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Astronomy PhotometryPhotosphere

Photon Belt
The photon belt is reportedly a band of intense photon light that is near Earth at this time.

 


Photon
A name for the discrete particles of pure energy that represent light, or electromagnetic radiation.
Photons have an energy E associated with their frequency f of oscillation such that: ...

Photon
Photons emitted in a coherent beam from a laser
Composition: ...

Photons :
Photons, also called light quantum, are minute energy packets of electromagnetic radiation.

Photons are often loosely associated to light, to which they relate only for a very narrow frequency window of the spectrum.

A photon is emitted when an atom dumps some of its energy. An excited atom, one in a high energy state, has an electron in a higher energy orbit than normal.

Definition: photon: The smallest (quantum) unit of light/electromagnetic energy. Photons are generally regarded as particles with zero mass and no electric charge.
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Photon
Wikipedia, the free encyclopedia - Cite This Source
In physics, the photon is the elementary particle responsible for electromagnetic phenomena.

Photons
Waves and particles seem to be diametrically opposed concepts: a wave fills a region in space, while an electron or ion has a well-defined location. That, at least, was the view before the discoveries of the first half of the 20th century.

Single Photon Calorimeters
Perhaps the most intriguing advance in X-ray astronomy instrumentation in the 1990s has been the development of single photon calorimeters, spearheaded by work at NASA's Goddard Space Flight Center.

Photon
A particle with energy equal to a single quanta. The energy of the particle is proportional to frequency. Electromagnetic energy may sometimes be considered to be wave-like, and at other times, particle-like.

Photon Pile-up →
Spin the Galex telescope to collect three photons of the same color.
Oceans of Climate Change Video → ...

photon Individual packet of electromagnetic energy that makes up electromagnetic radiation.
photosphere The visible surface of the Sun, lying just above the uppermost layer of the Sun's interior, and just below the chromosphere.

photons--A form of electromagnetic radiation, such as visible light or radio waves
photosphere--The layer of the Sun above the convective zone where light is emitted ...

PHOTON ORBITS
An alternative way of seeing the significance of the Schwarzschild radius is to consider what happens to rays of light emitted at different distances from the event horizon of a black hole.

PHOTON - Discrete bundle of light energy. Light of a given energy (frequency) cannot be broken up indefinitely. Rather for a given frequency it comes in discrete bundles with energy (h = Planck's constant and ν= frequency): ...

Photon: A discrete packet of electromagnetic energy.
Planetary Nebula: The gaseous outer layers of a star that have been ejected into space as the star collapses into a white dwarf.

Photon
(a) Smallest packet of the electromagnetic force field; messenger particle of the electromagnetic force; smallest bundle of light.
(b) The quantum of the electromagnetic field. It is the massless spin-1 gauge boson of QED.

photon
A component of light which is considered a particle with zero mass.
photosphere
The surface of the Sun.

Photon Noise Limited - An image is photon-noise limited when the exposure is of sufficient length so that photon noise is the major source of noise in the image instead of read-out noise.

Photon
A quantum of electromagnetic energy Carries an amount of energy that depends inversely on its wavelength
Photosphere ...

Photon
a discrete quantity of electromagnetic energy. Short wavelength (high frequency) photons carry more energy than long wavelength (low frequency) photons.

Photon. The smallest unit of light.
Photosphere. The bright visible surface of the Sun.

Photonic crystals are periodic optical nanostructures that are designed to affect the motion of photons in a similar way that periodicity of a semiconductor crystal affects the motion of electrons....
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Photon - A massless particle of electromagnetic energy
Photosphere - The visible region of the atmosphere of the Sun or another star ...

Photon- a quantum of light
Photosphere- the visible surface of the sun or a star
Plage- bright regions seen in the solar chromosphere ...

Photons have no mass, and travel at the speed of light c, about 300,000 km/sec or 186,000 miles/sec.

Photon A unit or "particle" of electromagnetic energy, or light.
Photosphere The visible surface of the Sun. Above it are the chromosphere, then the corona.
Physics The science dealing with matter and energy and their interaction.

Photon
A packet of electromagnetic energy, such as light. A photon is regarded as a charge-less, mass-less particle having an indefinitely long lifetime.
Photosphere ...

PHOTON
A photon is a quantum of electromagnetic energy. For example, light is composed of light.
PHOTOSPHERE
The photosphere is the layer of the which is visible to us. It consists of a and has a temperature of about 10,800°F (6,000°C).

photon - (n.)
A packet of energy that can be thought of as a particle of light travelling at the speed of light.

