An asteroid has a 5:2 orbital resonance with Jupiter. What is its orbital period (in years)? How far is it from the Sun in AU? How does the distance between the orbits of Mars and the asteroid compare to the distance between the orbits of Mars and Jupiter? Part 1 of 3 Orbital resonances compare how many orbits a body, in this case an asteroid, makes in terms of the orbit of a much larger body, in this case Jupiter. We can write resonances as (number of orbits of smaller body): (number of orbits of larger body). Na: N₂ If we want to know the orbital period of the smaller body, we can express this as a relation. The second number tells us how many times the larger body orbits and the first number tells us how many times the smaller body orbits. If we want the orbital period, we just take the ratio of these and multiply by the orbital period of the larger body. N P₂= Na An asteroid has a 5:2 orbital resonance with Jupiter. What is its orbital period (in years)? Pa = years Submit Skip (you cannot come back)

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
icon
Related questions
Question
Tutorial
An asteroid has a 5:2 orbital resonance with Jupiter. What is its orbital period (in years)?
How far is it from the Sun in AU?
How does the distance between the orbits of Mars and the asteroid compare to the distance between the orbits of Mars and Jupiter?
Part 1 of 3
Orbital resonances compare how many orbits a body, in this case an asteroid, makes in terms of the orbit of a much larger body, in this case Jupiter. We can write resonances as (number of orbits of smaller
body): (number of orbits of larger body).
Na: N₁
If we want to know the orbital period of the smaller body, we can express this as a relation. The second number tells us how many times the larger body orbits and the first number tells us how many times
the smaller body orbits. If we want the orbital period, we just take the ratio of these and multiply by the orbital period of the larger body.
Pa
=
Na
An asteroid has a 5:2 orbital resonance with Jupiter. What is its orbital period (in years)?
Pa
years
Submit Skip_(you cannot come back)
Transcribed Image Text:Tutorial An asteroid has a 5:2 orbital resonance with Jupiter. What is its orbital period (in years)? How far is it from the Sun in AU? How does the distance between the orbits of Mars and the asteroid compare to the distance between the orbits of Mars and Jupiter? Part 1 of 3 Orbital resonances compare how many orbits a body, in this case an asteroid, makes in terms of the orbit of a much larger body, in this case Jupiter. We can write resonances as (number of orbits of smaller body): (number of orbits of larger body). Na: N₁ If we want to know the orbital period of the smaller body, we can express this as a relation. The second number tells us how many times the larger body orbits and the first number tells us how many times the smaller body orbits. If we want the orbital period, we just take the ratio of these and multiply by the orbital period of the larger body. Pa = Na An asteroid has a 5:2 orbital resonance with Jupiter. What is its orbital period (in years)? Pa years Submit Skip_(you cannot come back)
Expert Solution
trending now

Trending now

This is a popular solution!

steps

Step by step

Solved in 3 steps with 2 images

Blurred answer
Follow-up Questions
Read through expert solutions to related follow-up questions below.
Follow-up Question
**Text Transcription:**

The region between Mars and Jupiter, where asteroids lie, extends from 1.52–5.20 AU from the Sun. To find the distance between Mars and this asteroid as a fraction of the total distance between Mars and Jupiter, we simply take their ratios:

\[ f = \frac{d_{Ma}}{d_{Mj}} \]

\[ f = \]

**Explanation:**

- **AU (Astronomical Unit):** A unit of measurement equivalent to the average distance from the Earth to the Sun, roughly 149.6 million kilometers (93 million miles).
  
- **Formula Explanation:**
  - The formula \( f = \frac{d_{Ma}}{d_{Mj}} \) is used to calculate the fraction \( f \), which represents the distance between Mars and the asteroid as a fraction of the total distance between Mars and Jupiter.
  - \( d_{Ma} \) is the distance from Mars to the asteroid.
  - \( d_{Mj} \) is the distance from Mars to Jupiter.
  
- **Input Field:**
  - Below the formula, there is an input field provided to enter the calculated fraction \( f \).
Transcribed Image Text:**Text Transcription:** The region between Mars and Jupiter, where asteroids lie, extends from 1.52–5.20 AU from the Sun. To find the distance between Mars and this asteroid as a fraction of the total distance between Mars and Jupiter, we simply take their ratios: \[ f = \frac{d_{Ma}}{d_{Mj}} \] \[ f = \] **Explanation:** - **AU (Astronomical Unit):** A unit of measurement equivalent to the average distance from the Earth to the Sun, roughly 149.6 million kilometers (93 million miles). - **Formula Explanation:** - The formula \( f = \frac{d_{Ma}}{d_{Mj}} \) is used to calculate the fraction \( f \), which represents the distance between Mars and the asteroid as a fraction of the total distance between Mars and Jupiter. - \( d_{Ma} \) is the distance from Mars to the asteroid. - \( d_{Mj} \) is the distance from Mars to Jupiter. - **Input Field:** - Below the formula, there is an input field provided to enter the calculated fraction \( f \).
Solution
Bartleby Expert
SEE SOLUTION
Follow-up Question
Kepler's Third Law tells us how the distance from the Sun relates to the orbital period of a body:

\[
\left( \frac{a}{1 \text{ AU}} \right)^3 = \left( \frac{p}{1 \text{ yr}} \right)^2
\]

So the distance from the Sun in AU based on the period calculated in Step 1 is:

\[ 
a = \_\_\_ \text{ AU} 
\]
Transcribed Image Text:Kepler's Third Law tells us how the distance from the Sun relates to the orbital period of a body: \[ \left( \frac{a}{1 \text{ AU}} \right)^3 = \left( \frac{p}{1 \text{ yr}} \right)^2 \] So the distance from the Sun in AU based on the period calculated in Step 1 is: \[ a = \_\_\_ \text{ AU} \]
Solution
Bartleby Expert
SEE SOLUTION
Recommended textbooks for you
Applications and Investigations in Earth Science …
Applications and Investigations in Earth Science …
Earth Science
ISBN:
9780134746241
Author:
Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:
PEARSON
Exercises for Weather & Climate (9th Edition)
Exercises for Weather & Climate (9th Edition)
Earth Science
ISBN:
9780134041360
Author:
Greg Carbone
Publisher:
PEARSON
Environmental Science
Environmental Science
Earth Science
ISBN:
9781260153125
Author:
William P Cunningham Prof., Mary Ann Cunningham Professor
Publisher:
McGraw-Hill Education
Earth Science (15th Edition)
Earth Science (15th Edition)
Earth Science
ISBN:
9780134543536
Author:
Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:
PEARSON
Environmental Science (MindTap Course List)
Environmental Science (MindTap Course List)
Earth Science
ISBN:
9781337569613
Author:
G. Tyler Miller, Scott Spoolman
Publisher:
Cengage Learning
Physical Geology
Physical Geology
Earth Science
ISBN:
9781259916823
Author:
Plummer, Charles C., CARLSON, Diane H., Hammersley, Lisa
Publisher:
Mcgraw-hill Education,