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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Answer:
Shakespeare was a man who wrote romantic poems and he was also a player
Explanation:
C
Explanation: it just is
The answer is:
a) What do pupils learn to create?
b) What do teachers train pupils to do?
c) Where do pupils learn photography?
d) What do pupils display in the classroom?
e) What attracts the eye?
The task consists in writing a question for each answer. As a consequence, each reply answers a question now which asks for information about the School Photography Club. For example, what students learn to do and where they exhibit their work.
Answer:
Aristotle's concept of scale of nature that the Elizabethans later adopted and modified was the belief that everything on Earth has a place in the natural order, which is determined by the creator.
Explanation:
Elizabethans adopted and modified was the belief that everything on Earth has a place in the natural order, which is determined by the creator.
