Answer:
<u>Realizing his date wasn't coming, he looked down at his lap and let out a long, weary sigh. </u>
I think it would be the first answer
Stage 1- Stars are born in a region of high density Nebula, and condenses into a huge globule of gas and dust and contracts under its own gravity.
This image shows the Orion Nebula or M42 .
Stage 2 - A region of condensing matter will begin to heat up and start to glow forming Protostars. If a protostar contains enough matter the central temperature reaches 15 million degrees centigrade.
This image is the outflow (coloured red)and protostar.
Stage 3 - At this temperature, nuclear reactions in which hydrogen fuses to form helium can start.
Stage 4 - The star begins to release energy, stopping it from contracting even more and causes it to shine. It is now a Main Sequence Star.
The nearest main sequence star to Earth, the Sun
Stage 5 - A star of one solar mass remains in main sequence for about 10 billion years, until all of the hydrogen has fused to form helium.
stage 6 - The helium core now starts to contract further and reactions begin to occur in a shell around the core.
give me your instagram profile name for chat
Answer:
not so much.....
Explanation:
I only liked to go to dinner when the dinner is not from my side,that will be given by my friend or another one, only then I liked to go to dinner. LoL....
just kidding brother.....
:-befrank
They should both restate the claim. Your conclusion could have a Call To Action which tells the reader that you are giving a reference to him/her.