Here is the chief administrator, he will solve our problems.
Katniss, Peeta, and Effie watch the hunger games:)
Answer:
- Listen to others. Don't make others follow you. Everyone has their own strengths.
- Make yourself heard. This might be the complete opposite to the tip I put before, but it's not. Everyone has their own strengths, including you. If you are smart, try to help your friend with their math homework, or if you are athletic, teach your friend football. Little things that make them feel better.
- Know who is your friend. Peer pressure is something that a lot of leaders struggle with. Don't lead your friends astray and don't get led astray by your friends.
- And lastly, Know your leader. Your leaders, parents, teachers, the principal. Remember to always listen to them, cause they have good advice for you.
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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