Jupiter - Carrera
Where can I find a book about Jupiter?
Encyclopedia of Astronomy and Astrophysics. Bristol: Institute of Physics Publishing. ISBN 978-0-12-226690-4. ^ Rogers, John H. (1995). The giant planet Jupiter. Cambridge University Press. pp. 188–189. ISBN 978-0-521-41008-3. Retrieved March 19, 2023. ^ Fimmel, Richard O.; Swindell, William; Burgess, Eric (August 1974).
Is Jupiter a real planet?
The existence of the planet Jupiter has been known since ancient times. It is visible to the naked eye in the night sky and can occasionally be seen in the daytime when the Sun is low. To the Babylonians, this planet represented their god Marduk, chief of their pantheon from the Hammurabi period.
Does Jupiter have a solid core?
It is still unclear if deeper down, Jupiter has a central core of solid material or if it may be a thick, super-hot and dense soup. It could be up to 90,032 degrees Fahrenheit (50,000 degrees Celsius) down there, made mostly of iron and silicate minerals (similar to quartz).
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Comparative Saturn?•Versus?•Jupiter Tether Operation
28-Jul-2018 Carrera-Calvo I. (2018). Comparative. Saturn-versus-Jupiter tether operation. Journal of Geophysical Research:. |
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The Possible Formation of Jupiter from Supersolar Gas
16-Jun-2022 the possibility that Jupiters current composition was acquired via the ... Yang |
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Diverse Protoplanetary Disk Morphology Produced by a Jupiter
06-Sept-2018 to trigger the streaming instability (Carrera et al. 2015). In addition when a disk managed to build a Jupiter-mass planet |
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BETsMA v2.0: A friendly software for the analysis of electrodynamic
electrodynamic tether missions in Jupiter [5] J. R. Sanmartin J. Pelaez |
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BETsMA v2.0: A friendly software for the analysis of electrodynamic
electrodynamic tether missions in Jupiter. [5] J. R. Sanmartin J. Pelaez |
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The Metallicity Distribution and Hot Jupiter Rate of the Kepler Field
21-Mar-2017 explain the discrepant hot Jupiter occurrence rates; the metallicity ... [Fe/H] = 0.01 ± 0.04 from a sample of 18 stars; Carrera &. |
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Diverse Protoplanetary Disk Morphology Produced by a Jupiter
to trigger the streaming instability (Carrera et al. 2015). In addition when a disk managed to build a Jupiter-mass planet |
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Design of a low-thrust assisted trajectory to Saturn
portion of the Jupiter-to-Saturn transfer and implements a steering law that minimizes Sanmartín et al.17 Sanmartín |
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Investigating the presence of stellar companions around hot Jupiter
15-Nov-2019 Jupiter host stars using MagAO. ... 1.2.1 Hot Jupiter properties . ... Recently a study by Daniel Carrera et al. modeled in 2019 the ... |
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Tether capture of spacecraft at Neptune
Jupiter's Europa or Saturn's Enceladus electrodynamic tethers can J. Pelaez |
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