Iupiter

Articul por Ladin Val Badia

Iupiter (simbol: ; dal latin Iovem, accusatif de Iuppiter) y cun referimënt al inom de Zeus (tl grech antich Ζεύς), le pere dles divinités tla mitologia greca, é le cuinto planët dl Sistem solar en cunt de destanza dal Sorëdl y le plü gran de döt le sistem di planëc. Süa massa è dui iadi y mez tan gran respet a chëra de düc i atri planëc adöm^[1]. Adöm cun Saturn, Uran y Netun él classifiché sicöche “gigant de gas”.

Süa composiziun ti somëia a chëra dl Sorëdl, cun idrogen, elio, amoniaca, ega y metan. Al vëgn araté che so nucleus sides metü adöm da crëp cun carbonium y silicac de fer curis da n mantel de idrogen metalich y na atmosfera^[2] cun presciuns dër altes^[3]. Le corú dl’atmosfera esterna, che é metüda adöm por le 88-92% da idrogen molecolar y da n 8-12% de elio^[4], vá dal ross lominus al ross cun chëra che vëgn nominada “Gran Tacia Cöcena^[5]. Iupiter é le cuarto corp dl cil plü slominant do le Sorëdl, la Löna y Venus^[6].

Le sistem d’aní de Iupiter é metü adöm dantadöt da silicac. Ai aní plü esterns ti vëgnel dit “aní Gossamer” ^[7]. Atualmënter él gnü identifiché 79 satelic naturai de Iupiter^[8].

Dal 1973 inant él gnü a se le dé deplü surajors (fly-by) de Iupiter cun sondes: la Pioneer 10 y dl 1974 la Pioneer 11^[9].

Notes

↑ George H. A. Cole e Michael M. Woolfson, Planetary Science: The Science of Planets Around Stars, CRC Press, 2002, p. 68, ISBN 978-0-7503-0815-1
↑ T Guillot, A comparison of the interiors of Jupiter and Saturn, te Planetary and Space Science, vol. 47, 10–11, 1999, pl. 1183–200, DOI:10.1016/S0032-0633(99)00043-4
↑ Linda T. Elkins-Tanton, Jupiter and Saturn, New York, Chelsea House, 2006, ISBN 0-8160-5196-8.
↑ Linda T. Elkins-Tanton, Jupiter and Saturn, New York, Chelsea House, 2006, ISBN 0-8160-5196-8.
↑ A. P. Ingersoll, T. E. Dowling, P. J. Gierasch, et al, Dynamics of Jupiter's Atmosphere (PDF), Lunar & Planetary Institute.
↑ Peter J. Gierasch, Philip D. Nicholson, Jupiter, World Book @ NASA, 2004.
↑ L. W. Esposito, Planetary rings, te Reports On Progress In Physics, vol. 65, 2002, pp. 1741–1783, DOI:10.1088/0034-4885/65/12/201
↑ Jupiter's Moons: 12 More Found, 79 Known - Sky & Telescope, su Sky & Telescope, 17 luglio 2018.
↑ Eric Burgess, By Jupiter: Odysseys to a Giant, New York, Columbia University Press, 1982, ISBN 0-231-05176-X.

[1] George H. A. Cole e Michael M. Woolfson, Planetary Science: The Science of Planets Around Stars, CRC Press, 2002, p. 68, ISBN 978-0-7503-0815-1

[2] T Guillot, A comparison of the interiors of Jupiter and Saturn, te Planetary and Space Science, vol. 47, 10–11, 1999, pl. 1183–200, DOI:10.1016/S0032-0633(99)00043-4

[3] Linda T. Elkins-Tanton, Jupiter and Saturn, New York, Chelsea House, 2006, ISBN 0-8160-5196-8.

[4] Linda T. Elkins-Tanton, Jupiter and Saturn, New York, Chelsea House, 2006, ISBN 0-8160-5196-8.

[5] A. P. Ingersoll, T. E. Dowling, P. J. Gierasch, et al, Dynamics of Jupiter's Atmosphere (PDF), Lunar & Planetary Institute.

[6] Peter J. Gierasch, Philip D. Nicholson, Jupiter, World Book @ NASA, 2004.

[7] L. W. Esposito, Planetary rings, te Reports On Progress In Physics, vol. 65, 2002, pp. 1741–1783, DOI:10.1088/0034-4885/65/12/201

[8] Jupiter's Moons: 12 More Found, 79 Known - Sky & Telescope, su Sky & Telescope, 17 luglio 2018.

[9] Eric Burgess, By Jupiter: Odysseys to a Giant, New York, Columbia University Press, 1982, ISBN 0-231-05176-X.

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