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Do any stars appear in both groups? How much overlap is there between the groups?

There are very few stars that appear in both groups. However, the number of these stars is very scarce and there the overlap as observed by the HR diagram is also very limited. Majority of the stars fall in their own respective groups i.e. either converted into Red Giants or end up as White Dwarfs and Black holes. Therefore, it can also be said that the few stars falling in both groups or in overlap region are few exceptions only.

What are the brightest and dimmest luminosity stars in each group? What are the highest and lowest temperature stars in each group? And, what are the largest and smallest radius stars in each group? If you highlight the whole table, you can sort by each column to easily finding the largest and smallest values. (Otherwise, you will need to figure it out by looking down the list.)

The Red Giant stars are the brightest while the White dwarfs along with some stars on the main sequence line are the dimmest stars in each group.

Sirius B is the brightest white star while Conopus is the brightest and hottest Red Giant. Bernards Star is the dimmest star on the HR diagram. In the HR Diagram, the star with highest temperature has 40,000K of temperature while the lowest is of 2500K (Bernard’s Star).

Copy and paste your completed HR Diagram.

How do the nearest and brightest stars compare? Does this agree with your hypothesis from the Pre-lab Assignment?

The nearest stars have cooler temperatures. They also have dimmer luminosity and their size is also considerably smaller. Also, the color of the nearest stars is red. However, in case of the brightest stars, they are hotter in temperature. Their luminosity is also higher i.e. they are brighter and larger in size. Their color is also bluer.

This finding is clearly in agreement with the hypothesis for the pre-lab assignment as it confirms the general properties of the two categories of the stars.

How can the differences between nearest and brightest stars be explained? Furthermore, if we presume that the Sun is not in a particularly unique part of the galaxy, what do your results tell you about the relative numbers of very bright and very dim stars?

The nearest stars are located at the bottom of the HR diagram while the brightest stars are located on top of the diagram. The brightest stars include Blue Giants and White dwarfs while the cooler stars include red giants as well as some main sequence stars. It is the distance and direction travelled by the star on the graph that determines its category and the nearest or the brightest location. Furthermore, the presumed number of hottest and collect stars appear to be more or less equivalent according to the generated HR Diagram – ignoring the position of the sun.

References

Schwarzschild, M. (2015). Structure and evolution of stars. Princeton University Press.

Portegies Zwart, S. F., McMillan, S. L., Hut, P., & Makino, J. (2001). Star cluster ecology—IV. Dissection of an open star cluster: photometry. Monthly Notices of the Royal Astronomical Society321(2), 199-226.

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