The orbital period of Jupiter is 4332.71 days.

2007or10's orbital period is 552.52 years

Haumea's orbital period is 283 or 103,468 days

The moon's orbital period is approximately 27.3 days.

Ganymede's orbital period is approximately 7.2 Earth days.

the orbital period of Saturn in earth years are 89years

Orbital period is the time it takes a planet to go around its star once.

A planet's orbital radius directly affects its orbital period through Kepler's third law of planetary motion. The farther a planet is from the star it orbits, the longer its orbital period will be, assuming all other factors remain constant. This relationship is expressed mathematically as T^2 ∝ r^3, where T is the orbital period and r is the orbital radius.

A planet's orbital period is also known as its year.

what is the term used for the orbital period of an object with respect to the stars?

Mars has an orbital period of approximately 687 Earth days.

Orbital speed = (circumference of the orbit) / (period of revolution)

Quaoar has an orbital period of about 285 years. It takes approximately 285 Earth years for Quaoar to complete one orbit around the Sun.

The orbital period of Deimos, one of Mars' moons, is approximately 30.3 hours.

The orbital period of Mars is approximately 687 Earth days, or about 1.88 Earth years.

The distance of a planet from the sun affects its orbital period. Generally, the farther a planet is from the sun, the longer its orbital period will be. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun.

27.3 days around the earth.

A planet's orbital period is related to its distance from the Sun by Kepler's third law, which states that the square of the orbital period is proportional to the cube of the semi-major axis of the orbit. For an orbital period of 3 million years, the planet would need to be located at a distance of approximately 367 AU from the Sun.

The year.

Mercury

The allowed orbital types for the second period of the periodic table are s and p orbitals. This means that elements in the second period can have a maximum of 2 electrons in an s orbital and 6 electrons in p orbitals.

Uranus has an orbital period of about 84 Earth years, or approximately 30,687 Earth days. It takes Uranus this long to complete one orbit around the sun.

The orbital period of Mars is equal to about 1.88 Earth years.

Neptune has 13 known moons and an orbital period of about 60190 Earth days.

Saturn's rotation period is about 10.7 hours, while its orbital period around the Sun is approximately 29.5 Earth years.

To calculate the orbital period of a planet, you can use Kepler's third law of planetary motion. The formula is T2 (42 r3) / (G M), where T is the orbital period, r is the average distance from the planet to the sun, G is the gravitational constant, and M is the mass of the sun. Simply plug in the values for r and M to find the orbital period of the planet.

To determine the energy level of the f-orbital in a particular period, consider the principal quantum number (n) of the period. The energy level of the f-orbital follows the pattern 4n, where n is the principal quantum number. This means that for each period, the energy level of the f-orbital will be 4 times the principal quantum number of that period.

The orbital period of a planet can be calculated using Kepler's third law: P^2 = a^3 where P is the orbital period in years and a is the semi-major axis in astronomical units. For a planet with an average distance of 10 au, its orbital period would be approximately 31.6 years.

75 years

687 earth days

Makemake's orbital period is about 309 Earth years. It takes Makemake nearly 310 years to orbit the sun once due to its distance from the sun and slower speed compared to inner planets.

The orbital period of the planet Mercury around the sun is approximately 88 Earth days. Mercury has a relatively short orbital period due to its proximity to the sun, which causes it to move quickly in its orbit.

From a star's orbital period, we can infer its distance from the object it is orbiting (based on Kepler's third law), the system's total mass (by combining other observable parameters), and potentially the star's luminosity and size if additional information is available. The orbital period can also give insights into the stability of the system and the potential presence of other planets or companions.

The last element in any period always has its outermost electron in the same type of atomic orbital, either an s or p orbital.

Not at all. The only thing that sets the orbital period is the semimajor axis, which is the average of the maximum and minimum distances from the Sun.

The first period of the periodic table can hold a maximum of 2 electrons, which are filled in the s orbital. There are no p orbitals in the first period, which is why there are no p-block elements in the first period. The p-orbital becomes available in the second period.

The orbital period of Jupiter is about 11.9 Earth years. This means it takes Jupiter approximately 11.9 Earth years to complete one orbit around the Sun.

it is 247 days of rotationalism

4 years 220 days

164 years

Triton, the largest moon of Neptune, has an orbital period of about 5.9 Earth days. It orbits Neptune in a retrograde direction, meaning it moves in the opposite direction of the planet's rotation. This unique orbital motion is thought to be the result of Triton being a captured object from the Kuiper Belt.

Mercury is the closest planet to the Sun and has an orbital period of 88 Earth days. (Pluto in contrast has an orbital period of about 248 Earth years.)

Venus.

Mercury = 66 days

Mars = 1.86 years.

686.980 earth days, sidereal period; 779.94 earth days, synodic period.

Comets are classified based on the length of their orbital period and their origin. Short-period comets have orbital periods less than 200 years, while long-period comets have longer orbital periods. Comets can also be classified based on their composition and physical characteristics, such as size and brightness.

Orbital information. You need to know the size of the "semi-major axis". Then you can calculate the orbital period, using Kepler's Third Law.

Yes, spot on, good guess . .

Triton's revolution period is the same as its orbital period, or approximately 5.877 days.

Mars has an orbital period of very approximately twice that of the earth