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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To create tension and suspense
Answer:
I think its b but am not sure
Explanation:
It means extraordinarily good or wonderful.
Answer:
d. The words "Running head" appear on the title page only, with the header being listed in the left margin and the page number being listed in the right margin of every page.
Explanation:
A running head is a short title that appears at the top of every page of any academic paper. It is in the page header where it identifies the pages for the readers so as not to make any confusion even if the pages get lost. According to the APA or American psychological Association style of writing, the "running heads" appear on the title page only, with the header being listed in the left margin and the page number being listed in the right margin of every page.