the file is now available for the sale and will sent a message in the mail on Monday after the company has it in the news channel and is currently working with my family for you and my
A to 2, B to 3, C to 1, and D to 4. Happy to help! ☺
B. is the answer. "Until I get a replacement for my broken cellular phone I will not be able to call you on my way home."
P.S. the answer C. had way too amny comma's in all the wrong places.
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.
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A person of great knowledge of money and business
