they transmit radio wave frequency to space and check for the their return or reflecting time , same as that used to calculate speed of light, for calculating the distance of galaxy.
if the return radio frequency has increased, then they are moving closer to earth and vice versa.
thank you
The Parallax Method. See the link for more info.
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.
Galaxy redshift is much light the Doppler effect. If a galaxy is traveling away from us, the light that it emits and is seen by us is stretched out (the faster we are separating, the stronger the redshift), that means that the wavelegnth is stretched a bit, shifting the light towards red.
A stellar unit refers to a unit of distance used in astronomy to measure the distance between stars. It is typically equivalent to the mean distance between stars within a galaxy, which can vary depending on the galaxy being observed.
Edwin Hubble used Cepheid variable stars to measure the distances to galaxies. These stars have a relationship between their luminosity and pulsation period, allowing astronomers to calculate their distance based on their observed brightness.
The Parallax Method. See the link for more info.
H II regions are regions of ionized gas in a galaxy that emit strong emission lines, allowing astronomers to determine the galaxy's distance using spectroscopy. Cepheid variables are pulsating stars with a period-luminosity relationship that allows astronomers to determine distances to galaxies based on their observed brightness variations. While both methods are used to measure extragalactic distances, they rely on different physical properties of objects within the galaxy.
Astronomers know it's a galaxy and they can measure some key characteristics. Thus they can be reasonably sure they have matched correctly it to a type of galaxy we can see.
When scientists measure the size of the redshift from a galaxy, they can determine its velocity relative to Earth, which helps in understanding its movement away from us due to the expansion of the universe. This redshift also provides insights into the galaxy's distance, allowing astronomers to estimate its location in space. Additionally, analyzing the redshift can reveal information about the galaxy's composition, age, and the effects of cosmic phenomena like gravitational waves or dark energy. Overall, redshift measurements are crucial for understanding the dynamics and evolution of galaxies.
The Milky Way Galaxy.
The distance to the Andromeda galaxy can be measured using various methods, such as parallax measurements, standard candles (e.g., Cepheid variables), and redshift. These methods help astronomers determine the distance of Andromeda from Earth with good accuracy.
Edwin Hubble measured the distance to the Andromeda Galaxy using Cepheid variable stars as standard candles. By observing how the brightness of these stars changed over time, he could determine their true brightness and then calculate their distance based on their apparent brightness. This allowed him to estimate the vast distance to the Andromeda Galaxy.
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.
Wavelengths is what allows astronomers redshift a background galaxy that is covered up. This is due to being close to the foreground galaxy.
The most accurate way to determine the distance to a nearby galaxy is by using the method of parallax, which involves measuring the slight shift in the position of the galaxy as observed from different points in Earth's orbit around the Sun. This method allows astronomers to calculate the distance based on the angle of the shift and the known distance between the observation points.
To measure the distance across our galaxy, astronomers often use methods like parallax, which involves observing the apparent shift of nearby stars against distant background stars as Earth orbits the Sun. For greater distances, they utilize standard candles, such as Cepheid variable stars, whose luminosity can be determined from their pulsation periods. Additionally, the Tying of distances to the cosmic distance ladder helps in calculating distances to the Milky Way's edge, estimated to be about 100,000 light-years across. Combining these techniques allows for a more accurate measurement of the galaxy's dimensions.
Galaxy redshift is much light the Doppler effect. If a galaxy is traveling away from us, the light that it emits and is seen by us is stretched out (the faster we are separating, the stronger the redshift), that means that the wavelegnth is stretched a bit, shifting the light towards red.