The Hertzsprung-Russel Diagram (Figure 4) shows patterns of __, __, and __ of __ a. distance, composition, size, stars. b. mass, size, color, asteroids. c. size, age, distance, stars. d. temperature, brightness, color, stars. e. composition, size, gas content, planets. 59. Which of the following does NOT characterize the type of star we would find at r, s, t, and u on the Hertzsprung-Russel Diagram (Figure 4, middle right side)? b. have a very large diameter compared to our sun. d. form from stars like our own when they run out of hydrogen fuel. a. are red in color. c. are very dim stars e. are relatively cool stars. 60. Which of the following WOULD NOT characterizes the type(s) of star we would find at g, m, n, o, and p on the Hertzsprung-Russel Diagram (Figure 4) a. are all smaller than q,i,h. b. fuse hydrogen into helium. c. are called, “the main sequence”. d. fuse He into heavier elements. e. get smaller towards the righ

Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
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The Hertzsprung-Russel Diagram (Figure 4) shows patterns of __, __, and __ of __
a. distance, composition, size, stars. b. mass, size, color, asteroids. c. size, age, distance, stars. d. temperature, brightness, color, stars. e. composition, size, gas content, planets.

59. Which of the following does NOT characterize the type of star we would find at r, s, t, and u on the

Hertzsprung-Russel Diagram (Figure 4, middle right side)?
b. have a very large diameter compared to our sun.
d. form from stars like our own when they run out of hydrogen fuel.

a. are red in color. c. are very dim stars

e. are relatively cool stars.

60. Which of the following WOULD NOT characterizes the type(s) of star we would find at g, m, n, o, and p on the Hertzsprung-Russel Diagram (Figure 4) a. are all smaller than q,i,h. b. fuse hydrogen into helium. c. are called, “the main sequence”. d. fuse He into heavier elements. e. get smaller towards the right side

igure 4:
D
ons I bartleby
X
CICEREER
* m
1
MEL
C
*q #i
#i
#h
*r*t *u
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P
The "apparent magnitude X +
Ⓒ
Q
>
Transcribed Image Text:igure 4: D ons I bartleby X CICEREER * m 1 MEL C *q #i #i #h *r*t *u #S ‘0 P The "apparent magnitude X + Ⓒ Q >
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