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What is the period of a planet?
The period of a planet is the time it takes for the planet to complete one orbit around its parent star. This period is typically measured in Earth days or years, depending on the length of the planet's orbit.
How long would it take light from the sun to reach planet earth?
approximately 8.33seconds
How did newton's work on orbit add to the work Kepler had done?
Kepler made discoveries regarding the planet's distance from the sun and how long it takes a planet to orbit the sun. In Newton's Version of Kepler's Third Law, Newton expands on these ideas by using his Theory of Gravity.
What planet has a year 248 earth years long?
The dwarf planet Pluto is the planet with a year 248 earth years long.
What planet has a year 280 earth years long?
The dwarf planet Haumea is the planet with a year 280 earth years long.
What planet has a year 310 earth years long?
The dwarf planet Makemake is the planet with a year 310 earth years long.
How long does it take a beam of light to reach planet earth from your nearest star?
It takes approx. 8 and half minutes to reach earth
How long does it take to get to a planet from Earth?
It depends which planet you mean.
Did Kepler go to the mars?
No. Johannes Kepler lived long before we had space travel. The Kepler telescope orbits the sun and was not designed to go to other planets.
How long is planet earth?
1000 feet
A calculation of how long it takes a planet to orbit the Sun would be most closely related to which Kepler's Law?
Kepler's 3rd law of planetary motion. It states that the square of a planets orbital period is proportional to the cube of a planets distance from a star.In mathematical notationTO2 = k*R03WhereTO = It's orbital periodRO = It's distance from the stark = A constant.
Is the shadow of the moon always long enough to reach the Earth?
No, the shadow of the moon is not always long enough to reach the Earth. During a solar eclipse, the moon's shadow on Earth is limited to a specific region where the alignment of the sun, moon, and Earth allows for the shadow to be cast on the Earth's surface.
