Yes. T = (2pi / sqroot of GM) multiplied by the radius^3/2.
A planets mass DOES NOT affect its orbital period.
A planets radius DOES affect its orbital period.
a planet's orbital period. based off kepler's 3rd law (Wrong.)The planet's orbital radius. (Correct.)
An orbit is the path followed by a planet according to Kepler's laws, which are very accurate but not exact. Size, speed and period are all related by simple formulas so that if you know one you can find out the other two. The orbit is an ellipse and the size is usually measured by its mean radius, also called its semi-major axis, which is the average of the maximum and minimum distances. For the Earth that is 149.6 million kilometres. The orbital period is proportional to the mean radius to the power 1.5, while the orbital speed is inversely proportional to the square root of the mean radius.
ecliptic but its really a plane orbital radius
Look in related links, "Planetary Attributes on Wikipedia". The column "Orbital Radius" shows the distance from the Sun, in AU. If you want that in kilometers, multiply the number of AUs by 150 million.
Jupiter's orbit is an ellipse with an eccentricity of 0.048, which means that it looks like a circle with the Sun off-centre by an amount equal to 0.048 times the average radius. Uranus has an eccentricity of 0.047 and that is the closest among the other planets.
pluto
yeet
a planet's orbital period. based off kepler's 3rd law (Wrong.)The planet's orbital radius. (Correct.)
Yes, spot on, good guess . .
charge, atomic radius, orbital penetration, and electron pairing.
5.2 Earth yearsExplanation: Kepler's third law, shown below, relates a planet's orbital period to its orbital radius. T is the planet's orbital period and r is its orbital radius. k is a constant that depends upon the mass of the star at the center of the solar system.soT2 = kr3When AU are used in our solar system, k is 1. To solve, cube the orbital radius, so 33 is 27. Then take the square root of the result. The square root of 27 is close to 5.2, so the period of a typical asteroid is close to 5.2 Earth years.
An orbit is the path followed by a planet according to Kepler's laws, which are very accurate but not exact. Size, speed and period are all related by simple formulas so that if you know one you can find out the other two. The orbit is an ellipse and the size is usually measured by its mean radius, also called its semi-major axis, which is the average of the maximum and minimum distances. For the Earth that is 149.6 million kilometres. The orbital period is proportional to the mean radius to the power 1.5, while the orbital speed is inversely proportional to the square root of the mean radius.
It doesn't orbit earth faster. The ISS is in a lower orbit with a period of 91 minutes compared to the Hubble's orbital period of 96-97 minutes. Orbital periods generally increase with orbit radius and speed in the orbit decreases with increasing orbit radius.
They have the smallest nuclear charge of that period so there is less attraction for the electron allowing a larger orbital radius (larger size).
19.2 rE
The atomic radius gets smaller the farther right it appears on the Periodic Table, until the addition of a new orbital increases the size again.
The atomic radius gets smaller the farther right it appears on the Periodic Table, until the addition of a new orbital increases the size again.