Red shift is the apparent elongation of the wavelength of light reaching us from distant sources of light due to the expansion of space in between. The amount of red shift can be used to work out the recessional velocity of a galaxy and it's distance from us.
Redshift is a phenomenon where light from distant galaxies appears redder than expected due to the expansion of the universe. It tells us that the universe is expanding and provides evidence for the Big Bang theory. By studying the redshift of galaxies, scientists can understand the rate of expansion and the age of the universe.
Many of the galaxies observed in the Hubble Deep Field appear young due to their high redshift values, which indicate they are seen as they were in the early universe. These galaxies often exhibit irregular shapes, high levels of star formation, and significant amounts of gas and dust, suggesting they are in formative stages of development. Additionally, their light has taken billions of years to reach us, meaning we are observing them as they were shortly after the Big Bang, confirming their youth.
The redshift tells scientists how fast a star or galaxy is moving away from us.
The Andromeda Galaxy is getting closer to the Milky Way, and this is primarily observed through redshift measurements. Unlike most galaxies, which are moving away from us due to the expansion of the universe, Andromeda shows a blueshift, indicating it is approaching. Additionally, astronomers have tracked its velocity and trajectory, confirming that it is on a collision course with our galaxy, expected to occur in about 4.5 billion years. Observations of its gravitational effects and interactions with nearby galaxies further support this conclusion.
In simplest terms, the shift of galactic spectral lines towards the red end of the spectrum would indicate simply that the galaxy in question is receding from the observer. This is an example of the Doppler effect, where the frequency is lowered (wavelengths become longer, and in this case energy of the photons is decreased) by the relative motion of the observer. The redshifting of galaxies in all directions became the primary evidence of an expanding universe (cosmological redshift). Because the expansion of the universe is fairly uniform in all directions, those galaxies that are most distant are receding the fastest and thus evidence the greatest amount of redshift. By contrast, if a characteristic spectral line of a galaxy or other object shifted towards the blue end of the spectrum (shorter wavelengths), it would be traveling towards the observer.
Redshift is a phenomenon where light from distant galaxies appears redder than expected due to the expansion of the universe. It tells us that the universe is expanding and provides evidence for the Big Bang theory. By studying the redshift of galaxies, scientists can understand the rate of expansion and the age of the universe.
By the redshift of the galaxies. In general, the farther away a galaxy is from us, the faster it moves away from us.
Mainly that galaxies that are very far away (i.e., from the distant past) look different to galaxies that are near-by (from the more recent past).
Redshift or blueshift is a change in the frequency of the light you receive, compared to the frequency at which it was emitted. A redshift is a reduction in frequency; this basically means that the object that emits the light is moving away from you.
No. You can figure out exactly what elements are in stars and galaxies by examining the color spectrum of the light detected; the frequencies of the bright and dark lines in the spectrum tell you what's what. But there's a problem. For distant galaxies, the light spectrum is wrong. The frequency lines of the spectrum are all too low. One possible explanation of the incorrect spectrum is that those stars and galaxies are MOVING AWAY from us, and that the spectrum is shifted toward the red end of the color spectrum because of the Doppler effect. So scientists believe that the "red-shift" on the color spectrum of stars and galaxies indicate that they are moving away. Not all galaxies show a red-shift; the Andromeda Galaxy, M31, shows a pronounced BLUE-shift, indicating that it is heading TOWARD us. In fact, scientists believe that the Milky Way and Andromeda will probably collide in about 3 billion years.
The Big Bang theory describes the early universe as a hot, dense state that expanded rapidly around 13.8 billion years ago. Initially, it was filled with energy and fundamental particles, which eventually cooled to form atoms, leading to the creation of stars and galaxies. This theory explains the observed redshift of distant galaxies and the cosmic microwave background radiation, providing evidence for the universe's expansion and its origins. Overall, it suggests that the universe has been evolving from a simple, uniform state to the complex structure we observe today.
Many of the galaxies observed in the Hubble Deep Field appear young due to their high redshift values, which indicate they are seen as they were in the early universe. These galaxies often exhibit irregular shapes, high levels of star formation, and significant amounts of gas and dust, suggesting they are in formative stages of development. Additionally, their light has taken billions of years to reach us, meaning we are observing them as they were shortly after the Big Bang, confirming their youth.
i can tell that there are many galaxies beyond the milky way like magalang and matulungin
The redshift tells scientists how fast a star or galaxy is moving away from us.
The light astronomers observe through telescopes provides crucial information about galaxies, including their composition, temperature, distance, and motion. Different wavelengths of light, such as visible, infrared, and ultraviolet, reveal the presence of elements, star formation rates, and the dynamics of galaxy structures. By analyzing the spectra of this light, astronomers can also determine redshift, which helps measure the galaxy's speed and distance from Earth, offering insights into the universe's expansion. Overall, light serves as a fundamental tool for understanding the nature and evolution of galaxies.
They get distant, but you have to see it.
The redshift was not "invented" by anyone. It is a natural phenomenon that has always been with us. It was the Austrian mathematician and physicist Christian Doppler who first described the effect in the year 1842. The idea was latched onto by astronomers who (eventually) applied it to observations of more and more distant galaxies. These observers found that by taking the colors of the observed light and shifting them up, the light looked "more normal" to the observers. It was then easy to deduce that the galactic light sources were receding, and the the speed of recession could be calculated based on their redshift. Links can be found below for more information.