Diagram age log easily

Aug 6th, 2022
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How to diagram age log

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okay lets talk about log scales and how to read them in engineering we typically use a base 10 log scale and what that means is that every major tick mark is equal to 10 to an exponent and that exponent increases as you proceed increasingly along the log scale so simply really to just see it this way look point 1 its 10 to the minus 1 1 is 10 to the 0 10 is 10 to the 1 and 100 is 10 to the 2 so look at the exponent minus 1 0 1 2 etc okay so how do you read the log scale well what youre gonna do is youre gonna read the tick marks right so lets first actually see how we read the tick marks lets just pick this tick mark right here because this is a 1 and this is a 10 this tick marks are spaced by ones so this would be 2 this would be 3 this would be 4 5 6 7 8 9 okay now if we move to the right here Ive seen students for example right here 16 or sorry 11 12 13 14 no thats not right here we have to go by tens right so this is 20 30 40 etc okay this one over here is 90 I hope that y

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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).
For the higher mass, luminosity will be higher. From the HR diagram of open clusters, as the luminosity increases the stars age decreases. Therefore, the star with higher mass will have less age. Therefore, the highest mass star is the youngest one.
Essentially, astronomers determine the age of stars by observing their spectrum, luminosity and motion through space. They use this information to get a stars profile, and then they compare the star to models that show what stars should look like at various points of their evolution.
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.
As time passes the most massive stars at the top of the main sequence evolve into red giants. Therefore, the older the cluster, the fewer stars to be found at the top of the main sequence, and an obvious grouping of red giants will be seen at the top right of the HR diagram.
And globular clusters contain the oldest stars. Their age is determined by their almost complete lack of what astronomers call metals, the heavier elements forged in star interiors. Because the early universe, before the first stars and galaxies were born, contained only hydrogen and helium.
By determining the mass of the main-sequence turnoff stars, we get the age of the cluster. The cluster age equals the main-sequence lifetime of the turnoff stars. This is one of the ways we have studied the age of the Universe and the formation history of the Galaxy.
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.
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.
Answer and Explanation: A star cluster whose brightest main sequence stars are white is the youngest. The color of the star shows its age.

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