Hot Jupiters may have migrated close to their stars due to interactions with the protoplanetary disk during their formation, gravitational interactions with other planets, or tidal forces from the star.
The semi-major axis of an orbit is calculated as the average distance between the center of the orbit and the farthest point of the orbit. It can be found by taking the average of the closest and farthest distances from the center of the orbit.
"orbit"
The eccentricity of a planet's orbit can be calculated using the formula e c/a, where c is the distance between the center of the orbit and the focus, and a is the length of the semi-major axis of the orbit.
To calculate the mass of an object in orbit, we can use the period and radius of its orbit by applying Newton's version of Kepler's third law. This formula states that the square of the period of an orbit is proportional to the cube of the semi-major axis of the orbit. By rearranging this formula and plugging in the known values of the period and radius, we can solve for the mass of the object.
The mass of a satellite does not affect its orbit. The orbit of a satellite is determined by its speed and the gravitational pull of the object it is orbiting around, such as a planet. The mass of the satellite itself does not play a significant role in determining its orbit.
Jupiters orbit is between Mars and Saturn's orbit. Jupiters orbit can also be said to be within the orbits of Saturn, Uranus and Neptune.
13.06km/s
Jupiters orbit is a imaginary circle that the planets circle around that is how we count years.
Astronomers explain the orbit of hot Jupiters, gas giant exoplanets located close to their stars, through theories of planetary migration. These planets likely formed further from their stars and later migrated inward due to gravitational interactions with the protoplanetary disk or through interactions with other bodies. Tidal forces and the dissipative processes in the disk can also help circularize their orbits. Additionally, some hot Jupiters may have formed in situ through rapid gas accretion in their current locations.
It can't because planet Nibru isn't real.
the shape of earth's orbit around the sun
Many newly detected extrasolar planets are called hot Jupiters because they are large, gaseous planets with characteristics similar to Jupiter, but they orbit very close to their host star. This proximity to their star causes them to have high surface temperatures, hence the term "hot."
Hot Jupiters are giant gas planets that orbit very close to their stars. They are believed to have migrated inward from their original formation locations due to interactions with the protoplanetary disk or other planets in the system. This migration process could have been caused by gravitational interactions or tidal forces, leading to their current close proximity to their stars.
Jupiters orbit is a imaginary circle that the planets circle around that is how we count years.
None. Jupiters year lasts about 11 years and Saturn about 29.
You might contrast objects in open orbit with those in closed orbit such as the Earth. Up to an approximation, and relative to the Sun, when the Earth completes an orbit around the Sun it returns to the same place in space. Thus it can be said to 'close' its orbit. Objects that do not return to the same point in space are said to be in open orbit. They might be following parabolic or hyperbolic paths, or some other more complicated locuses of points.
Hot Jupiters were among the earliest known exoplanets discovered because they are large gas giants that orbit very close to their parent stars, making them easier to detect using early planet-hunting techniques.