So Loeb and colleagues calculated just
how big an asteroid, how strong a supernova, or how powerful a gamma - ray burst would have to be to inject that much energy into Earth's oceans.
Not exact matches
To determine which theory is correct, the researchers needed to find some of the
asteroid belt's original occupants to see
how big they are.
That's just long enough to make a
big difference in
how an
asteroid evolves.
How our planet's water arrived may be a story of
big, bullying planets and ice - filled
asteroids.
The authors suggest that searches for these impact ejecta layers will be more fruitful for determining
how many times Earth was hit by
big asteroids than searches for large craters.
u One of the
big problems in the current story on
how asteroids evolved is: «How do gas and dust in a hypothetical solar nebula condense into dense boulders (asteroids, planetesimals, and meteoroids)?&raq
how asteroids evolved is: «
How do gas and dust in a hypothetical solar nebula condense into dense boulders (asteroids, planetesimals, and meteoroids)?&raq
How do gas and dust in a hypothetical solar nebula condense into dense boulders (
asteroids, planetesimals, and meteoroids)?»