Diagram age release easily

Aug 6th, 2022
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How to diagram age release

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Ovulation is a part of the menstrual cycle when the ovary releases a ripe egg, or ovum. Inside the ovary are hundreds of thousands of follicles. Each follicle is a hollow ball of cells with an immature egg in the center. The typical 28-day menstrual cycle begins on the first day of menstrual bleeding. During the first 7 days of the cycle, a few follicles begin to grow at the same time. These maturing follicles secrete estrogen hormone into the blood stream to prepare the lining of the uterus for pregnancy. Around Day 7, all of the follicles stop growing, and begin to degenerate, except for one. This dominant follicle continues to grow and nourishes the developing egg inside it. Around Day 12, the follicle secretes a large amount of estrogen into the blood stream. When the estrogen docHubes the hypothalamus and the pituitary gland in the brain, the anterior, or front part, of the pituitary gland releases a huge surge of luteinizing hormone into the blood stream. Around day

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In particular, by plotting a HR diagram for either a globular or open cluster of stars, astronomers can estimate the age of the cluster from where stars appear to turnoff the main sequence (see the entry on main sequence for how this works).
because all of a clusterss stars were born at the same time, we can measure a clusters age by finding the main-sequence turnoff point on an H-R diagram of its stars. The clusters age is equal to the hydrogen-fusion lifetime of the hottest, most luminous stars that remain on the main sequence.
In particular, by plotting a HR diagram for either a globular or open cluster of stars, astronomers can estimate the age of the cluster from where stars appear to turnoff the main sequence (see the entry on main sequence for how this works).
It is impossible to determine the age of a single star all by itself. The only real means we have to determine stellar ages is through the study of star clusters.
What is the approximate age of the star cluster in the H-R diagram? (Hint: Main sequence stars of spectral types O and B have a core supply of hydrogen that is sufficient to last about 250 million years; types A and F, about 2 billion years; type G about 10 billion years; types K and M about 30 billion years.
The Hertzsprung-Russell diagram shows the relationship between a stars temperature and its luminosity. It is also often called the H-R diagram or colour-magnitude diagram. It is a very useful graph because it can be used to chart the life cycle of a star. We can use it to study groups of stars in clusters or galaxies.
By placing the stars in a globular cluster on a Hertzprung-Russell diagram, astronomers can determine the clusters age by looking at the main sequence turnoff point and comparing it with models of stellar evolution.
One of the most useful and powerful plots in astrophysics is the Hertzsprung-Russell diagram (hereafter called the H-R diagram). It originated in 1911 when the Danish astronomer, Ejnar Hertzsprung, plotted the absolute magnitude of stars against their colour (hence effective temperature).

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