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The formation of Saturn and its disk is simulated using a new N-body self-gravitational model. It is demonstrated that the
formation of the disk and the planet is the result of gravitational contraction of a slowly rotated particle cloud that have
a shape of slightly deformed sphere. The sphere was flattened by a coefficient of 0.8 along the axis of rotation. During the
gravitational contraction, the major part of the cloud transformed into a planet and a minor part transformed into a disk.
The thin structured disk is a result of the electromagnetic interaction in which the magnetic forces acting on charged particles
of the cloud originate in the core of the planet. The simulation program gives such parameters of Saturn as the escape velocity
of about 35 km/s at the surface, density, rotational velocities of the rings and temperature distribution. 相似文献
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B. I. Stepanov Institute of Physics, Academy of Sciences of Belarus, 70, F. Skorina Ave., Minsk, 220072, Belarus. Translated
from Zhurnal Prikladnoi Spektroskopii, Vol. 62, No. 2, pp. 200–205, March–April, 1995. 相似文献
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Saratov State University, 83 Astrakhanskaya Str., Saratov, 410601, Russia. Translated from Zhurnal Prikladnoi Spektroskopii,
Vol. 62, No. 6, pp. 49–57, November–December, 1995. 相似文献
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Zaitseva V. A. Lovchikova L. P. Naumenko E. K. Kononovich S. I. Nikonenko S. V. Plyuta V. E. 《Journal of Applied Spectroscopy》1996,63(6):772-778
Journal of Applied Spectroscopy - 相似文献
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S. I. Druzhinin M. V. Rusalov B. M. Uzhinov M. V. Alfimov S. P. Gromov O. A. Fedorova 《Journal of Applied Spectroscopy》1995,62(3):458-461
Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 62, No. 3, pp. 69–72, May–June, 1995. 相似文献
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