Temperature Temperature (Fahrenheit) 32 72 Condition (kelvin) 199 296 Water freezes Room temp. Human body Water boils 2000 98.6 310 -Mercury 212 373 Venus Earth Mars 1000 500 200 Jupiter Saturn 100 - Uranus -Neptune 50 0.1 0.2 0.5 1.0 2.0 5.0 10 20 50 Distance from the Sun (AU) Temperature (kelvin) 20

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
Section: Chapter Questions
Problem 1LR
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Question

The graph in the upper right shows the temperatures at various distances
from the Sun during the formation of our solar system. (You
can assume that the planets formed at roughly their current distances
from the Sun, although that may not be strictly true.) Use it to answer
the following:
a. Which planet(s) formed at locations in the solar system where the
temperature was hotter than the boiling point of water?
b. Which planet(s) formed at locations in the solar system where the
temperature was cooler than the freezing point of water? 

Temperature Temperature
(Fahrenheit)
32
72
Condition
(kelvin)
199
296
Water freezes
Room temp.
Human body
Water boils
2000
98.6
310
-Mercury
212
373
Venus
Earth
Mars
1000
500
200
Jupiter
Saturn
100
- Uranus
-Neptune
50
0.1
0.2
0.5 1.0
2.0
5.0
10
20
50
Distance from the Sun (AU)
Temperature (kelvin)
20
Transcribed Image Text:Temperature Temperature (Fahrenheit) 32 72 Condition (kelvin) 199 296 Water freezes Room temp. Human body Water boils 2000 98.6 310 -Mercury 212 373 Venus Earth Mars 1000 500 200 Jupiter Saturn 100 - Uranus -Neptune 50 0.1 0.2 0.5 1.0 2.0 5.0 10 20 50 Distance from the Sun (AU) Temperature (kelvin) 20
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Follow-up Question

1. What was the temperature at the location of Earth? 

2. What was the temperature at the location of Mars?

At temperatures hotter than the freezing point of water, light gases, such as hydrogen helium, likely had too much energy to condense together to form the large, gas giant, Jovian planets.

Over what range of distances from the sun would you expect to find light gases, such as hydrogen and helium to form a Jovian planet?

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