Ejecta distribution from impact craters on Ryugu: possible origin of the bluer units

Abstract

Asteroid (162173) Ryugu was the first spinning-top-shaped asteroid to be closely approached by a probe, the Hayabusa2 spacecraft, which sent numerous high-resolution images of Ryugu to the Earth and revealed the nature of this type of asteroid. One of the notable features of Ryugu is the equatorial ridge, which is considered the result of rapid spin in the past. Despite the advanced age of the ridge, indicated by the presence of numerous craters, the ridge exhibits a bluish color, indicating that it is covered with fresh material. In addition to Ryugu, many other asteroids have similar blue areas, which are considered the result of ejecta emplacement. We examined the distribution of ejecta blankets from actual craters on Ryugu to assess ejecta emplacement as a possible origin of Ryugu's bluer units. We determined that when Ryugu's rotation was fast, ejecta from craters formed at lower latitudes accumulated along the equator, which may explain the bluish color of the equatorial ridge. On the other hand, ejecta emplacement does not fully explain the bluish color of Tokoyo Fossa, although we attempted to find the corresponding ejecta blankets.

21 pages 8 figures

References in corpus (5)

• Landslides and Mass Shedding on Spinning Spheroidal Asteroids
• The Western Bulge of 162173 Ryugu Formed as a Result of a Rotationally Driven Deformation Process
• The spatial distribution of impact craters on Ryugu
• Evidence for Surface Variegation in Rosetta OSIRIS Images of Asteroid 2867 Steins
• Rotational effect as the possible cause of the east-west asymmetric crater rims on Ryugu observed by LIDAR data

Cited by in corpus (2)

• Ejecta emplacement as the possible origin of Ryugu's equatorial ridge
• Secondary cratering from Rheasilvia as the possible origin of Vesta's equatorial troughs