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Saturn has an intrinsic magnetic field that has a simple, symmetric shape—a magnetic dipole. Its strength at the equator—0.2 gauss (20 μT)—is approximately one twentieth of that of the field around Jupiter and slightly weaker than Earth's magnetic field. [32] As a result, Saturn's magnetosphere is much smaller than Jupiter's. [82]
In classical mechanics, a gravitational field is a physical quantity. [5] A gravitational field can be defined using Newton's law of universal gravitation. Determined in this way, the gravitational field g around a single particle of mass M is a vector field consisting at every point of a vector pointing directly towards the particle. The ...
Gravimetry is the measurement of the strength of a gravitational field. Gravimetry may be used when either the magnitude of a gravitational field or the properties of matter responsible for its creation are of interest. The study of gravity changes belongs to geodynamics.
Vector field (blue) and its associated scalar potential field (red). Point P between earth and moon is the point of equilibrium. In physics, a gravitational field or gravitational acceleration field is a vector field used to explain the influences that a body extends into the space around itself. [6]
This formulation is dependent on the objects causing the field. The field has units of acceleration; in SI, this is m/s 2. Gravitational fields are also conservative; that is, the work done by gravity from one position to another is path-independent. This has the consequence that there exists a gravitational potential field V(r) such that
At the Earth's surface, an object whose mass is exactly one kilogram weighs approximately 9.81 newtons, the product of its mass and the gravitational field strength there. The object's weight is less on Mars , where gravity is weaker; more on Saturn , where gravity is stronger; and very small in space, far from significant sources of gravity ...
The tidal force experienced by objects subject to the gravitational field of a galaxy such as the Milky Way. galactocentric distance A star or cluster's distance from the gravitational center of a particular galaxy. For example, the Sun is about 27,000 light-years (approximately 8 kiloparsecs) away from the Galactic Center of the Milky Way. [13]
Gravitational attraction of the proton and the electron in hydrogen atom [1] 10 −30 quectonewton (qN) 8.9 qN Weight of an electron [1] 10 −26: 16 rN Weight of a hydrogen atom [1] 10 −24 yoctonewton (yN) 5 yN Force necessary to synchronize the motion of a single trapped ion with an external signal measured in a 2010 experiment [2] [3] 10 ...