• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
ASTR-264-Lecture
ASTR-264-Lecture

... local group of galaxies in the local supercluster How did we come to be? -matter in our bodies came from big bang, which produced hydrogen and helium -all other elements were constructed from H and He in start and then recycled into new solar systems How can we know that the universe was like in the ...
5th_state_of_matter - the Electric Universe!
5th_state_of_matter - the Electric Universe!

... Ice is transformed to water at 0°C when the energy of its molecules (particles) increases. Water is similarly transformed to vapour at 100°C (Fig.1). Much stronger zig-zag motion of the particles separates and ionises hydrogen and oxygen i.e. plasma comes into existence (above 13 000 K). Do all bodi ...
Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

... Supernovae are not alike. For decades, astronomers had known that supernovae fell into different types based on their light curves, that is, their pattern of rising and falling brightness. Later, they found these types actually corresponded to different physical circumstances triggering the explosio ...
dark matter?
dark matter?

... at least 1 billion times less massive — so the universe would need a whole lot more axions than WIMPs to make up all the invisible matter. One would expect that with so many CDM particles, WIMPs or axions would be easy to find. But because they don’t interact through the electromagnetic force, detec ...
Cosmology: Black Holes, Dark Matter and Dark Energy
Cosmology: Black Holes, Dark Matter and Dark Energy

... VLBA Reveals Closest Pair of Supermassive Black Holes Astronomers using the National Science Foundation's Very Long Baseline Array (VLBA) radio telescope have found the closest pair of supermassive black holes ever discovered in the Universe -- a duo of monsters that together are more than 150 milli ...
File - Science Website
File - Science Website

... One theory of the origin of the Universe was that billions of years ago all matter was in one place, then it exploded (‘big bang’). Describe, in as much detail as you can, how our star (the Sun) formed from the time when there was just dust and gas (mostly hydrogen) up to now when it is in its main ...
Chapter 3 Cosmology 3.1 The Doppler effect
Chapter 3 Cosmology 3.1 The Doppler effect

... www.oxfordsecondary.co.uk/acknowledgements This resource sheet may have been changed from the original. ...
Chapter 26 Photons
Chapter 26 Photons

... The question is whether the electric force is capable of ejecting an electron from the metal surface. A certain amount of energy is required to do this. For example, in our electron gun experiment we had to heat the filament in order to get an electron beam. It was the thermal energy that allowed el ...
The Hubble Space Telescope
The Hubble Space Telescope

... Scientist for the FOC, comments: “Although the images obtained with the FOC have only rarely been as photogenic as the famous images from the Wide Field and Planetary Camera 2, the FOC has served the astronomical community well and brought home its fair share of scientific firsts.” Observations made ...
Stars, Galaxies, and the Universe Section 1 Section 1
Stars, Galaxies, and the Universe Section 1 Section 1

... from Earth, is caused by the movement of Earth. • The stars seem as though they are moving counterclockwise around a central star called Polaris, the North Star. Polaris is almost directly above the North Pole, and thus the star does not appear to move much. • Earth’s revolution around the sun cause ...
sun.galaxy.notes
sun.galaxy.notes

... • It is difficult to know for sure because it is impossible to see our galaxy from the outside • You can see the Milky Way stretching across the night sky as a faint band of light • All of the stars you can see in the night sky belong to the Milky Way ...
Where Do Chemical Elements Come From?
Where Do Chemical Elements Come From?

... occur when there is no longer enough fuel for the fusion process in the core of the star to create an outward pressure which combats the inward gravitational pull of the star's great mass. First, the star will swell into a red supergiant...at least on the outside. On the inside, the core yields to g ...
Supermassive black holes
Supermassive black holes

... younger, more metal rich and orbit in the same orientation, excepting some up and down motion ...
© Taganov I
© Taganov I

... and protoglobularstarcluster (PGC) masses and freezing to solid H-He dark objects as the expanding universe cooled, Fig. 1e. We see from Tadpole that stars form from planets in dense clumps of planets, not from gas clouds falling into merging, mythical, CDM halos. The first stars formed gently at 0. ...
Extremely Large Telescopes
Extremely Large Telescopes

