The rotation curves of galaxies show that the stars in the outer regions of galaxies are rotating faster than expected based on the visible mass of the galaxy. This suggests that there is additional mass, or dark matter, present in galaxies.

Dark matter is estimated to make up about 27% of the total mass-energy content of the universe, while ordinary matter makes up about 5% and dark energy makes up the remaining 68%.

Weakly interacting massive particles (WIMPs) are one of the leading candidates for dark matter. They are hypothetical particles that are massive but interact with ordinary matter only through weak interactions, making them difficult to detect.

The main challenge in detecting dark matter is its weak interactions with ordinary matter. This makes it difficult to detect directly, and indirect methods, such as observing its gravitational effects, are typically used.

LUX-ZEPLIN (LZ) is a direct detection experiment that is searching for dark matter particles in the Milky Way. It is located in the Sanford Underground Research Facility in South Dakota, USA.

The Dark Energy Survey is a satellite that is mapping the distribution of dark matter in the universe by measuring the weak gravitational lensing of light from distant galaxies.

Dark matter and dark energy are both forms of energy that make up the universe. Dark matter is thought to be a form of matter that does not interact with ordinary matter, while dark energy is a form of energy that is causing the expansion of the universe to accelerate.

Dark matter plays a crucial role in the formation and evolution of galaxies. It helps to hold galaxies together by providing additional gravitational force, it provides the fuel for star formation by cooling gas clouds, and it regulates the growth of black holes by preventing them from becoming too large.

The impact of dark matter on the future of the universe is still unknown. It depends on the properties of dark matter and the amount of dark energy in the universe. Some theories suggest that dark matter will cause the universe to expand forever, while others suggest that it will eventually cause the universe to collapse in on itself.

Studying dark matter is challenging due to its weak interactions with ordinary matter, its lack of electromagnetic radiation, and its large mass. These properties make it difficult to detect and study directly.

There are several proposed solutions to the dark matter problem, including modified theories of gravity, axion-like particles, and sterile neutrinos. These solutions attempt to explain the observed effects of dark matter without the need for a new type of particle.

Dark matter plays a significant role in cosmology. It helps to explain the formation and evolution of galaxies, provides an explanation for the observed cosmic microwave background radiation, and is a key component in understanding the large-scale structure of the universe.

Future directions in dark matter research include direct detection experiments, indirect detection experiments, and theoretical studies. Direct detection experiments aim to detect dark matter particles directly, while indirect detection experiments aim to detect the effects of dark matter on ordinary matter. Theoretical studies aim to develop new models and theories to explain the nature and properties of dark matter.

Dark matter is a hypothetical particle that is not included in the standard model of physics. It is a mysterious substance that makes up about 27% of the universe, but its exact nature is still unknown.

Dark matter could have profound implications for our understanding of the universe. It could provide an explanation for the observed acceleration of the universe's expansion, help to explain the formation of galaxies and other large structures in the universe, and provide insights into the nature of gravity and the fundamental laws of physics.