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the claim
The particle density of the asteroid belt is extremely low.
the verdict
SUPPORTED
the evidence backs this
refutedsupported
the weight of evidence
1 source for · 0 against
AS REPORTEDno primary record reached; this is what the reporting says

Reference sources confirm that the asteroid belt has a very low density of materials, with spacecraft safely traversing it because the odds of colliding with an asteroid are extremely small.

Evidence for · 1
cited by 0
The asteroid belt is a torus-shaped region in the Solar System, centered on the Sun and roughly spanning the space between the orbits of the planets Jupiter and Mars. It contains a great many solid, irregularly shaped bodies called asteroids or minor planets. The identified objects are of many sizes, but much smaller than planets, and, on average, are about one million kilometers (or six hundred t The high population of the asteroid belt makes for an active environment, where collisions between asteroids occur frequently (on deep time scales). Impact events between main-belt bodies with a… The first spacecraft to traverse the asteroid belt was Pioneer 10, which entered the region on 16 July 1972. At the time, there was some concern that the debris in the belt would pose a hazard to the spacecraft, but it has since been safely traversed by multiple spacecraft without incident. Pioneer 11, Voyagers 1 and 2 and Ulysses passed through the belt without imaging any asteroids. Cassini measured plasma and fine dust grains while traversing the belt in 2000. On its way to Jupiter, Juno traversed the asteroid belt without collecting science data. Due to the low density of materials within the belt, the odds of a probe running into an asteroid are estimated at less than 1 in 1 billion. Most main belt asteroids imaged to date have come from brief flyby opportunities by probes headed for other targets. Only the Dawn mission has studied main belt asteroids for a protracted period in orbit. The Galileo spacecraft imaged 951 Gaspra in 1991 and 243 Ida in 1993, then NEAR imaged 253 Mathilde in 1997 and landed on near–Earth asteroid 433 Eros in February 2001. Cassini imaged 2685 Masursky in 2000, Stardust imaged 5535 Annefrank in 2002, New Horizons imaged 132524 APL in 2006, and Rosetta imaged 2867 Šteins in September 2008 and 21 Lutetia in July 2010. Dawn orbited Vesta between July 2011 and September 2012 and has orbited Ceres since March 2015. The Lucy space probe made a flyby of 152830 Dinkinesh in 2023 and 52246 Donaldjohanson in 2025 on its way to study the Jupiter trojans. As of 2026, there are several future and proposed missions to the asteroid belt. The NASA spacecraft Psyche will enter orbit around large M-type asteroid 16 Psyche in 2029. Additionally, Tianwen-2 is scheduled to visit main belt comet 311P/PanSTARRS in 2035. The future UAESA spacecraft MBR Explorer, which is planned to launch in 2028 will visit main belt asteroids 10253 Westerwald, 623 Chimaera, 13294 Rockox, 88055 Ghaf, 23871 Ousha, and 59980 Moza, and enter orbit and land on 269 Justitia in 2035.
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The analysis

rails:sufficiency:supported:single_source:for=1+0p:against=0+0p | v55:sufficiency

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  1. Asteroid beltreferenceno side taken
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first checked01 Aug 2026
judged → COMMON KNOWLEDGE · 9501 Aug 2026
held for human review07 Aug 2026
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