How closely packed are Jupiter’s Trojan asteroids?

The quantity density of asteroids in the primary belt about 10 instances larger than that of Jupiter’s Trojan asteroids.

How carefully packed are Jupiter’s Trojan asteroids in comparison with the density of the primary belt?

Doug Kaupa
Council Bluffs, Iowa

Jupiter’s Trojans are asteroids that share the fuel big’s orbit across the Solar, clustering at one in every of two Lagrange factors within the Jupiter-Solar system (L4 or L5, 60° forward of or behind Jupiter in its orbit, respectively).

It seems that main-belt asteroids (MBAs) and Trojan asteroids occupy a comparatively comparable quantity in house. The majority of MBAs lie between 2.1 and three.3 AU from the Solar, whereas Jupiter’s Trojans are 5 to five.3 AU from our star. Most of those our bodies (in each teams) have orbital inclinations lower than 30°.

You’ll be able to approximate the amount these asteroids occupy utilizing rings. So, image a torus with a round cross-section, with the interior and outer diameter being the interior and outer extents of the orbits simply given, in order that the amount every occupies is 61 AU3 and 58 AU3, respectively, for MBAs and Trojans. (One AU, or astronomical unit, is the typical Earth-Solar distance of 93 million miles [150 million kilometers]. So, 1 AU3 = 8 x 1023 miles3 [2.7 x 1024 km3].)

There are about 108 MBAs bigger than about 330 ft (100 meters) in diameter, and about 107 Trojans of this similar measurement. That makes the amount density of asteroids in the primary belt about 10 instances larger than that of Jupiter’s Trojan asteroids.

Nonetheless, MBAs are arduous to return by within the vastness of house. A sphere with a radius of about 249,000 miles (400,000 km) accommodates just one MBA bigger than 330 ft (100 m) in diameter.

Simone Marchi
Employees Scientist, Southwest Analysis Institute, Boulder, Colorado

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