Here's how we know: astronomers can estimate how many
asteroids of a given size are out there, even if we haven't seen them all, by looking at the rate of re-detection, or how often we see the same asteroid a second time.
Not exact matches
The analysis
of the orbital evolution
of the meteorite has showed, according to researchers, a «disturbing similarity» with the evolution
of 2014 UR116 which,
given its
size and minimum distance
of intersection with the orbit
of the Earth, has been classified as a potentially dangerous
asteroid.
If it's any comfort, Chodas explains that the chance
of asteroid SG344's colliding with Earth in 2030 is less than the chance that an undiscovered object
of the same
size will hit Earth in any
given year.
Giving the advantage
of its high - angular resolving power (~ 7mas), TMT will be able to resolve a dozen large Trans - Neptunian objects and ~ 50 - 100 Trojan
asteroids, providing a good estimate
of their
size.
Given that Tau Ceti does not appear to be a young star, the ring
of dusty debris is believed to be produced by collisions between larger comets and
asteroids that break them down into smaller and smaller pieces, and Tau Ceti's disk is similar in
size and shape to the disk
of comets and
asteroids that orbits the Sun, Sol.