
Spectroscopy - Mr. Borchik
... Definitions • Spectroscopy- the study of the light from an object. • Spectrometer- an instrument which spreads out light making a spectra. • Spectra- range of electromagnetic energy separated by wavelength. ...
... Definitions • Spectroscopy- the study of the light from an object. • Spectrometer- an instrument which spreads out light making a spectra. • Spectra- range of electromagnetic energy separated by wavelength. ...
Today`s Powerpoint
... 2. If you are in freefall, you are also weightless. Einstein says these are equivalent. So in freefall, the light and the ball also travel in straight lines. 3. Now imagine two people in freefall on Earth, passing a ball back and forth. From their perspective, they pass the ball in a straight line. ...
... 2. If you are in freefall, you are also weightless. Einstein says these are equivalent. So in freefall, the light and the ball also travel in straight lines. 3. Now imagine two people in freefall on Earth, passing a ball back and forth. From their perspective, they pass the ball in a straight line. ...
HEIC0007 Photo release: Stephan`s Quintet
... finally resolved. Hubble's resolution is so high that individual stars can be discerned in NGC 7320, showing that it is definitely closer than the more remote, compact group of galaxies. Today other measurements have also shown that the galaxies NGC 7320C and NGC 7318B are just passing and are not b ...
... finally resolved. Hubble's resolution is so high that individual stars can be discerned in NGC 7320, showing that it is definitely closer than the more remote, compact group of galaxies. Today other measurements have also shown that the galaxies NGC 7320C and NGC 7318B are just passing and are not b ...
Big Bang Balloon
... Big Bang Balloon An activity you can use in the classroom In the 1920s astronomer Edwin Hubble used the red shift of the spectra of stars to determine that the universe was expanding. By carefully observing the light from galaxies at different distances from Earth, he determined that the farther som ...
... Big Bang Balloon An activity you can use in the classroom In the 1920s astronomer Edwin Hubble used the red shift of the spectra of stars to determine that the universe was expanding. By carefully observing the light from galaxies at different distances from Earth, he determined that the farther som ...
pptx
... At any location in a universe that is expanding, galaxies that are farther away will appear to be moving away faster. In other words, the Hubble Law would be observed by everyone in an expanding universe. Rather than indicating that we are at the center of the universe, the Hubble Law tells us that ...
... At any location in a universe that is expanding, galaxies that are farther away will appear to be moving away faster. In other words, the Hubble Law would be observed by everyone in an expanding universe. Rather than indicating that we are at the center of the universe, the Hubble Law tells us that ...
Astronomy
... Astronomy Galaxies Test Name: Directions: Answer the following questions with the most correct answers. TRUE/FALSE: 1. _____ Hubble classified galaxies 2. _____ There are three main classifications of galaxies 3. _____ Elliptical galaxies have little or no star formation 4. _____ Elliptical galaxies ...
... Astronomy Galaxies Test Name: Directions: Answer the following questions with the most correct answers. TRUE/FALSE: 1. _____ Hubble classified galaxies 2. _____ There are three main classifications of galaxies 3. _____ Elliptical galaxies have little or no star formation 4. _____ Elliptical galaxies ...
The evolution of galaxy groups
... • More star formation in groups at z=0.5 than at z=0 • On average, groups at 0
... • More star formation in groups at z=0.5 than at z=0 • On average, groups at 0
Key Topics Astronomy Unit
... expanded explosively into existence about 13.7 billion years ago. • After the big bang, the universe expanded quickly, and continues to expand, and cooled enough for atoms to form. • Gravity pulled the atoms together into gas clouds that eventually became stars, which comprise young galaxies. ...
... expanded explosively into existence about 13.7 billion years ago. • After the big bang, the universe expanded quickly, and continues to expand, and cooled enough for atoms to form. • Gravity pulled the atoms together into gas clouds that eventually became stars, which comprise young galaxies. ...
Redshift
In physics, redshift happens when light or other electromagnetic radiation from an object is increased in wavelength, or shifted to the red end of the spectrum. In general, whether or not the radiation is within the visible spectrum, ""redder"" means an increase in wavelength – equivalent to a lower frequency and a lower photon energy, in accordance with, respectively, the wave and quantum theories of light.Some redshifts are an example of the Doppler effect, familiar in the change of apparent pitches of sirens and frequency of the sound waves emitted by speeding vehicles. A redshift occurs whenever a light source moves away from an observer. Another kind of redshift is cosmological redshift, which is due to the expansion of the universe, and sufficiently distant light sources (generally more than a few million light years away) show redshift corresponding to the rate of increase in their distance from Earth. Finally, gravitational redshift is a relativistic effect observed in electromagnetic radiation moving out of gravitational fields. Conversely, a decrease in wavelength is called blueshift and is generally seen when a light-emitting object moves toward an observer or when electromagnetic radiation moves into a gravitational field. However, redshift is a more common term and sometimes blueshift is referred to as negative redshift.Knowledge of redshifts and blueshifts has been applied to develop several terrestrial technologies such as Doppler radar and radar guns. Redshifts are also seen in the spectroscopic observations of astronomical objects. Its value is represented by the letter z.A special relativistic redshift formula (and its classical approximation) can be used to calculate the redshift of a nearby object when spacetime is flat. However, in many contexts, such as black holes and Big Bang cosmology, redshifts must be calculated using general relativity. Special relativistic, gravitational, and cosmological redshifts can be understood under the umbrella of frame transformation laws. There exist other physical processes that can lead to a shift in the frequency of electromagnetic radiation, including scattering and optical effects; however, the resulting changes are distinguishable from true redshift and are not generally referred to as such (see section on physical optics and radiative transfer).