This is an example of irony:
Nothing is perfect. This was one of Mrs. Hopewell's favorite sayings. Another was: that is life! And still another, the most important, was: well, other people have their opinions too.
From the excerpt above, we see Mrs. Hopewell adding the name to the girl eventhough the girl feel that it's intrusive and she feel that she got to has a say about it. But despite that, Hopewell's favourite saying is other people have their opinions too.
Answer:
HOPE IT WILL HELP YOU
Explanation:
The information in this booklet has been adapted from “The Americans with Disabilities Act Questions and Answers” document produced by the U.S. Equal Employment Opportunity Commission and U.S. Department of Justice, Civil Rights Division, October 2008 version.
This publication was produced as a collaborative project by the ADA National Network, which is funded by the U.S. Department of Education, National Institute on Disability and Rehabilitation Research. This document does not reflect the opinions of the U.S. Department of Education and is not a legal determination of your rights and/or responsibilities under the ADA. It is provided as technical assistance and you should consult an attorney for legal matters.
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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