Skip to main content
Commonmark migration
Source Link

##What are the requirements for a planet to orbit around the sun at twice the Earth's rate?

What are the requirements for a planet to orbit around the sun at twice the Earth's rate?

##Would it rotate at twice the rate?

Would it rotate at twice the rate?

##Would a planet that close to the sun be habitable?

Would a planet that close to the sun be habitable?

##Would a planet rotating that quickly be habitable?

Would a planet rotating that quickly be habitable?

##What are the requirements for a planet to orbit around the sun at twice the Earth's rate?

##Would it rotate at twice the rate?

##Would a planet that close to the sun be habitable?

##Would a planet rotating that quickly be habitable?

What are the requirements for a planet to orbit around the sun at twice the Earth's rate?

Would it rotate at twice the rate?

Would a planet that close to the sun be habitable?

Would a planet rotating that quickly be habitable?

added 14 characters in body
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14

While the rate of a planet's revolution is determined by its proximity to the star, its rate of rotation is almost entirely arbitrary. Tidal force between two bodies acting over a sufficiently long period of time can cause tidal locking, although no known planets are synchronously tidally locked with their star.

While the rate of a planet's revolution is determined by its proximity to the star, its rate of rotation is almost entirely arbitrary. Tidal force between two bodies acting over a sufficiently long period of time can cause tidal locking, although no known planets are tidally locked with their star.

While the rate of a planet's revolution is determined by its proximity to the star, its rate of rotation is almost entirely arbitrary. Tidal force between two bodies acting over a sufficiently long period of time can cause tidal locking, although no known planets are synchronously tidally locked with their star.

added 5 characters in body
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14

In fact, in 1609, based on new measurements of our own solar system, Johannes Kepler figured out some general rules. Kepler's third law of planetary motion states that the cube of a planet's semi-major axis (that is, the distance from the sun) is proportional to the square of its orbital period (year). So to get a body to orbit twice as quickly requires requires it to be about a hirdthird closer: I calculate that for a planet to revolve every 180 days you'd want it to be about 0.62 AU from the sun.

In fact, in 1609, based on new measurements of our own solar system, Johannes Kepler figured out some general rules. Kepler's third law of planetary motion states that the cube of a planet's semi-major axis (that is, the distance from the sun) is proportional to the square of its orbital period (year). So to get a body to orbit twice as quickly requires it to be about a hird closer: I calculate that for a planet to revolve every 180 days you'd want it to be 0.62 AU from the sun.

In fact, in 1609, based on new measurements of our own solar system, Johannes Kepler figured out some general rules. Kepler's third law of planetary motion states that the cube of a planet's semi-major axis (that is, the distance from the sun) is proportional to the square of its orbital period (year). So to get a body to orbit twice as quickly requires it to be about a third closer: I calculate that for a planet to revolve every 180 days you'd want it to be about 0.62 AU from the sun.

Radius vs diameter error; integrade later revisions better; etc.
Source Link
JDługosz
  • 69.8k
  • 13
  • 131
  • 313
Loading
added 7 characters in body
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14
Loading
Post Undeleted by Thriggle
Realized I misunderstood the premise of the question... thought "half the orbit" meant "half the orbital distance"
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14
Loading
Post Deleted by Thriggle
Added correction from comments.
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14
Loading
phraseology
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14
Loading
added 170 characters in body
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14
Loading
Source Link
Thriggle
  • 2.6k
  • 1
  • 13
  • 14
Loading