![]() |
|
According to this theory, the life of a star is said to begin with the collapse of a gas cloud--a doubtful beginning, as explained in Do new stars form today?. Bypassing this fundamental origin problem, a young star is said to begin in the “main-sequence” category. These are average stars with a stable light output. The great majority of stars are in the main sequence, including our sun. Then when a star's hydrogen fuel runs low, it becomes a red giant or super-giant star. The star expands hundreds of times in size and becomes somewhat cooler. Red giants include Betelgeuse and Aldebaran. Next, the star may either explode as a supernova or may slowly collapse into a small, hot white dwarf star. The companion star circling Sirius is such a dwarf. Such stars are said to be very old. [ If this information has been helpful, please prayerfully consider a donation to help pay the expenses for making this faith-building service available to you and your family! Donations are tax-deductible. ] Author: Dr. Donald B. DeYoung - adapted from Astronomy and the Bible: Questions and Answers, 2nd Edition (Grand Rapids, Michigan: Baker Books, 2000), 176 pp. Copyright © 2000, Films for Christ, All Rights Reserved - except as noted on attached “Usage and Copyright” page that grants ChristianAnswers.Net users generous rights for putting this page to work in their homes, personal witnessing, churches and schools. www.ChristianAnswers.Net |
