In the formation of the solar system nearly all of the mass of the solar nebula became ?

Answer Are
Terrestrial planets
GAS giant
SUN
OORT CLOUD
THANK YOU

if your doing lesson 7: the sun the answers are

1. C
2. D
3. B
4. C
5. C
6. B
hope it helped

bunny bunny’s answers are right i got a 100%

bunny bunny is right i did the test and got 100%

Well, if we're talking about the formation of the solar system, then nearly all of the mass of the solar nebula became... drumroll please... the Sun! That's right, the big ball of fiery goodness at the center of our solar system. It's like the star of the show, you know? But don't worry, there was still plenty of mass left over for other fun things like the terrestrial planets, gas giants, and even the Oort Cloud. So, it's like a cosmic buffet of mass, with the Sun as the main course. Enjoy!

In order to determine what nearly all of the mass of the solar nebula became in the formation of the solar system, we need to understand the process of solar system formation.

The solar system formed about 4.6 billion years ago from a cloud of gas and dust called a solar nebula. This nebula started collapsing under its own gravity and spinning due to its angular momentum. As it collapsed, the nebula flattened into a spinning disk.

Within this disk, particles began to collide and stick together, forming larger and larger objects known as planetesimals. These planetesimals eventually grew into protoplanets, which are essentially the precursors to planets.

Now, getting back to your question, nearly all of the mass of the solar nebula became two main categories of objects in the solar system:

1. Terrestrial planets: These are the inner planets of the solar system, including Mercury, Venus, Earth, and Mars. They are primarily composed of rock and metal. These planets formed closer to the Sun where it was hotter, and only rocky materials could condense and accumulate.

2. Gas giants: These are the outer planets of the solar system, including Jupiter and Saturn. They are primarily composed of hydrogen and helium, with smaller amounts of other gases and traces of rock and metal. The outer regions of the solar nebula were colder, allowing for the condensation of gases and the formation of these massive gas-rich planets.

Therefore, the correct answer to your question is that nearly all of the mass of the solar nebula became terrestrial planets and gas giants. The Sun, being the central star of the solar system, contains the majority of the remaining mass of the solar nebula. The Oort Cloud, on the other hand, is a hypothetical region far beyond the planets where long-period comets are believed to originate from, so it does not account for a significant portion of the solar nebula's mass.

I hope this explanation helps clarify the formation of the solar system and provides you with a satisfying answer to your question.