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galactic$30671$ - vertaling naar grieks

UNIT OF TIME
Galactic time; Galactic Year; Galactic orbit; Galactic Orbit; Galactic years
  • The orientation of the Solar System's motion

galactic      
adj. γαλακτικός, γαλαξία, γαλαξιακός
cosmic radiation         
  • air shower]].
  • Left image:Cosmic ray muon passing through a cloud chamber undergoes scattering by a small angle in the middle metal plate and leaves the chamber.Right image: Cosmic ray muon losing considerable energy after passing through the plate as indicated by the increased curvature of the track in a magnetic field.
  • Increase of ionization with altitude as measured by Hess in 1912 (left) and by Kolhörster (right)
  • Hess lands after his balloon flight in 1912.
  • Sources of ionizing radiation in interplanetary space.
  • access-date=31 May 2013}}</ref>
  • 160px
  • Shock front acceleration (theoretical model for supernovae and active galactic nuclei): Incident proton gets accelerated between two shock fronts up to energies of the high-energy component of cosmic rays.
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  • The [[VERITAS]] array of air Cherenkov telescopes.
HIGH-SPEED, I.E. HIGH-ENERGY PARTICLE, MAINLY ORIGINATING IN OUTER SPACE, OUTSIDE THE SOLAR SYSTEM
Galactic cosmic ray; Cosmic radiation; Cosmic-ray; Cosmic Ray; Anomalous cosmic ray; Cosmic Rays; Galactic cosmic rays; Auger shower; Cosmoclimatology; Galatic cosmic rays; Extensive shower; Cosmic-ray mesons; Cosmic-ray detector; Cosmic-rays; Cosmic rays; Galactic cosmic radiation; Cosmic particle; Origins of cosmic rays; Origin of cosmic rays; Primary cosmic rays; Primary cosmic ray; Secondary cosmic rays; Astroparticle
κοσμική ακτινοβολία
cosmic rays         
  • air shower]].
  • Left image:Cosmic ray muon passing through a cloud chamber undergoes scattering by a small angle in the middle metal plate and leaves the chamber.Right image: Cosmic ray muon losing considerable energy after passing through the plate as indicated by the increased curvature of the track in a magnetic field.
  • Increase of ionization with altitude as measured by Hess in 1912 (left) and by Kolhörster (right)
  • Hess lands after his balloon flight in 1912.
  • Sources of ionizing radiation in interplanetary space.
  • access-date=31 May 2013}}</ref>
  • 160px
  • Shock front acceleration (theoretical model for supernovae and active galactic nuclei): Incident proton gets accelerated between two shock fronts up to energies of the high-energy component of cosmic rays.
  • url-status=dead}}</ref>
  • The [[VERITAS]] array of air Cherenkov telescopes.
HIGH-SPEED, I.E. HIGH-ENERGY PARTICLE, MAINLY ORIGINATING IN OUTER SPACE, OUTSIDE THE SOLAR SYSTEM
Galactic cosmic ray; Cosmic radiation; Cosmic-ray; Cosmic Ray; Anomalous cosmic ray; Cosmic Rays; Galactic cosmic rays; Auger shower; Cosmoclimatology; Galatic cosmic rays; Extensive shower; Cosmic-ray mesons; Cosmic-ray detector; Cosmic-rays; Cosmic rays; Galactic cosmic radiation; Cosmic particle; Origins of cosmic rays; Origin of cosmic rays; Primary cosmic rays; Primary cosmic ray; Secondary cosmic rays; Astroparticle
κοσμικές ακτίνες

Definitie

galactic
[g?'lakt?k]
¦ adjective relating to a galaxy or galaxies.
?Astronomy measured relative to the galactic equator.
Derivatives
galactically adverb
Origin
C19: from Gk galaktias (see galaxy) + -ic.

Wikipedia

Galactic year

The galactic year, also known as a cosmic year, is the duration of time required for the Sun to orbit once around the center of the Milky Way Galaxy. One galactic year is 230 million Earth years. The Solar System is traveling at an average speed of 230 km/s (828,000 km/h) or 143 mi/s (514,000 mph) within its trajectory around the galactic center, a speed at which an object could circumnavigate the Earth's equator in 2 minutes and 54 seconds; that speed corresponds to approximately 1/1300 of the speed of light.

The galactic year provides a conveniently usable unit for depicting cosmic and geological time periods together. By contrast, a "billion-year" scale does not allow for useful discrimination between geologic events, and a "million-year" scale requires some rather large numbers.