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Models of the Solar System
Models of the Solar System

... circle that has been stretched out along one axis. Most planets’ orbits are nearly circular, and so are only slightly elliptical. • The plane of Earth’s orbit is called the ecliptic plane. ...
Before Humankind - Salem State University
Before Humankind - Salem State University

... with a flowing forth of trillions-of-degrees hot energy and matter moving faster than the speed of light. As this matter and energy expanded, it cooled and differentiated into different types of energy and matter. These changes are called “phase changes.” This early energy and matter was in the form ...
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PSSA Prep Earth History Jeopardy
PSSA Prep Earth History Jeopardy

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Jeopardy Review Earth Science

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Astronomyunitbingo
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... caused by the Moon’s gravitational force on Earth precession ...
Study Guide - James E. Neff
Study Guide - James E. Neff

... equator. The minimum orbital velocity is about 8 km/s. What happens if you try to launch into an orbit slower or faster than this speed? Why are astronauts more accurately described to be "in freefall" rather than "weightless" or "zero gravity"? Earth orbits the sun in close to a circular orbit at 3 ...
Introduction to the Solar System
Introduction to the Solar System

... Ex) Mercury is closer to sun (.39 AU) ...
Science CRCT Jeopardy 1
Science CRCT Jeopardy 1

... sunlight, the climate gets colder. B. Climate is the average of the conditions of the atmosphere over many years. C. Weather is the average of the atmosphere over ...
Astronomy Vocabulary - Thomas C. Cario Middle School
Astronomy Vocabulary - Thomas C. Cario Middle School

... 28. Light year (381): The distance that light travels in one year (9.5 Trillion km) . The nearest star to Earth, besides the Sun, is called Proxima Centauri and is 4.24 light years away. 29. Telescope (412): Two types: Optical and Radio. Optical telescopes are used to collect light and form images ( ...
TYPES OF PLANETS AND STARS
TYPES OF PLANETS AND STARS

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Lecture 1 - Department of Physics and Astronomy
Lecture 1 - Department of Physics and Astronomy

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Regents Earth Science – Unit 5: Astronomy
Regents Earth Science – Unit 5: Astronomy

... the Sun produces energy by the process of nuclear fusion in its core the sun’s outer atmosphere “the corona” can be seen during a total solar eclipse the Sun has sunspots (cooler, dark in color) - spots associated with the its magnetic field these increase and decrease in a cyclic pattern the sun al ...
15 September: Basic properties of the Sun
15 September: Basic properties of the Sun

... increases rapidly from very low values in interplanetary space to very high values, and it becomes opaque within an interval of altitude of about 200 kilometers (out of 696,000) ...
Internet Space Scavenger Hunt
Internet Space Scavenger Hunt

... 28.What determines how large a star will become? The amount of matter that is available for star formation in the nebula determines how large a star becomes. 29.Will a star’s lifecycle be shorter or longer if its mass is greater? Shorter 30.Black holes have an enormous ________________ pull. Gravita ...
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Which of the following is the best description of an Sc galaxy? A) a

... c. Molecular clouds d. Reflection nebulae e. Dark nebulae The presence of forbidden lines in the spectra of emission nebula indicates that the a. nebula has a very high temperature. b. nebula contains large amounts of hydrogen. c. gas in the nebula has a very low density. d. dust in the nebula is co ...
Intro ES Sense of Time and Space Test Key
Intro ES Sense of Time and Space Test Key

... 46. (4 pts.) State two differences between inner and outer planets besides their distance from the sun.! inner planets ...
God, science and you – 2 The solar system
God, science and you – 2 The solar system

... • The last slide showed how big the solar system is. But the universe is much, much bigger. • To travel from here to Neptune, light takes 4 hours. We say that Neptune is 4 light-hours away. • The nearest star apart from the sun, Proxima Centauri, is 4 light-years away. • The nearest spiral galaxy ot ...
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... A natural object that orbits around another object in space.  Sentence: The earth is a satellite of the sun. ...
Today`s Powerpoint
Today`s Powerpoint

... Further subdivision: BO - B9, GO - G9, etc. GO hotter than G9. Sun is a G2. ...
Worldly Wise 3000
Worldly Wise 3000

... Earth. Four smaller planets are closer to the sun. They are Mars, Earth, Venus, and Mercury. All of them are made of solid rock. Mercury, which is the closest to the sun, is very hot. The temperature there can rise to almost twice as high as the top setting on an oven. About four hundred years ago, ...
Episode1: Overview of the radio serial
Episode1: Overview of the radio serial

... of the nature of the Universe. It is not designed to be a popular account of the development of astronomy as a scientific discipline and its impact on our understanding of the cosmos. Since the treatment is not rigorous, many details are not included. The script has to be developed along the outline ...
Celestial Bodies (Mike Stroppa) - Powerpoint
Celestial Bodies (Mike Stroppa) - Powerpoint

... • Consume their hydrogen in about 10 billion years • (Our sun is about 5 billion years old) • Once H is burned up, energy production stops • Core collapses due to gravity • Increased T = increased pressure ...
Cosmic Survey PowerPoint
Cosmic Survey PowerPoint

... galaxies are among the most ancient and distant objects we can see in the sky. The light from them has taken about 10 billion years to reach us. So they were born long before the Sun. On the other hand, the Hubble deep field galaxies are young! Because light takes time to travel, telescope images of ...
PPT Slides
PPT Slides

... The Big Bang • The Universe as we know it began 13.7 billion years ago in an explosion so powerful that space itself was propelled outwards. • Even atoms could not exist in this hot fireball. • 380,000 years after the bang, H atoms formed • 200 Million years later, the first stars formed How do w ...
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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.
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