Why is Ice More Prevalent in Comets than in Early Planetary States?

In summary: It is, therefore, abundant in outer space. Additionally, water molecules are relatively small and light, which makes them more easily carried by the wind and by space currents.
  • #1
skeleton
86
1
I have read a few times that comets are significant transports of ice (perhaps in having supplied water to fill Earth's oceans). That implies that water is more abundant in the few comets (in accumulated mass) that have impacted Earth than that which would have existed within the initial planet when it was forming.

1) WHY is ice more prevalent in comets than in the initial state of a planet?

2) Where did the ice come from when a comet is formed? This question may be equivalent to asking how is a comet formed?

3) Why is H2O, being a light molecule, more prevalent in outer space than other light molecules?

(Thanks in advance for your anticipated replies.)
 
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  • #2
Good questions skeleton.

skeleton said:
1) WHY is ice more prevalent in comets than in the initial state of a planet?
Comets form much farther away from the sun than Earth did. At those larger distances, water accumulates as ice which can stick/clump together into larger bodies (e.g. comets), instead of closer towards the sun where water tends to be gaseous or liquid (if its confined) at best.
See these links: http://en.wikipedia.org/wiki/Ice_line http://en.wikipedia.org/wiki/Habitable_zone

skeleton said:
3) Why is H2O, being a light molecule, more prevalent in outer space than other light molecules?
Water is far far less common than Hydrogen or Helium, or simple things like that. But water is also extremely stable (which is a big part of why its so useful/important for biology), and thus it is a little more common that just two hydrogens and an oxygen.

skeleton said:
2) Where did the ice come from when a comet is formed? This question may be equivalent to asking how is a comet formed?
I'm not sure about the details, but the overall picture is that 'dust' and 'ice' conglomerate together in the outer edges of the solar system (for the reasons explained in answering 1 and 3). When comets pass near the sun (e.g. haley, etc) they have large tails because the water/ice is being vaporized and blown off. This illustrates that comets would be unstable if they were always in the inner solar system.

Hope this helps.
 
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  • #3
Hydrogen is the most abundant element in the universe and oxygen is produced in abundance in most stars. Hydrogen bonds readily with oxygen and, once formed, water molecules are extremely stable.
 

1. How did comets acquire ice?

Comets are believed to have acquired ice through a process called accretion. This is when dust and gas particles in the solar system clump together to form larger bodies, such as comets. As these bodies move further away from the sun, the low temperatures allow for the ice to form and become part of the comet.

2. Where did the ice in comets come from?

The majority of the ice in comets is thought to have originated from the outer regions of the solar system, beyond the orbit of Neptune. This area, known as the Kuiper Belt, is a region of icy bodies that are remnants from the formation of the solar system.

3. How long has the ice been present in comets?

It is believed that the ice in comets has been present since the formation of the solar system, approximately 4.6 billion years ago. This ice has remained preserved due to the extremely low temperatures in the outer regions of the solar system where comets originate.

4. Can comets lose their ice?

Yes, comets can lose their ice as they approach the sun and begin to heat up. This process, known as sublimation, causes the ice to directly turn into gas and escape the comet's surface. This is why comets have a distinct tail when they get closer to the sun.

5. How does the ice in comets help us understand the solar system?

The ice in comets contains valuable information about the early formation of the solar system. By studying the composition of the ice, scientists can learn about the conditions and materials present during the formation of the solar system. Additionally, the presence of certain types of ice can also provide insight into the movement and changes in the solar system over time.

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