Fig. 20
Eccentricity vs. inclination for inner Solar System (q < 1.2 AU) asteroids and comets and the Bering Sea bolide. The nominal bolide solution is marked by the blue cross. The light blue area shows other possible radiant solutions within two sigma limits for the speed of 32 km s−1. The light green area is the same for the assumed speed of 27 km s−1. Asteroid and comet data are from the JPL Small-Body Database (https://ssd.jpl.nasa.gov/sbdb_query.cgi).
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