Astronomers can watch galaxies that are far away. Since the light takes billions of years to reach us from the farthest known galaxies, they would be watching galaxies in the early Universe. It turns out, from such observations, that the Universe is changing.
When astronomers investigate the most distant galaxies, they find evidence that the universe was much younger and more active in its early stages. Observations of these galaxies reveal higher rates of star formation and interactions, suggesting that they were in a more chaotic and dynamic state. Additionally, the light from these galaxies has taken billions of years to reach us, allowing astronomers to study the evolution of galaxies over cosmic time. This research helps to deepen our understanding of the universe's formation and the processes that shaped its structure.
Astronomers have various theories on how galaxies are formed, including the idea that they started as small clumps of matter that grew through mergers and collisions. Observations and simulations have provided insights into the evolution of galaxies over billions of years, but the precise details of galaxy formation remain an area of active research and ongoing discovery.
it changes overtime with constant movement and change in rotation
15 Galaxies? There are over 1,000,000,000 galaxies possibly more.
Galaxies are vast collections of stars, gas, dust, and dark matter, and they are the fundamental building blocks of the visible Universe. Clusters of galaxies consist of groups of galaxies bound together by gravity, showcasing the large-scale structure of the cosmos. Together, these galaxies and their clusters form a complex web-like arrangement known as the cosmic web, which defines the distribution of visible matter in the Universe. This structure helps astronomers understand the evolution and dynamics of the Universe over time.
Astronomers consider elliptical galaxies more abundant than spiral galaxies because they are more prevalent in the universe's large-scale structure and are often found in dense environments like galaxy clusters. While more spiral galaxies have been observed, this is partly due to selection bias, as spirals are more visible at certain wavelengths and are often located in less crowded regions. Elliptical galaxies, on the other hand, tend to be older and can be more difficult to detect, leading to an underrepresentation in observational surveys. Additionally, the processes of galaxy evolution suggest that many spirals may eventually evolve into ellipticals over time.
Astronomers determine the size of quasars by analyzing the variability of their light. Quasars show rapid and dramatic changes in brightness over short periods, indicating that they must be very compact, likely smaller than our own solar system. By studying the time scales of these changes, astronomers can estimate the size of quasars.
Astronomers discovered an object pulsing waves in space by observing changes in the intensity of its light over time. This pulsing pattern indicated that the object was emitting regular waves of energy, which led to the discovery of its pulsar nature.
I don't think we can see 100 billion galaxies from our solar system, so it wouldnot be possible to count that many.In any case, assuming it were possible to find, identify, and make a recordof one galaxy every second, then to gather 100 billion of them would takesomething like 3,170 years . . . roughly the length of time that has elapsedsince the Israelites' Exodus from Egypt.
At present the company has 100 galaxies in all over the country and in which 4 galaxies are in Delhi.
The exact number of stars in the universe is not known, but estimates suggest there are around 100 billion to 200 billion stars in our Milky Way galaxy alone, and there are likely over 2 trillion galaxies in the observable universe. Astronomers use various methods, including surveys and calculations based on the brightness of galaxies, to estimate these numbers. The work of astronomers like Edwin Hubble and advancements in telescopic technology have significantly contributed to our understanding of the vastness of the cosmos. However, the true number of stars remains an estimate due to the sheer scale and complexity of the universe.
The number of stars in a galaxy can change due to the birth and death of stars, as well as interactions with other galaxies like mergers and collisions. Additionally, new stars can form from the gas and dust present in galaxies, contributing to changes in the total number of stars over time.