1) The measured velocities of stars in the outer reaches of galaxies.
2) The distortion of the path of light from distant galaxies.
Neither of these can be explained by the amount of luminous matter we see in galaxies and in our Universe, meaning either we don't understand gravity OR there's some stuff out there we don't understand. The latter idea is conceptually easier to overcome, but it still leaves open the simple question: what IS that stuff? Because we can't answer that question, we simply call it "dark" matter.
We will, one day, likely understand dark matter as well as we understand x-rays today -- even though the latter were, when first found, so mysterious we called them 'x' rays.
These helped predict the existence of dark matter. Dark matter in astronomy is used appear as the result of mass, where no actual mass can be seen.
Astronomers detect the existence of dark objects in space through indirect methods like gravitational lensing, where the object's gravity bends light from background sources. They also use the dynamics of stars and galaxies to infer the presence of unseen mass, such as in the case of dark matter.
Astronomers make predictions about celestial events based on theories and observations. Some predictions that have been proved include the existence of black holes and the existence of exoplanets. Some predictions that have been disproved include certain theories about the behavior of dark matter and the nature of certain astronomical phenomena.
This is not known. All that is known about dark matter is that it has mass. Searches are underway to try to work out what it is. The existence of dark matter was learned rather recently, and its composition is still being speculated, hence the name. There are several theories about what dark matter may be made of.
Dark matter may be invisible to light, but it can still be detected, through its gravitational interactions. Specifically, it can be detected: * By the fact that galaxies rotate way too fast, for the amount of known matter. * By gravitational lensing.
most of the mass in a cluster of galaxies is invisible, which provides astronomers with the strongest evidence that the universe contains a great amount of DARK MATTER
most of the mass in a cluster of galaxies is invisible, which provides astronomers with the strongest evidence that the universe contains a great amount of DARK MATTER
The evidence for the existence of dark matter in the universe includes the extra mass of Galactic clusters discovered by Fritz Zwicky, and the spinning galaxies which rotate at the same speed as discovered by Vera Rubin.
The motions indicate a greater gravitation pull than from what we see.
These helped predict the existence of dark matter. Dark matter in astronomy is used appear as the result of mass, where no actual mass can be seen.
Astronomers detect the existence of dark objects in space through indirect methods like gravitational lensing, where the object's gravity bends light from background sources. They also use the dynamics of stars and galaxies to infer the presence of unseen mass, such as in the case of dark matter.
That is because the dark matter attracts normal matter through its gravitation.
The gravitational effects. For example, gravitational lensing; also, galaxies spin way too fast for the amount of known matter.
Astronomers make predictions about celestial events based on theories and observations. Some predictions that have been proved include the existence of black holes and the existence of exoplanets. Some predictions that have been disproved include certain theories about the behavior of dark matter and the nature of certain astronomical phenomena.
'Dark matter' and 'dark energy' have not been observed or proven yet.
'Dark matter' and 'dark energy' have not been observed or proven yet.
Hypothetically Yes - But then dark matter is expected to be very pervasive in the cosmos, and pretty much associated with normal matter. The prevailing hypothesis is that dark matter presence is accumulated consistent mass density; i.e. the more mass density, the greater the accumulation of dark matter. However, important as dark matter is thought to be in the cosmos, direct evidence of its existence and a concrete understanding of its nature have remained elusive.