• Study Resource
  • Explore
    • 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
Bulletin of the American Meteorological Society
Bulletin of the American Meteorological Society

... The Sun is not a solid body, and so it would not be expected to rotate rigidly. It rotates differentially: at the surface, the polar regions rotate more slowly than the equator, causing a shearing motion between solar plasma at different latitudes. At the equator, the solar synodic rotation period ...
Answering the Fermi Paradox - Acceleration Studies Foundation
Answering the Fermi Paradox - Acceleration Studies Foundation

... to universal transcension. For sixty years answers have been attempted for the Fermi paradox, yet the vast majority neglect what may be the most parsimonious explanation—a process of constrained universal transcension. I propose that any species or von Neumann probe complex enough to improve its int ...
Galactic Encounters: The Dynamics of Mergers and Satellite Accretion
Galactic Encounters: The Dynamics of Mergers and Satellite Accretion

... galaxies merge, direct hits of stars are very unlikely. This shouldn’t be surprising, considering how small the fraction of the area filled by stars in a galaxy is. For the solar neighbourhood we typically have 20 stars/pc3 and the radius of each star is about 0.2Rsun on average. So the fractional a ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

... Lesson 1: Images ...
Online_Review
Online_Review

... An asteroid is an irregularly shaped celestial object made up of rock or metal. They are smaller than planets and have irregular shapes rather than spherical shapes. A comet is a celestial object made up of ice, rock, and dust that has a very long orbit around the sun. As they move closer to the sun ...
Our Universe—Infinite and Eternal: Its Physics
Our Universe—Infinite and Eternal: Its Physics

... We model a spiral galaxy simply. We model it as a spherical central bulge surrounded by a thin flat disk of stars and gas that revolves about the central bulge. Surrounding both the disk and the bulge is a diffuse spherical halo. The calculation of the dynamics resulting from the gravitation of the th ...
Chapter 16 - Follow “Ironmtn.wordpress.com”
Chapter 16 - Follow “Ironmtn.wordpress.com”

... c. have less gravitational pull than that found on any planet. d. usually have active volcanoes. e. have been found orbiting all planets except for Mercury and Venus. Ans: e Link To: The Formation of the Solar System Difficulty Level: Easy 11. The composition of the Earth’s Moon is most like ...
Lecture Notes – Galaxies
Lecture Notes – Galaxies

... Galaxies were first systematically categorized by Edwin Hubble who in 1929 classified them according to shape: the Hubble Classification Scheme or Tuning Fork Diagram Elliptical galaxies (‘Early type’) E0 – E7 (0 spherical, 7 most distorted): S0 These galaxies are intermediate between E0 and Sa – th ...
File - Mr. Pelton Science
File - Mr. Pelton Science

... collide to form strangely shaped galaxies or galaxies with more than one nucleus (Andromeda) ...
American Scientist
American Scientist

... not to be the dominant outcome of planet formation and it may be exerting a provincial influence on our theoretical ideas. In seeking to map out the universe, we find ourselves to be the exception rather than the norm. An intriguing idea, suggested during a recent conference on Kepler exoplanets by ...
FREE Sample Here
FREE Sample Here

... 2 percent of this material into heavier elements, including all the elements of which we and Earth are made. Stars expel this material through winds and explosions, and the galaxy recycles it into new generations of stars. When a new star system forms, it therefore contains the ingredients needed to ...
Galaxy Notes
Galaxy Notes

... theories state that much smaller objects such as globular clusters formed first. These objects then merged to form galaxies. According to top-down theories, large objects such as galaxies and clusters of galaxies formed first. The smaller groups of stars then formed within them. But all big bang the ...
Paper
Paper

... mass MJ = (RT/ρG)3/2 ρ decreases below a solar mass as the temperature of the universe decreases, but this requires hundreds of millions of years rather than only a few million years by the present theory. Recent observations suggest that stars, galaxies, and even galaxy clusters existed at the earl ...
Chapter 2: The Solar System and Beyond
Chapter 2: The Solar System and Beyond

... The Lunar Cycle The phase of the Moon that you see on any given night depends on the relative positions of the Moon, the Sun, and Earth in space. These positions change because the Moon is continually revolving around Earth as Earth revolves around the Sun. It takes the Moon about one month to go th ...
Century-Long Monitoring of Solar Irradiance and Earth`s Albedo
Century-Long Monitoring of Solar Irradiance and Earth`s Albedo

