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Open AccessA contact binary satellite of the asteroid (152830) Dinkinesh
Asteroids with diameters less than about 5 km have complex histories because they are small enough for radiative torques (that is, YORP, short for the Yarkovsky–O’Keefe–Radzievskii–Paddack effect)1 to be a notabl...
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Open AccessThermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation
We present distributions of the zonal-mean temperature and static stability in the Venusian atmosphere obtained from Venus Express and Akatsuki radio occultation profiles penetrating down to an altitude of 40 ...