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Edwin Hubble measured the distance to the Andromeda Galaxy by observing the light from its variable stars, specifically Cepheid variables. He utilized the relationship between the luminosity and the pulsation period of these stars to determine their absolute brightness. By comparing this intrinsic brightness with the observed brightness, Hubble could calculate the distance to Andromeda, ultimately establishing it as a separate galaxy outside the Milky Way. This groundbreaking work significantly expanded our understanding of the universe.
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How did Edwin Hubble measure the distance to the Andromeda Galaxy?
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.
What two measurements are required to determine the Hubble constant?
To determine the Hubble constant, two key measurements are required: the distance to a galaxy and its redshift. The distance can be obtained using various methods, such as the cosmic distance ladder, while the redshift is measured through the light spectrum emitted by the galaxy, indicating how fast it is moving away from us due to the expansion of the universe. By plotting these values, astronomers can calculate the Hubble constant, which describes the rate of this expansion.
Is the Hubble galaxy the closest major galaxy to our own?
No, the Hubble Galaxy (Messier 31, or the Andromeda Galaxy) is not the closest major galaxy to our own. The Andromeda Galaxy is located about 2.537 million light-years from the Milky Way. The closest major galaxy to us is the Triangulum Galaxy (Messier 33), which is approximately 3 million light-years away.
what is the Hubble effect?
The Hubble effect, also known as Hubble's Law, describes the observation that galaxies are moving away from us, and their speed is proportional to their distance from Earth. This phenomenon is a key piece of evidence for the expanding universe theory, indicating that the universe has been expanding since the Big Bang. The relationship is expressed mathematically as ( v = H_0 \times d ), where ( v ) is the velocity of a galaxy, ( H_0 ) is the Hubble constant, and ( d ) is the distance to the galaxy. The Hubble effect provides crucial insights into the dynamics and evolution of the cosmos.
What is the recessional velocity of a galaxy at a distance of 200 Mpc?
The recession velocity of a galaxy at a distance of 200 Mpc (mega-parsecs) would depend on Hubble's Law and the rate of expansion of the universe. For a rough estimate, assuming a Hubble constant of 70 km/s/Mpc, the recession velocity would be around 14,000 km/s.
How did Edwin Hubble measure the distance to the Andromeda Galaxy?
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.
What is the type of star used by Hubble to measure the distance to other galaxies?
what is the type of star used by the Hubble to measure the distance to other galaxies.
Edwin Hubble demonstrated that distant galaxies existed by measuring which type of stars?
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.
Who measure the distance of Andromeda nebulae?
Hubble
What was Edwin Hubble's equation?
Hubble's equation states that the velocity at which various galaxies are receding from the Earth is proportional to their distance from us.The law is often expressed by the equation v = H0D, with H0 the constant of proportionality (the Hubble constant) between the distance D to a galaxy and its velocity v. The SI unit of H0 is s-1 but it is most frequently quoted in (km/s)/Mpc, thus giving the speed in km/s of a galaxy one Megaparsec away. The reciprocal of H0 is the Hubble time.
What did the astronnmer Edwin Hubble discover about the relationship between the distance of a galaxy and the rate at which it is receding?
He discovered that the farther away a galaxy was, the faster it was moving away from Earth.
What two measurements are required to determine the Hubble constant?
To determine the Hubble constant, two key measurements are required: the distance to a galaxy and its redshift. The distance can be obtained using various methods, such as the cosmic distance ladder, while the redshift is measured through the light spectrum emitted by the galaxy, indicating how fast it is moving away from us due to the expansion of the universe. By plotting these values, astronomers can calculate the Hubble constant, which describes the rate of this expansion.
How quickly is the universe expanding?
The farther away a galaxy, the faster it will go away from us. Check the Wikipedia article on "Hubble's Law" for more details. According to the article, the currently accepted value for the "Hubble constant" is 74.2 ± 3.6 (km/s)/Mpc. That is to say, if a galaxy is at a distance of 1 Megaparsec, on average our distance from this galaxy will increase at a rate of about 74 km/s. For a galaxy at 2 Megaparsec distance, the speed would increase at twice this value, etc.
Is the Hubble galaxy the closest major galaxy to our own?
No, the Hubble Galaxy (Messier 31, or the Andromeda Galaxy) is not the closest major galaxy to our own. The Andromeda Galaxy is located about 2.537 million light-years from the Milky Way. The closest major galaxy to us is the Triangulum Galaxy (Messier 33), which is approximately 3 million light-years away.
what is the Hubble effect?
The Hubble effect, also known as Hubble's Law, describes the observation that galaxies are moving away from us, and their speed is proportional to their distance from Earth. This phenomenon is a key piece of evidence for the expanding universe theory, indicating that the universe has been expanding since the Big Bang. The relationship is expressed mathematically as ( v = H_0 \times d ), where ( v ) is the velocity of a galaxy, ( H_0 ) is the Hubble constant, and ( d ) is the distance to the galaxy. The Hubble effect provides crucial insights into the dynamics and evolution of the cosmos.
He originally suggested that galaxies are moving farther away He also suggested that the distance of a galaxy is proportional to its recessional speed who is He?
Edwin Hubble.
What is the recessional velocity of a galaxy at a distance of 200 Mpc?
The recession velocity of a galaxy at a distance of 200 Mpc (mega-parsecs) would depend on Hubble's Law and the rate of expansion of the universe. For a rough estimate, assuming a Hubble constant of 70 km/s/Mpc, the recession velocity would be around 14,000 km/s.
