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Dwarf planet Ceres. Image Credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA / Justin Cowart |
Small planets originate from the edge of our Solar System
New astronomical measurements in the infrared range have led to the identification of a heretofore unknown class of asteroids. An international research team including geoscientists from Heidelberg University has succeeded in characterizing these small planets using infrared spectroscopy. They are located in the asteroid belt between Mars and Jupiter and are – similar to the dwarf planet Ceres – rich in water. According to computer models, complex dynamic processes shifted these asteroids from the outer regions of our Solar System into today’s asteroid belt shortly after their creation.
With an equatorial diameter of approximately 900 kilometers, the dwarf planet Ceres is the largest object in the asteroid belt between Mars and Jupiter. Many other small planets orbit in this region as well. “These are the remains of the building materials from which the planets of our Solar System were created four and a half billion years ago. In these small bodies and their fragments, the meteorites, we find numerous relics that point directly to the process of planet formation,” explains Prof. Dr Mario Trieloff from the Institute of Earth Sciences of Heidelberg University. The current study shows that the small astronomical bodies originate from all regions of the early Solar System. By means of small bodies from the outer Solar System, water could have reached the still growing Earth in the form of asteroids, because the building blocks of the planets in the inner Solar System tended to be arid, according to Prof. Trieloff, who heads up the Geo- and Cosmochemistry research group.