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

01
Gather all necessary data: Collect observational data from telescopes and other instruments regarding galaxy distributions and cosmic microwave background.
02
Choose a suitable model: Select a theoretical framework that explains the presence of dark matter, like the Lambda Cold Dark Matter (ΛCDM) model.
03
Create simulations: Use computational tools to simulate galaxy formation and structure based on the chosen model.
04
Match simulations with observations: Compare the simulation results with actual observational data to assess accuracy.
05
Adjust parameters: Fine-tune the model parameters based on discrepancies between simulated outcomes and observed structures.
06
Analyze structures: Identify and describe key features of dark matter structures in the universe, such as halos and filaments.
07
Document findings: Prepare a detailed report of the methodology, analysis, and conclusions drawn from the study.

Who needs Dark Matter Structure of the Universe?

01
Astrophysicists and cosmologists: They require a comprehensive understanding of the universe's structure to study cosmic evolution.
02
Academic researchers: Those engaged in theoretical and observational research need insights into dark matter for their work.
03
Government and space agencies: Organizations involved in space exploration and research look into dark matter to inform future missions.
04
Educators and students: They need knowledge about dark matter to educate and enhance learning about the universe.
05
Technology developers: Companies creating instruments or software for astronomical research might require understanding of dark matter dynamics.
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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.
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.
As humbling as it sounds, normal matter almost certainly accounts for the smallest proportion of the Universe, somewhere between 1% and 10%.
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.
Visible matter (everything we can see, including stars and planets) only makes up around 5% of the universe. Scientists are investigating the nature of the unknown 95%.
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.
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.

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Dark Matter Structure of the Universe refers to the theoretical framework that describes how dark matter, a non-luminous and invisible component of the cosmos, influences the formation, evolution, and arrangement of galaxies and clusters of galaxies. It plays a crucial role in the large-scale structure of the universe.
The concept of Dark Matter Structure is primarily related to astrophysicists and cosmologists conducting research on the universe's structure. There are no formal filing requirements as it pertains to scientific study rather than regulatory documentation.
As there is no filing process for Dark Matter Structure, researchers typically engage in observational and theoretical studies. They collect data using telescopes and simulations to analyze the distribution and properties of dark matter in the universe.
The purpose is to understand the nature of dark matter and its role in shaping the universe. This knowledge helps scientists explain the formation of galaxies, cosmic structures, and the overall dynamics of the universe.
The information typically includes data on dark matter density, distribution, gravitational effects on visible matter, and insights from simulations and observational results that validate or challenge existing theories.
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