## Which of the following describes Hubble’s law?

Hubble’s law, also known as the Hubble–Lemaître law, is the observation in physical cosmology that galaxies are moving away from the Earth at speeds proportional to their distance. In other words, the further they are the faster they are moving away from Earth.

## What is the Hubble’s Law Why is it significant?

Because the exact value of the Hubble constant, H, is so important in extragalactic astronomy and cosmology – it leads to an estimate of the age of the universe, helps test theories of Dark Matter and Dark Energy, and much more – a great deal of effort has gone into working it out. …

## How does the age of the universe depend on Hubble’s constant and why?

We know how fast the universe is expanding, because we know the value of Hubble’s constant (H0 ). The faster the universe is expanding, the faster the galaxies will appear to be moving away from each other. You can actually calculate an estimate for the age of the Universe from Hubble’s Law.

## What is the resolution of the dilemma known as olbers’s paradox?

What is the resolution of the dilemma known as Olbers’s paradox? The observable universe is not infinite in extent and it has evolved in time, the universe has been expanding continuously since the Big Bang.

## What can we learn from Hubble’s law?

Hubble’s law, which says simply that a galaxy’s velocity (or as is sometimes plotted, its redshift) is directly proportional to its distance, also tells us something important about the state of the universe.

## Is Hubble’s law true?

If the theory is not correct, the distances determined in this way are all nonsense. Most astronomers believe that Hubble’s Law does, however, hold true for a large range of distances in the universe. It should be noted that, on very large scales, Einstein’s theory predicts departures from a strictly linear Hubble law.

## What is the value of Hubble’s constant?

Planck found the Hubble constant to be 46,200 mph per million light-years (67.4 km/s/Mpc) in 2018. The two values might not seem very different. But each is extraordinarily precise, and they contain no overlap between their error bars.

## What is meant by dark matter?

Dark matter is composed of particles that do not absorb, reflect, or emit light, so they cannot be detected by observing electromagnetic radiation. Dark matter is material that cannot be seen directly. … Scientists believe that dark matter may account for the unexplained motions of stars within galaxies.

## Why was Hubble’s age of the universe wrong?

This age estimate for the universe, Hubble acknowledged, was clearly less than the age of the Earth, as determined by geologists who measured the radioactivity in rocks. … Walter Baade made the crucial observation that doubled the distance scale and thus resolved the problem that the universe seemed too young.

## What kind of universe do we live in?

We live on a planet called Earth that is part of our solar system. But where is our solar system? It’s a small part of the Milky Way Galaxy. A galaxy is a huge collection of gas, dust, and billions of stars and their solar systems.

## What is the inverse of Hubble’s constant?

The inverse of the Hubble Constant is the Hubble Time, tH = d/v = 1/Ho; it reflects the time since a linear cosmic expansion has begun (extrapolating a linear Hubble Law back to time t = 0); it is thus related to the age of the Universe from the Big-Bang to today.

## How is the flatness problem resolved?

The small universe inflated by a large amount and the part of the universe you can observe appears to be nearly flat. That solves the flatness problem. The horizon problem is solved by inflation because regions that appear to be isolated from each other were in contact with each other before the inflation period.

## What is olbers’s Paradox quizlet?

Olbers’s paradox is that the universe is both flat and curved. False. Observations of distant supernovae indicate that our universe is accelerating in its expansion. True.

## What is the flatness problem quizlet?

flatness problem. In cosmology, the circumstance that the early universe must have contained almost exactly the right amount of matter to close space-time (make space-time flat). Only $2.99/month. horizon problem.