If a moon revolves opposite to the planet's rotation, it probably a. was captured after the planet formed. b. had its orbit altered by a collision. c. has a different composition than other moons have. d. formed very recently in the Solar System's history.

Short Answer

Expert verified
The moon was likely captured after the planet formed.

Step by step solution

01

- Understand the question

The question asks about the cause behind a moon revolving in the opposite direction of the planet's rotation.
02

- Analyze each option

Evaluate the likelihood of each option being the correct explanation for the moon's backward orbit.
03

- Option a: Captured moon

Moons captured after the planet formed might orbit differently because they were not originally part of the planet's development.
04

- Option b: Altered orbit

A collision could alter a moon’s orbit, possibly causing it to revolve in the opposite direction.
05

- Option c: Different composition

A different composition does not directly explain the direction of the moon’s orbit.
06

- Option d: Formed recently

Recent formation in the Solar System's history does not necessarily explain why the moon orbits in a reverse direction.
07

- Conclusion

Options a and b are plausible, but option a (captured moon) is more likely to explain an opposite direction orbit, as captured moons often have irregular orbits.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

captured moons
A captured moon is one that was not originally formed alongside its parent planet. Instead, it was gravitationally captured by the planet after both had already formed.
Captured moons often have irregular orbits that can be very different from the orbits of moons that formed with their planet.
These irregular orbits are usually elliptical or highly inclined. Sometimes, captured moons can even revolve opposite to the rotation of their parent planet.
This opposite direction orbit is called a retrograde orbit. One famous example of a captured moon is Neptune's moon, Triton.
Retrograde orbits are strong indicators that the moon was likely captured by the planet's gravity.
This is because typical moon formation follows the direction of the planet's spin, making retrograde motion unusual unless external forces like capture are involved.
orbital mechanics
Orbital mechanics is the study of the motions of celestial bodies under the influence of gravitational forces.
This concept helps us understand why moons and planets move the way they do in space.
The path of a moon or satellite around a planet is determined by the gravitational attraction between them. If a moon has a retrograde orbit, meaning it moves in the opposite direction of the planet's rotation, this can be explained by orbital mechanics.
  • If an object is captured by a planet's gravity, it can enter into various types of orbits, depending on its velocity and the angle of capture.
  • Orbital mechanics laws, such as Kepler's laws of planetary motion, help to predict the orbits of these celestial bodies.
  • Understanding these mechanics is crucial for space missions, satellite launches, and predicting the movement of natural celestial bodies in our Solar System.
Overall, orbital mechanics provides the foundation for why certain moons might behave differently.
planetary formation
Planetary formation is the process by which a planet forms from a disk of gas and dust surrounding a new star.
During this time, moons can also form from the same material orbiting the young planet. This typical moon formation results in moons that orbit in the same direction as the planet's rotation.
However, sometimes a moon does not follow this norm. If a moon has a retrograde orbit, it often means that it was captured after the planet was fully formed.
Contrastingly, moons like the ones that formed with the planet usually have prograde orbits, meaning they move in the same direction as the planet's rotation.
  • The presence of a retrograde moon suggests a more dynamic history, including potential gravitational interactions with other celestial bodies.
  • This has implications for understanding the history and evolution of the planet as well as the overall architecture of the Solar System.
Thus, studying planetary formation gives us insights into the various stages and processes that result in the diverse set of moons we observe today.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Planetary scientists have estimated that Io's extensive volcanism could be covering the moon's surface with lava and ash to an average depth of up to 3 millimeters (mm) per year. a. Io's radius is \(1,820 \mathrm{km}\). If you assume Io is a sphere, what are its surface area and volume? b. What is the volume of volcanic material deposited on Io's surface each year? c. How many years would it take for volcanism to perform the equivalent of depositing Io's entire volume on its surface? d. How many times might Io have "turned inside out" over the age of the Solar System?

Saturn's bright rings are located within the Roche limit of Saturn. This fact supports the theory that these rings (select all that apply) a. formed of moons torn apart by tidal stresses. b. formed at the same time that Saturn formed. c. are relatively recent. d. are temporary.

Scientists determine the geological history of the moons of the outer planets from a. seismic probing. b. radioactive dating. c. surface features. d. all of the above

Categorizing moons by geological activity is helpful because a. comparing them reveals underlying physical processes. b. geological activity levels drop with distance from the Sun. c. geological activity determines the size and composition of the moons. d. most moons are very similar to each other.

Particles at the very outer edge of Saturn's A Ring are in a 7: 6 orbital resonance with the moon Janus. If the orbital period of Janus is 16 hours 41 minutes \(\left(16^{\mathrm{h}} 41^{\mathrm{m}}\right),\) what is the orbital period of the outer edge of Ring A?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free