More than one, Jupiter has the red stop (a constant storm) and Saturn has a blueish spot (Hubble AKA space camera took pic of it) has raging storms
Gravity on a planet varies because it depends upon mass and distance. Mass is proportional to gravity is and every planet have different sizes and masses.F = G(mass1*mass2)/D squared.(G is the gravitational constant, which has the same value throughout our universe.)
You can use the formula M = (V^2 * R) / G, where M is the planet's mass, V is the orbital speed, R is the distance from the sun, and G is the gravitational constant. By plugging in the values of V and R, you can calculate the planet's mass.
Force of gravity equals mass of planet times mass of other times the constant (G) that makes the units work all divided by the distance from one to the other AND the other to one (turns out to be distance squared). F=GxM1xM2/(DxD)
The mass of an astronaut would remain constant, so it would be 80 kg regardless of the planet they are on. Weight, on the other hand, is the force due to gravity acting on the mass of the astronaut, so it would vary depending on the gravitational pull of the planet.
as mass is the quantity of matter contained in a body
Gravity on a planet varies because it depends upon mass and distance. Mass is proportional to gravity is and every planet have different sizes and masses.F = G(mass1*mass2)/D squared.(G is the gravitational constant, which has the same value throughout our universe.)
The weight of an object on the surface of a planet with radius r is determined by the planet's mass and the object's distance from the planet's center. The weight can be calculated using the formula W (G M m) / r2, where W is the weight, G is the gravitational constant, M is the planet's mass, m is the object's mass, and r is the radius of the planet.
The angular momentum of a planet remains constant in its motion around the sun. This is due to the conservation of angular momentum, which dictates that the product of the planet's mass, velocity, and distance from the sun remains the same as the planet orbits.
That is answerd by Newton's law of gravity:F = G M1M2/ R2F is the force, your weight, M1 is your mass, M2 is the planet's mass, and R is the radius of the planet. G is the universal gravitational constant.
Yes, the storm on Saturn, known as the hexagonal storm, has been observed for decades. It is a persistent feature in Saturn's atmosphere, located at its north pole. The storm's hexagonal shape is thought to be caused by the planet's jet stream patterns.
You can use the formula M = (V^2 * R) / G, where M is the planet's mass, V is the orbital speed, R is the distance from the sun, and G is the gravitational constant. By plugging in the values of V and R, you can calculate the planet's mass.
An object with twice the mass of another will weigh twice as much when both objects are on the same planet or celestial body with a constant gravitational acceleration. Weight is directly proportional to mass when the gravitational acceleration remains constant.
Mass(m) is the product of the gravitational pull, which is constant (g), of the planet or the largest heavenly body nearest to the object to be weighed and it's weight(w). Hence, gravitational constant(g) is the ratio between the MASS of an object and the Weight of the object. While the mass of an object is constant anywhere in the universe, the weight depends on the value of the gravitational constant. Thus, a 1 lb-mass of an object in earth will have the same mass of 1 lb-mass in the moon though they will weigh differently.Mass is measured in kilograms, hectograms , decagrams , grams , decigrams ,centigrams , milligrams.
Your mass will remain the same regardless of the planet you are on. Mass is a measure of the amount of matter in an object, while weight is the force of gravity acting on that mass. So, your weight will change on a different planet due to differences in gravitational pull, but your mass will stay constant.
Force of gravity equals mass of planet times mass of other times the constant (G) that makes the units work all divided by the distance from one to the other AND the other to one (turns out to be distance squared). F=GxM1xM2/(DxD)
Force of gravity equals mass of planet times mass of other times the constant (G) that makes the units work all divided by the distance from one to the other AND the other to one (turns out to be distance squared). F=GxM1xM2/(DxD)
Force of gravity equals mass of planet times mass of other times the constant (G) that makes the units work all divided by the distance from one to the other AND the other to one (turns out to be distance squared). F=GxM1xM2/(DxD)