Millions of asteroids exist, many are shattered remnants of planetesimals, bodies within the young Sun's solar nebula that never grew large enough to become planets. ... Individual asteroids are classified by their characteristic spectra, with the majority falling into three main groups: C-type, M-type, and S-type.
Millions of asteroids exist, many are shattered remnants of planetesimals, bodies within the young Sun's solar nebula that never grew large enough to become planets. ... Individual asteroids are classified by their characteristic spectra, with the majority falling into three main groups: C-type, M-type, and S-type.
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Answer:
Millions of asteroids exist, many are shattered remnants of planetesimals, bodies within the young Sun's solar nebula that never grew large enough to become planets. ... Individual asteroids are classified by their characteristic spectra, with the majority falling into three main groups: C-type, M-type, and S-type.
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Explanation:
Millions of asteroids exist, many are shattered remnants of planetesimals, bodies within the young Sun's solar nebula that never grew large enough to become planets. ... Individual asteroids are classified by their characteristic spectra, with the majority falling into three main groups: C-type, M-type, and S-type.