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Rogue Asteroids in the Inner Main Asteroid Belt
2014Very red featureless asteroids (spectroscopic D-types) are common among Jupiter Trojans, Hildas, and the outer main belt, and are thought to have formed in the outer solar system. Dynamical models of planetary migration and orbital drift by the Yarkovsky effect predict these D-types could have been transported as close to the sun as the middle main ...
Demeo, Francesca E. +4 more
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Olivine-rich asteroids in the main asteroid belt
2015Olivine-dominated asteroids, classified as A-types with near-infrared spectral measurements are largely thought to be the mantle remnants of disrupted differentiated small bodies. These A-type asteroids hold clues to asteroid differentiation and to the collisional history of those differentiated bodies.
Demeo, Francesca E. +5 more
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1996
In 1772, Johann Titius, a German astronomer, came to Johann Bode at the Berlin Observatory with a simple mathematical relationship he had discovered that appeared to give the orbits of the planets. He pointed out that if you start with the series 0, 3, 6, 12, 24,..., add four to each, then divide by 10 you get the distance to each of the planets in ...
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In 1772, Johann Titius, a German astronomer, came to Johann Bode at the Berlin Observatory with a simple mathematical relationship he had discovered that appeared to give the orbits of the planets. He pointed out that if you start with the series 0, 3, 6, 12, 24,..., add four to each, then divide by 10 you get the distance to each of the planets in ...
openaire +1 more source
Solar System evolution from compositional mapping of the asteroid belt
Nature, 2014Benoit Carry
exaly