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Catherine Cress - CHPC Conference
Catherine Cress - CHPC Conference

... 1. Instrument simulations for the Atacama Cosmology Telescope 2. N-body simulations for galaxy evolution and cosmology studies 3. Statistical techniques for experimental “forecasting” eg MCMC ...
Outline - Picnic Point High School
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... As part of this ongoing process the Sun and the Solar System were formed over 4x109 years ago from a gas cloud which resulted from a supernova explosion. The condensing gas and dust that formed the Sun and the planets contained all its original elements. The planets were formed when matter came toge ...
How big is the Universe? - Contemporary Science Issues
How big is the Universe? - Contemporary Science Issues

... • The Greeks and religions thought the universe was static, its size was constant. • Is this possible? • Gravity would cause the universe to collapse in on itself! • Do we see this happening? • The only solution to this was for the galaxies to be moving away from each other. The universe was expandi ...
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Watching Galaxies Form Near the Beginning of Time

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... All of this leads to the standard so called concordance cosmology, or “ΛCDM” (Lambda stands for vacuum energy and ‘CDM’ is “cold dark matter”). • The universe started from a very dense state 13.7 Billion years ago and has expanded ever since • In the very beginning the expansion was enormous (inflat ...
Astrophysics * Glossary - Uplift Summit International
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... In 1960 it was proposed that sometime during the early history of the Universe it was at a sufficiently high temperature to produce helium by fusion. In this process many high energy photons would be produced. The CMB (Cosmic Microwave Background Radiation) radiation was emitted only a few hundred t ...
The Early Universe and the Big Bang
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... Due to the unique Tucson location and the wide variety of student backgrounds, AST 102LB offers students many options in terms of lab experience. These options include self-initiated field trips, personal observational projects, in-class collaborative laboratory activities, and individualized labora ...
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... Life demands the presence of elements, heavier than hydrogen. The production of heavy elements demands thermonuclear combustion. Thermonuclear combustion normally requires several 109 years of cookin time in a star. Several 109 years of time will not and cannot be available in a closed universe, acc ...
Gresham Lecture, Wednesday 15 December 2010 Unsolved
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... apparent "asymmetry", or difference, between matter and antimatter to explain why there arose this tiny excess of matter over antimatter. Today, antimatter is created primarily by cosmic rays - extraterrestrial high-energy particles that form new particles as they penetrate the earth's atmosphere. I ...
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E-ELT - Science and Technology Facilities Council
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... • explore the nature and distribution of dark matter and dark energy, thought to make up most of our Universe, but as yet not directly observed or understood • measure changes in the expansion rate of the Universe, without the need to make assumptions such as a standard luminosity for distant supern ...
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... Einstein introduced the world to his theory of general relativity, scientists are seeing that he was right all along about measuring what we now call dark matter. Astronomers supported by the National Science Foundation have found the first evidence of an effect called cosmological shear, a phenomen ...
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PPT - Wayne State University Physics and Astronomy
PPT - Wayne State University Physics and Astronomy

... •In the intervening time, the universe has expanded, but this original energy can be seen in the cosmic microwave background. ...
Measuring the Masses of Galaxies in the Sloan Digital Sky Survey
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... By probing for weak lensing - how is the apparent shape of galaxies altered by intervening materials? 2. Another strength will be looking for near-Earth objects, as well as more distant objects in our solar system - will find 90% of potentially hazardous asteroids down to 140 m in 10 years of operat ...
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Wilkinson Microwave Anisotropy Probe

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