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Item: Astrophysics ->Category: Science -> Author: DF -> Revision: 07/10/2008
Carbon cycle


Cycle reactions by which the nitrogen nuclei become thanks to the helium isotopes of carbon, nitrogen and oxygen. It is the method of generating energy from some stars.



Complete Glossary of astrophysics

A

Abell
Aberration
Abside
Absolute magnitude
Accelerating Fermi
Acrecion
Active galaxy
Afelio
Agglomeration
Agglomeration globular
Albedo
Almagest
Angstrom
Anion
Annihilation
Anomaly gravitational
Antilepton
Antileptoquark
Antimateria
Antiparticula
Antiproton
Antiquark
Apoapsis
Apogee
Apparent magnitude
Asteroid
Astronomical unit
Atmosphere
Atomo
Attendance gravitational
Aureola galactic
Aurora
Axion
Axis

C

Campo
Carbon cycle
Casquetes polar
Cationic
CCD
Cefeida
Celestial sphere
Centrifugal force
Chain perseo piscis
Color
Color index
Cometa
Concealment
Conjunction
Constellation
Convection
Coordinates heavenly
Corona
Corpusculo planetarium
Cosmic rays
Cosmos
Cromosfera
Cuark
Cuasar
Cumulation of galaxies
Cumulation of stars

E

Eclipse
Ecliptica
Eddington limit
Electromagnetic radiation
Electron
Electronvoltio
Epiciclo
Ergoesfera
Espin
Ether
Event horizon
Exiton
Explosion radio
Extragalactico

G

Gal
Galaxy
Gamma rays
Ganymede
Gas
Giant
Giant blue
Gluon
Graviton

I

Inclination
Inflationary Universe
Infrared
Intergalactic medium
Interstellar absorption
Interstellar dust
Interstellar medium
Intragalactico
Ion
Ionisation
Ionosphere
Isofotas
Isotope

L

Law of gravity
Layer clash
Lemb
Lepton
Leptoquark
Light year
Limit Roche
Line emission
Luminosity

N

Nanometro
Nebula
Neutrino
Neutron
Neutron star
Nova
Nova fast
Nova slow
Nuclear fusion

P

Parallax stellar
Parsec
Particle
Pastors moons
Periapsis
Periastro
Perigee
Perihelio
Phase
Plage
Planck Era
Planet
Plasma
Polar cap
Polarization
Positron
Potential energy
Preones
Process triple alfa
Protoestrella
Protogalaxia
Proton
Protosol
Push

R

Radial velocity
Radiation
Radiation belt
Radiation synchtron
Radio lobe
Radioactive transport
Radiofuente double
Radiogalaxia
Radioondas
Recession
Red dwarf
Red Giant
Reflection
Refractive
Regolito
Relativity
Relaxation violent
Revolution
Roche lobe
Ropes flow
Rotation
Rupes

T

Taquion
Tau
Tecnecio
Theory of relativity
Tholus
Tidal force
Tide
Tilt galaxy
Transitional phase
Tritium
Troposphere

V

Vacuum
Van Allen belt
Variable
Variable cefeida
Variable elliptic
Visible light
Visual magnitude

B

Baricentro
Barion
Basalt
Big Bang
Binary star
Binary system
Bipolar flow
Black body
Black dwarf
Black hole
Boson
Bremsstrahlung
Brightness
Brown dwarf
Button

D

Dark matter
Day apparent
Deceleration radioactive
Decomposition
Deferente
Degeneration
Density
Deterioration orbital
Deuterium
Device Charging Acoplada
Deyeccion
Diagram Hertzsprung Russell
Diameter angle
Disk
Disk accretion
Dwarf
Dynamic friction

F

Facula
False vacuum
Fermion
Filamento
Fluid modeling
Flute
Fonon
Force of gravity
Foton
Fotosfera

H

H I region
H II region
Halo
Heliosfera
House bubble
Hubble Constant

J

Jets

M

Magellanic stream
Magnetic field
Magnetocola
Magnetopausa
Magnetosfera
Magnitude
Magnitude B
Magnitude blue
Magnitude yellow
Mantle
Mare
Megaton
Meteor
Meteroide
Microwave
Miligal
Milky Way
Molecule
Moon
Movement itself
Moving toward the blue
Moving toward the red
Muon

O

Onda
Oort cloud
Orbit

Q

Quantum mechanics
Quark
Quasar

S

Satellite
Second arc
Severity
Shock wave
Sidereal day
Size angle
Solar system
Solar wind
Spectral line
Spectrum
Speed exhaust
Speed of light
Spiral Arm
Star fleeting
Star in astrophysic
Stellar association
Stellar population
Stellar wind
Subduccion
Sublimation
Sun Spots
Supercampos
Supercumulos
Supergigante
Supernova
Supernova type I
Supernova type II

U

UA
Ultraivoleta
Ultraviolet light
Umbra
Uniqueness
Unit light standard
Universe

W

Wave of curvature
Wave of hertzian
Wave radio
Wavelength
Weak force
White dwarf
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