... FALCON concept (Hammer et al) ...
The Hubble Ultra Deep Field Project Overview
The Hubble Ultra Deep Field Project Overview

... Concordance Model is assumed, but you can change these parameters and explore how varying the relative densities of “stuff” in the Universe can change this distance measure. Exercise 1: Galaxy morphology over cosmic time In this exercise you will consider a variety of galaxies over a range of redshi ...
Astrophysics Questions (DRAFT)
Astrophysics Questions (DRAFT)

... 94. Sketch a typical cooling function (T ) for di use interstellar gas and identify its prominent features. Overplot a hypothetical heating curve and show how to identify points of thermal equilibrium and their stability. 95. Explain the physics of 21 cm radio emission from neutral hydrogen atoms. ...
Protogalaxies
Protogalaxies

... of smaller satellites is still possible. Conversely, one often hears assertions that (some) ellipticals are made by merging spirals, which is indeed observed in the nearby universe. Obviously this is not the only possible path: a young elliptical may be made by merging a thousand small fragments ear ...
Protogalaxies Encyclopedia of Astronomy & Astrophysics eaa.iop.org S G Djorgovski
Protogalaxies Encyclopedia of Astronomy & Astrophysics eaa.iop.org S G Djorgovski

... of smaller satellites is still possible. Conversely, one often hears assertions that (some) ellipticals are made by merging spirals, which is indeed observed in the nearby universe. Obviously this is not the only possible path: a young elliptical may be made by merging a thousand small fragments ear ...
Solutions for homework #5, AST 203, Spring 2009
Solutions for homework #5, AST 203, Spring 2009

... The main sequence lifetime of a solar type star is only 1010 years. But only the Hydrogen in the core of the Sun is hot enough to burn, so the Sun ends its main sequence lifetime when only 10% of its hydrogen has burned to helium. 11 points for doing the calculation correctly; 4 points for giving th ...
RECOMBINATION OF HYDROGEN IN THE HOT MODEL OF THE
RECOMBINATION OF HYDROGEN IN THE HOT MODEL OF THE

... in the Wien region. The energy exchange between electrons and radiation in the Compton effect maintains the temperature of matter equal to that of the radiation up to a time corresponding to a red shift of z ~ 150, and this leads, in particular, to a change in the time dependence of the Jeans wavele ...
question - UW Canvas
question - UW Canvas

... 23. How is it that the core of a massive star is able to fuse heavier and heavier elements without any of these stages resulting in degeneracy or any flashes like the helium flash that occurs in solar-type stars? a. The cores of massive stars are so hot, have such high densities and pressures, that ...
astronomy
astronomy

... State Newton’s laws of motion and universal gravitation and explain how they account for Kepler’s laws. Explain how the law of gravitation enables us to measure the masses of astronomical bodies. Chapter 3 & 4 Discuss the nature of electromagnetic radiation, and tell how that radiation transfers ene ...
Document
Document

... • The scenario that leads to nova explosions can produce an even wilder phenomenon. • In the early 1900s `novae’ were sometimes observed in other galaxies and were used to help set the distances to galaxies. • But, when it became clear that even the nearest galaxies were much further away than anyon ...
Introducing a New Product
Introducing a New Product

... While doing so, one must ensure that the Collapse develops from a Regular initial Data. The Trapped Surfaces and Spacetime Singularity Develop then as the collapse evolves, and the main task then is to examine the Nature of the Singularity, namely whether it is Covered within Horizon, or Visible to ...
< 1 ... 16 17 18 19 20 21 22 23 24 ... 71 >

Chronology of the universe



The chronology of the universe describes the history and future of the universe according to Big Bang cosmology, the prevailing scientific model of how the universe developed over time from the Planck epoch, using the cosmological time parameter of comoving coordinates. The model of the universe's expansion is known as the Big Bang. As of 2015, this expansion is estimated to have begun 13.799 ± 0.021 billion years ago. It is convenient to divide the evolution of the universe so far into three phases.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report