Photon
A particle of light composed of a minute quantity of electromagnetic energy.
Photosphere
The bright visible surface of the Sun.

Photon: Experiments have shown that light of a given energy (frequency) is not something that can be broken up indefinitely. Rather for a given frequency it comes in discrete bundles with energy hf where h is Planck's constant and f is the frequency.

- Photon - What is a photon?
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A photon of light provides the energy that an electron needs to climb up a level. If the photon comes close enough to an atom, it can be absorbed by the atom, pushing the electron up (see diagram below).

As photons are absorbed by the outer portion of the Sun, the temperature gradient increases and convection occurs. Great currents of hot plasma, or ionized gas, carry heat upward.

The photons from the microwave background have been travelling nearly the age of the universe to reach us right now.

(a) Photons of wavelengths between about 0.1 Å and 100 Å - more energetic than ultraviolet, but less energetic than -rays. [H76]
(b) A large band of electromagnetic radiation with wavelengths smaller than extreme ultraviolet light.

Energy of a photon - There are two versions of this formula, one using the frequency, the other using the wavelength. The basic upshot is that as frequency goes up, so does energy, however wavelength goes down.

Wavebands - Photons from Space
Electromagnetic Spectrum
Atmospheric Windows
Why Observe at Different Wavebands?
Further Information
Questions ...

4 1H - 4He + photons + others
It requires extreme conditions to start the nuclear fusion. Those conditions still cannot be stably reproduced in laboratory on Earth.

gamma photon = gamma ray. gamma radiation = gamma ray. gamma ray A quantum of electromagnetic radiation emitted by a nucleus, each such photon being emitted as the result of a quantum transition between two energy levels of the nucleus.

(See entry for gamma ray.) gamma photon (NASA SP-7, 1965) = gamma ray. gamma radiation (NASA SP-7, 1965) = gamma ray.

When ultraviolet photons strike particles moving at an appreciable fraction of the speed of light, the photons gain energy and become gamma rays.

A unit of energy used to describe the total energy carried by a particle or photon. The energy acquired by an electron when it accelerates through a potential difference of 1 volt in a vacuum. 1 eV = 1.6 x 10-12 erg.

How is wavelength related to photon energy?
How does the surface temperature of a reddish star compare with the surface temperature of a bluish-white star? Does the diameter of the star matter when determining the Temperature?

radiation Energy radiated in the form of waves or particles; photons. radiationbelt Regions of charged particles in a magnetosphere. red giant A star that has low surface temperature and a diameter that is large relative to the Sun. regio Region.

A key question must be answered from observation - what was the source of reionizing photons? One could imagine that either stars or active nuclei could provide the energy.

Einstein which demonstrates that light seems to be made up of particles, or photons. Light can excite electrons (called photoelectrons in this context) to be ejected from a metal.

Light, or electromagnetic radiation, can be thought of as coming in tiny packets of energy called photons. These photons come with a wide range of energies. At the low-energy end, we find radio waves. At the high-energy end, we find gamma-rays.

Photons in the Radioactive Zone (PDF, 602 KB): Participants model how photons leave the Sun.
Grade Level: 5-8
Teacher Guide (PDF, 602 KB) Student Activity (PDF, 147 KB) Student Text (PDF, 336 KB) ...

This frequency corresponds to the energy of the photon emitted when the nitrogen atom moves from one side to the other of the triangle formed by the three hydrogen atoms in an ammonia molecule.

When a photon (a particle of light) hits a capacitor, the photon dispaces some electrons, generating a small current - charging the capacitor. A CCD can detect light coming in at rates as low as one photon per minute.

When this decay occurs, the photon produced is not necessarily emitted in the same direction as the original photon. The most common angle of this has been shown to be about 45 degrees of the original photon.

At this temperature the photons split the iron nuclei into protons and neutrons, thereby undoing millions of years of nuclear synthesis in a fraction of a second.

" and I my answer was, "I've always wanted to see a photon torpedo go right through the ship. There's one place on the primary hull where it's really thin." We designed that shot and they accepted it.

The energy generated in the core is carried by light (photons) that bounces from particle to particle through the radiative zone.

Electromagnetic energy of all frequencies or energies can be viewed in physics as if it were waves, as described above, and also as particles, known as photons.

These particles of light are called photons. But light also exhibits the characteristics of a wave.

They are ionized by ultraviolet light from the hot central stars, which must be hotter than about 26,000 Kelvin to have sufficiently energetic photons to ionize the dominant hydrogen.

See also: Energy, Light, Time, Field, Universe