Zusammenfassung
Bevor wir uns der Frage zuwenden, welche Prozesse zur Entstehung unseres Sonnensystems geführt haben, müssen wir uns zunächst einige grundlegende Tatsachen ins Gedächtnis rufen (Unsöld u. Baschek 2005; Chambers 2005; Weigert et al. 2005):
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1.
Die Bahnen der Planeten sind nahezu kreisförmig und koplanar; sie besitzen den gleichen Umlaufsinn, der mit dem der Sonne übereinstimmt. Nach der Regel von Titius-Bode.
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Okrusch, M., Matthes, S. (2014). Die Entstehung unseres Sonnensystems. In: Mineralogie. Springer-Lehrbuch. Springer Spektrum, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-34660-6_34
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