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This document serves as a worksheet for a group lab activity on the dark matter structure of the universe, exploring the Big Bang theory, dark matter in 2D and 3D simulations, and the expansion of
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How to fill out Dark Matter Structure of the Universe

01
Gather all relevant data on galaxies and cosmic structures.
02
Use telescopes to observe gravitational effects on visible matter.
03
Analyze the distribution of galaxies and their movements.
04
Apply simulations to model how dark matter influences structure formation.
05
Compile findings into a comprehensive report that outlines the evidence and conclusions regarding dark matter's role.

Who needs Dark Matter Structure of the Universe?

01
Astrophysicists seeking to understand the universe's composition.
02
Cosmologists studying the evolution of the universe.
03
Researchers developing models of galaxy formation.
04
Theoretical physicists exploring the nature of dark matter.
05
Students and educators in fields related to astronomy and physics.
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Our hypothesis is not that black holes are dark matter, but that dark matter would consist of substances from black holes, including sterile neutrinos associated with a magnetic charge.
Dark matter is thought to serve as gravitational scaffolding for cosmic structures. After the Big , dark matter clumped into blobs along narrow filaments with superclusters of galaxies forming a cosmic web at scales on which entire galaxies appear like tiny particles.
Unlike normal matter, dark matter does not interact with the electromagnetic force. This means it does not absorb, reflect or emit light, making it extremely hard to spot. In fact, researchers have been able to infer the existence of dark matter only from the gravitational effect it seems to have on visible matter.
Dark matter is that invisible glue that keeps stars, dust, and gas together in a galaxy. This mysterious substance makes up the majority of a galaxy's mass and forms the foundation of our Universe's structure. Dark matter is still one of the greatest mysteries of science. Credit: NASA/JPL-Caltech.
Like the jelly beans in this jar, the Universe is mostly dark: about 96 percent consists of dark energy (about 69%) and dark matter (about 26%). Only about 5 % (the same proportion as the lighter colored jelly beans) of the Universe — including the stars, planets and us — is made of familiar atomic matter.
So far as we know at this time, dark matter only interacts through gravity. It is also possibly very diffuse, only detectable on much larger scales like the size of galaxies. Gravity is the weakest force. Therefore, based on what little we know, it seems the effect would be effectively unmeasurable on a human scale.
She teamed up with Kent Ford, an astronomer who had developed an extremely sensitive spectrometer. Rubin and Ford used the spectrometer to spread out the spectrum of light coming from the stars in different parts of spiral galaxies. The stars in the disk of a galaxy move in roughly circular orbits around the center.
In the standard Lambda-CDM model of cosmology, the mass–energy content of the universe is 5% ordinary matter, 26.8% dark matter, and 68.2% a form of energy known as dark energy. Thus, dark matter constitutes 85% of the total mass, while dark energy and dark matter constitute 95% of the total mass–energy content.

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Dark Matter Structure of the Universe refers to the unseen components of the universe that do not emit light or energy, making them invisible to current detection methods. It plays a crucial role in the gravitational framework of the universe, influencing the formation and movement of galaxies and clusters.
Currently, there is no official requirement to 'file' anything specific regarding Dark Matter Structure of the Universe as it is a theoretical construct studied by astrophysicists and astronomers rather than a legal or administrative document.
Since Dark Matter Structure of the Universe is not a formal document or a tangible application to fill out, there are no specific instructions for 'filling out' related to it. Research in this area is conducted through scientific studies, simulations, and observation rather than forms.
The purpose of studying Dark Matter Structure of the Universe is to understand the underlying framework that governs cosmic formation and evolution. It helps scientists explain phenomena like galaxy rotation curves, gravitational lensing, and the large-scale structure of the cosmos.
As Dark Matter Structure of the Universe is primarily a scientific concept rather than a document, there is no specific information mandated to be reported. However, studies typically include theoretical models, observational data, and results from simulations related to dark matter's effects on the universe.
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