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The Planet Jupiter [PDF]

open access: possibleScience, 1963
Internal heat source, hydrogen deficiency, presence of gases that are precursors of life, and cloud band coloration in Jupiter ...
Nicholas Panagakos, Robert Jastrow
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Jupiter

2004
International ...
Encrenaz, Thérèse, Murdin, P.
openaire   +3 more sources

A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion

Nature, 2015
Thousands of transiting exoplanets have been discovered, but spectral analysis of their atmospheres has so far been dominated by a small number of exoplanets and data spanning relatively narrow wavelength ranges (such as 1.1–1.7 micrometres).
D. Sing   +20 more
semanticscholar   +1 more source

Jupiter's Interior as Revealed by Juno

Annual Review of Earth and Planetary Science, 2020
Jupiter is in the class of planets that we call gas giants, not because they consist of gas but because they were primarily made from hydrogen-helium gas, which upon gravitational compression becomes a metallic fluid.
D. Stevenson
semanticscholar   +1 more source

Jupiter: Atmosphere

2004
International ...
Drossart, Pierre, Murdin, P.
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Evidence for very early migration of the Solar System planets from the Patroclus–Menoetius binary Jupiter Trojan

Nature Astronomy, 2018
The orbital distribution of trans-Neptunian objects provides strong evidence for the radial migration of Neptune1,2. The outer planets’ orbits are thought to have become unstable during the early stages3, with Jupiter having scattering encounters with a ...
D. Nesvorný   +3 more
semanticscholar   +1 more source

Jupiter IX and Jupiter XII

Publications of the Astronomical Society of the Pacific, 1952
The ninth satellite of Jupiter was discovered and its orbit first computed by Nicholson in 1914 at the Lick Observatory. His most recent orbit,1 epoch about 1940, which we have been carrying on for a number of years, latterly with automatic computing machinery, has proved to be one of the most accurate of all those determined for Jupiter's satellites ...
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Life on Jupiter?

Origins of Life, 1974
The possibilities of life on Jupiter are discussed from the point view of life as we know it. That is, we assume that any life on Jupiter would not involve new principles foreign to us. Proteins would be a constituent as would fats and the other building blocks of living organisms on Earth.
openaire   +3 more sources

The Meteorology of Jupiter [PDF]

open access: possibleScientific American, 1976
The visible features of the giant planet reflect the circulation of its atmosphere. A model reproducing those features should apply to other planetary atmospheres, including the earth's.
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Jupiter’s Aurorae

1998
Planets with magnetic fields are found to display luminous curtains similar to the aurorae on Earth. This phenomenon occurs when charged particles traveling along the planet’s magnetic field lines collide with gases in the upper atmosphere, stimulating them to fluoresce or glow.
Daniel Fischer, Hilmar W. Duerbeck
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