ASTR 1303 - Ages and Distances of Clusters

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Stephen F Austin State University *

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105

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Astronomy

Date

Dec 6, 2023

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pdf

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2

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Name: Type Your Name Here Lab Section: ### Date: ##/##/#### ASTR 1303 - Ages and Distances of Clusters Select File Make a Copy from the menu to begin to edit this document. Complete the table on page 2 and then answer the questions below. Questions 1. How would you characterize the H-R diagrams of a young cluster and of an old cluster? Type your answer here. 2. What are the effects of interstellar reddening on the measured distances and observed colors of stars? Type your answer here. 3. If interstellar reddening is not taken into account, how would the observed size of the galaxy and the universe be affected? Type your answer here. 4. Is star formation still occurring within our galaxy? Support your answer with the cluster ages you have just determined. Type your answer here. 5. The color-magnitude diagram of the open cluster NGC 2682 (M67) is very similar to the HR diagrams of all globular clusters. Is there anything you can conclude about globular clusters from this fact? Type your answer here.
Ages and Distances of Clusters Use the Color-Magnitude Diagrams to complete the table below. Cluster Name Distance Modulus m v - M v Distance (Parsecs) Color Excess CE Absorption Factor A = 3 X CE Distance Modulus (Corrected) m v - M v - A Corrected Distance (Parsecs) Distance (LY) Color of Main Sequence Turn-off Point Age (yrs) Mel 20 M45 NGC 6791 2000 MY IC 4725 NGC 6705 NGC 2632 NGC 2682 NGC 752 Distance in Parsecs = parsecs = 10^(( m v - M v + 5)/5) parsecs 𝑑 = 10 (𝑚−𝑀+5)/5 1 parsec = 3.26 lightyear 1 x 10 6 years = 1 Myr = 1 Million Years 1 x 10 7 years = 10 Myr = 10 Million Years 1 x 10 8 years = 100 Myr = 100 Million Years 1 x 10 9 years = 1000 Myr = 1000 Million Years
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