Type of variable star.
Cepheid Variables have played a crucial role in our understanding of the universe. Their unique properties have allowed astronomers to measure distances on a cosmic scale. In this article, we will explore three significant case studies involving Cepheid Variables.
The Andromeda Galaxy, also known as M31, is the closest spiral galaxy to the Milky Way and is one of the few galaxies that can be seen unaided from the Earth. In 1923, Edwin Hubble discovered a Cepheid Variable star in the Andromeda Galaxy.
Hubble used the period-luminosity relationship of Cepheid Variables to calculate the distance to the star, and hence to the Andromeda Galaxy itself. His calculations showed that the Andromeda Galaxy was far too distant to be part of the Milky Way, proving for the first time that the universe consisted of multiple galaxies.
Before the discovery of Cepheid Variables in other galaxies, they were used to measure the size of our own galaxy, the Milky Way. In the early 20th century, Harlow Shapley used Cepheid Variables to estimate the size of the Milky Way and the Sun's position within it.
Shapley found that the Milky Way was much larger than previously thought, and that the Sun was not at the center. This was a significant shift in our understanding of our place in the universe.
Even today, Cepheid Variables continue to contribute to our understanding of the universe. For example, in 2013, astronomers used the Hubble Space Telescope to observe a Cepheid Variable in a galaxy known as NGC 4258.
This particular Cepheid Variable was unique because its distance had also been measured using Water Maser Emission, an entirely different method. The agreement between the two measurements provided a powerful validation of the accuracy of the Cepheid distance scale.
In conclusion, Cepheid Variables have been instrumental in our exploration of the universe. From the discovery of other galaxies to the measurement of the size of our own, these fascinating stars continue to illuminate our understanding of the cosmos.