# Angular momentum and energy

**Angular momentum and energy** are concepts developed to try to understand everyday reality.

An angular momentum **L** of a particle about an origin is given by

where **r** is the radius vector of the particle relative to the origin, **p** is the linear momentum of the particle, and × denotes the cross product (r · p sin θ). Theta is the angle between **r** and **p**.

## Masses edit

**Def.** the "quantity of matter which a body contains, irrespective of its bulk or volume"^{[1]} or a "quantity of matter cohering together so as to make one body, or an aggregation of particles or things which collectively make one body or quantity"^{[2]} is called **mass**, or a **mass**.

Mass is an idea.

The smallest unit of mass appears to be an electron (or positron).

## Motions edit

**Def.** a property of a body that resists any change to its uniform motion is called **inertia**.

Mass and inertia are generally considered equivalent.

Isaac Newton's laws of motion contain the idea of inertia.

Newton's First law:
"Every body persists in its state of being at rest or of moving uniformly straight forward, except insofar as it is compelled to change its state by force impressed."^{[3]}

While motion in a straight line, or rectilinear motion can be produced over limited distances in a laboratory, it may not occur naturally.

When a body or particle is radiated it is given motion.

## Vectors edit

**Def.** the product of a body's mass and velocity is called **momentum**.

**Def.** the rotary inertia of a system [such as] an isolated rigid body is a measure of the extent to which an object will continue to rotate in the absence of an applied torque is called **angular momentum**.

## Energies edit

**Def.** a rotational or twisting effect of a force is called a **torque**.

**Def.** a turning effect of a force applied to a rotational system at a distance from the axis of rotation is called a **moment of force**.

The moment is equal to the magnitude of the force multiplied by the perpendicular distance between its line of action and the axis of rotation.

A torque and a moment of force are the same. Each is a "unit of work done, or energy expended.

For an object with a fixed mass that is rotating about a fixed symmetry axis, the angular momentum is expressed as the product of the moment of inertia of the object and its angular velocity vector:

where *I* is the moment of inertia of the object (in general, a tensor quantity), and **ω** is the angular velocity.

The moment of inertia is the mass property of a rigid body that defines the torque needed for a desired angular acceleration about an axis of rotation. Moment of inertia depends on the shape of the body and may be different around different axes of rotation. A larger moment of inertia around a given axis requires more torque to increase the rotation, or to stop the rotation, of a body about that axis. Moment of inertia depends on the amount and distribution of its mass, and can be found through the sum of moments of inertia of the masses making up the whole object, under the same conditions.

In two dimensions the angular velocity *ω* is given by

This is related to the cross-radial (tangential) velocity by:^{[4]}

An explicit formula for **v**_{⊥} in terms of **v** and *θ* is:

"Combining the above equations gives a formula for *ω*:

## Problem 1 edit

Using the following values, and considering the Sun to be a rigid, solid object, answer the questions below. and

What is the angular velocity of the Sun?

What is its moment of inertia?

What is the Sun's angular momentum?

Estimate how much torque is necessary to bring the Sun's rotational velocity down to zero?

What are the units of angular momentum for the Sun?

## Problem 2 edit

Using the following values, and considering Jupiter to be a rigid, solid object, answer the questions below. and

What is the angular velocity of the Jupiter?

What is its moment of inertia?

What is the Jupiter's angular momentum from rotation?

Estimate how much torque is necessary to bring the Jupiter's rotational velocity down to zero?

Using a mean orbital radius between 8.16 x 10^{8} km and 7.41 x 10^{8} km, what's its angular momentum from revolution around the Sun?

Is the total angular momentum of Jupiter greater than the Sun's?

## Problem 3 edit

Using the following values, and considering Saturn to be a rigid, solid object, answer the questions below. and

What is the angular velocity of the Saturn?

What is its moment of inertia?

What is the Saturn's angular momentum from rotation?

Estimate how much torque is necessary to bring the Saturn's rotational velocity down to zero?

Using a mean orbital radius between 1.51 x 10^{9} km and 1.35 x 10^{9} km, what's its angular momentum from revolution around the Sun?

Is the total angular momentum of Saturn greater than the Sun's?

## Problem 4 edit

Using the following values, and considering Uranus to be a rigid, solid object, answer the questions below. and

What is the angular velocity of the Uranus?

What is its moment of inertia?

What is the Uranus's angular momentum from rotation?

Estimate how much torque is necessary to bring the Uranus's rotational velocity down to zero?

Using a mean orbital radius between 3.00 x 10^{9} km and 2.75 x 10^{9} km, what's its angular momentum from revolution around the Sun?

Is the total angular momentum of Uranus greater than the Sun's?

## Problem 5 edit

Using the following values, and considering Neptune to be a rigid, solid object, answer the questions below. and

What is the angular velocity of the Neptune?

What is its moment of inertia?

What is the Neptune's angular momentum from rotation?

Estimate how much torque is necessary to bring the Neptune's rotational velocity down to zero?

Using a mean orbital radius between 4.55 x 10^{10} km and 4.45 x 10^{10} km, what's its angular momentum from revolution around the Sun?

Is the total angular momentum of Neptune greater than the Sun's?

## Hypotheses edit

- To use angular momentum or energy a mass must be assigned.

## See also edit

- Column densities
- Cosmic circuits
- Energy phantoms
- Furlongs per fortnight
- Planck's equation
- Radiation astronomy/Problem set
- Radiation dosage
- Radiation astromathematics problems
- Spectrographs
- Star jumping
- Synchrotron radiation
- Telescopes and cameras
- Unknown coordinate systems
- Unusual units
- Vectors and coordinates

## References edit

- ↑ Eclecticology (12 September 2003).
*mass*. San Francisco, California: Wikimedia Foundation, Inc. http://en.wiktionary.org/wiki/mass. Retrieved 2013-08-12. - ↑ Emperorbma (14 November 2003).
*mass*. San Francisco, California: Wikimedia Foundation, Inc. https://en.wiktionary.org/wiki/mass. Retrieved 2014-02-28. - ↑ Isaac Newton,
*The Principia*, A new translation by I.B. Cohen and A. Whitman, University of California press, Berkeley 1999. - ↑ Russell C. Hibbeler (2009).
*Engineering Mechanics*. Upper Saddle River, New Jersey: Pearson Prentice Hall. pp. 314, 153. ISBN 978-0-13-607791-6. http://books.google.com/?id=tOFRjXB-XvMC&pg=PA314.

## External links edit

- International Astronomical Union
- NASA/IPAC Extragalactic Database - NED
- NASA's National Space Science Data Center
- NCBI All Databases Search
- Office of Scientific & Technical Information
- The SAO/NASA Astrophysics Data System
- Scirus for scientific information only advanced search
- SDSS Quick Look tool: SkyServer
- SIMBAD Astronomical Database
- SIMBAD Web interface, Harvard alternate
- Spacecraft Query at NASA
- Universal coordinate converter

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