... The GSO space environment is not “clean”. Surfaces exposed to propellant, silicone, and/or exposed to the solar UV flux and ionizing radiation, change their reflective properties (Dever et al. 2012). Oxidation is a serious issue in low earth orbit (LEO) where oxygen densities are 105−6 cm−3 in typic ...
Life on Our Evolving Planet slides
Life on Our Evolving Planet slides

... organisms, ecosystems, and even astronauts How did a giant cloud of cold dilute gas and dust evolve into astronauts in a spacecraft orbiting a planet orbiting a star? The short answer is when energy flows, complexity grows. The fact is that the solid Earth, hydrosphere, atmosphere, and biosphere hav ...
Satellites
Satellites

... years of taking pictures in deep space. As it continues to orbit Earth at 17,000 miles per hour, the Hubble’s reflecting telescopes, highpowered cameras, sensors, and other tools act as “eyes” to the universe. In its first twenty years, these eyes have recorded more than 45 terabytes of data, which ...
Cosmic Hide and Seek: the Search for the Missing
Cosmic Hide and Seek: the Search for the Missing

... many of their observations (2). Scientists also realize that the existence of some unseen mass would also support theories regarding the structure of the universe (3). Today, scientists are searching for the mysterious dark matter not only to explain the gravitational motions of galaxies, but also t ...
The Sun`s journey through the local interstellar medium: the
The Sun`s journey through the local interstellar medium: the

... stars near the Sun, indicates that sometime in the late Quaternary the Sun, which has been moving through the very low density region known as the Local Bubble, encountered the cluster of local interstellar clouds (CLIC) flowing away from the direction of the Scorpius-Centaurus Association (Frisch, ...
L. Moustakas
L. Moustakas

... ~50% of jk galaxies would be missed by R-limit, but not by z-limit The implied X-ray and (uncorrected) UV SFRr are comparable The pure AGN fraction is similar; it may be higher for jk galaxies ...
Cosmology - Stockton University
Cosmology - Stockton University

... In the past, right after the Big Bang, if the average density were slightly larger or smaller we have and open or closed universe. At the beginning the density would have to be very close to the critical value (1 part in 1015); Otherwise a Big Crunch or Big Chill would have occurred long ago. ...
1. setting the scene 2. the cosmic dark ages and the first stars
1. setting the scene 2. the cosmic dark ages and the first stars

... Universe and make an educated guess as to its future destiny. This ‘standard model’ of cosmology is illustrated in Figure 1. Our Universe began 13.7 billion years ago, in an event whose popular name – the Big Bang – reflects our ignorance of its nature and cause. As the Universe expanded (and cooled ...
Fulltext
Fulltext

... The intense research of the Solar System in the last several decades draws a much more complicated picture. The current theory of the origin of the Solar System is that the Sun, together with the planets, was created from an interstellar cloud of gas and dust that went gravitationally unstable due t ...
Lecture7_2014_v2
Lecture7_2014_v2

... • Observed data (today) are most consistent with theory that all the planets formed out of the same cloud of gas at the same time • Some of the wide variety seen within the existing planets may be due to chance events like collisions • Discovery of planet-forming disks and actual planets around othe ...
Earth and spaces
Earth and spaces

... There are nine planets moving around the sun, the Earth is one of them. The sun and the nine planets make up the solar system. ...
< 1 ... 31 32 33 34 35 36 37 38 39 ... 215 >

Outer space



Outer space, or just space, is the void that exists between celestial bodies, including the Earth. It is not completely empty, but consists of a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium as well as electromagnetic radiation, magnetic fields, neutrinos, dust and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvin (K). Plasma with a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvin in the space between galaxies accounts for most of the baryonic (ordinary) matter in outer space; local concentrations have condensed into stars and galaxies. In most galaxies, observations provide evidence that 90% of the mass is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Data indicates that the majority of the mass-energy in the observable Universe is a poorly understood vacuum energy of space which astronomers label dark energy. Intergalactic space takes up most of the volume of the Universe, but even galaxies and star systems consist almost entirely of empty space.There is no firm boundary where space begins. However the Kármán line, at an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which was passed by the United Nations in 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights, followed by manned rocket launches. Earth orbit was first achieved by Yuri Gagarin of the Soviet Union in 1961 and unmanned spacecraft have since reached all of the known planets in the Solar System. Due to the high cost of getting into space, manned spaceflight has been limited to low Earth orbit and the Moon.Outer space represents a challenging environment for human exploration because of the dual hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is high.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report