "Less absorbed solar energy and more internal heat for Jupiter". Nature Communications. 9 (1): 3709. Bibcode: 2018NatCo...9.3709L. doi: 10.1038/s41467-018-06107-2. PMC 6137063. PMID 30213944.

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