
Some physics and math…
... motion of the planets that we observe: a)Inner planets, Mercury and Venus, never seen at large angles from sun b)Outer planets, Mars, Jupiter, Saturn move slowly eastward (over weeks and months) but about once a year, reverse their motion, go west for a distance, then reverse again to move eastward ...
... motion of the planets that we observe: a)Inner planets, Mercury and Venus, never seen at large angles from sun b)Outer planets, Mars, Jupiter, Saturn move slowly eastward (over weeks and months) but about once a year, reverse their motion, go west for a distance, then reverse again to move eastward ...
Planetary motion: Let`s try this animation again! Venus, Mars http
... motion of the planets that we observe: a) Inner planets, Mercury and Venus, never seen at large angles from sun b) Outer planets, Mars, Jupiter, Saturn move slowly eastward (over weeks and months) but about once a year, reverse their motion, go west for a distance, then reverse again to move eastw ...
... motion of the planets that we observe: a) Inner planets, Mercury and Venus, never seen at large angles from sun b) Outer planets, Mars, Jupiter, Saturn move slowly eastward (over weeks and months) but about once a year, reverse their motion, go west for a distance, then reverse again to move eastw ...
Benchmark 1 Study Guide Answers 1. mMechanical: m-
... Radio telescopes receive radio waves emitted from objects in space; can be used any time of day in any weather Spectroscopes collect and separate light from stars into color bands & uses those bands to identify star elements Satellites are in orbit around Earth & use special instruments & telescopes ...
... Radio telescopes receive radio waves emitted from objects in space; can be used any time of day in any weather Spectroscopes collect and separate light from stars into color bands & uses those bands to identify star elements Satellites are in orbit around Earth & use special instruments & telescopes ...
Ontario Grade One Describe, using models or simulations, how the
... Visualize and describe the size, shape, and motions of the solar system, and the place of the Earth within it. Describe the origin and evolution of the Earth and other objects in the solar system, and identify the fundamental forces and processes involved. Compare the Earth with other objects in the ...
... Visualize and describe the size, shape, and motions of the solar system, and the place of the Earth within it. Describe the origin and evolution of the Earth and other objects in the solar system, and identify the fundamental forces and processes involved. Compare the Earth with other objects in the ...
Stellar Evolution
... The Big Bang • Tremendous explosion started the expansion of the universe • All of the matter and energy of the universe was contained at one point ...
... The Big Bang • Tremendous explosion started the expansion of the universe • All of the matter and energy of the universe was contained at one point ...
KS2 Earth and Space
... huge the distances involved are. Pupils will learn about how gravity keeps our solar system together. We then focus in to the Earth with pupils exploring the rotation of the Earth, day, night and shadows by getting hands-on with globes and torches. Pupils can see at first hand why it is that differe ...
... huge the distances involved are. Pupils will learn about how gravity keeps our solar system together. We then focus in to the Earth with pupils exploring the rotation of the Earth, day, night and shadows by getting hands-on with globes and torches. Pupils can see at first hand why it is that differe ...
Some facts and concepts to have at your fingertips.
... • The Sun will eventually become a white dwarf star, a bit larger than the diameter of the Earth. It will not explode as a supernova. • The visible portion of the Milky Way Galaxy is about 75,000 lt-yrs in diameter. The solar system is about 26,000 lt-yrs from the center of the Galaxy. • For galaxie ...
... • The Sun will eventually become a white dwarf star, a bit larger than the diameter of the Earth. It will not explode as a supernova. • The visible portion of the Milky Way Galaxy is about 75,000 lt-yrs in diameter. The solar system is about 26,000 lt-yrs from the center of the Galaxy. • For galaxie ...
File
... – Our solar system is full of planets, moons, asteroids and comets, all of which revolve around the Sun at the center. – When a star forms from a nebula, gravity pulls most of the material into the new star, but some may also clump together to form objects in a solar system. ...
... – Our solar system is full of planets, moons, asteroids and comets, all of which revolve around the Sun at the center. – When a star forms from a nebula, gravity pulls most of the material into the new star, but some may also clump together to form objects in a solar system. ...
CK12- Study of Space by the EM Spectrum Student Name: ______
... Write a one sentence summary of the article that highlights the most important concepts. ...
... Write a one sentence summary of the article that highlights the most important concepts. ...
Important fact!
... • The sun produces large amounts of solar radiation. • Radiation in space can damage the astronaut’s DNA. • Damaged DNA increases the risk of cancer. • Radiation is especially high during solar flares. ...
... • The sun produces large amounts of solar radiation. • Radiation in space can damage the astronaut’s DNA. • Damaged DNA increases the risk of cancer. • Radiation is especially high during solar flares. ...
Eye on the Sky - Sci-Port
... Big Bang: a theory that deduces a cataclysmic birth of the universe (big bang) from the observed expansion of the universe, cosmic background radiation, abundance of the elements, and the laws of physics. Infrared: the part of the invisible spectrum that is contiguous to the red end of the visible s ...
... Big Bang: a theory that deduces a cataclysmic birth of the universe (big bang) from the observed expansion of the universe, cosmic background radiation, abundance of the elements, and the laws of physics. Infrared: the part of the invisible spectrum that is contiguous to the red end of the visible s ...
Stars & Galaxies
... Temp just right because of sun Gravity force is just right Single moon provide for gentle tides Atmosphere clear so sun can penetrate Ozone layer protects us from UV Material that accreted had minerals and water to form the Earth’s crust ...
... Temp just right because of sun Gravity force is just right Single moon provide for gentle tides Atmosphere clear so sun can penetrate Ozone layer protects us from UV Material that accreted had minerals and water to form the Earth’s crust ...
Galaxies - schoolphysics
... gravity of the Earth. However if you jump up very fast - 40000 km/hour (25000 miles/hour) then you will never come down. You have reached the ESCAPE VELOCITY of the Earth Now the pull of gravity of a Black Hole is so huge that its escape velocity is as big as the speed of light. That’s why it’s blac ...
... gravity of the Earth. However if you jump up very fast - 40000 km/hour (25000 miles/hour) then you will never come down. You have reached the ESCAPE VELOCITY of the Earth Now the pull of gravity of a Black Hole is so huge that its escape velocity is as big as the speed of light. That’s why it’s blac ...
Final Exam Practice Part I
... 26. When a massive, dying star blows itself apart, if the remaining mass is less than three times the mass of the sun, the leftover material will form a ______. 28. Cosmologists think the material in our bodies was once part of a massive star. Explain how it went from a star to our bodies. 29. Descr ...
... 26. When a massive, dying star blows itself apart, if the remaining mass is less than three times the mass of the sun, the leftover material will form a ______. 28. Cosmologists think the material in our bodies was once part of a massive star. Explain how it went from a star to our bodies. 29. Descr ...
11.3.1 Grade 6 Standard 4 Unit Test Astronomy Multiple Choice 1
... Betelgeuse Polaris (North Star) Sirius (Dog Star) ...
... Betelgeuse Polaris (North Star) Sirius (Dog Star) ...
Name________________ Astronomy I cans 1. What is the Big Bang
... The energy and matter expanded like a balloon ...
... The energy and matter expanded like a balloon ...
Glossary Annual Motion – the Earth`s orbital motion around the sun
... Equinox – the two days in which the day on earth is equally divided between 12hrs of sunlight and darkness, caused as the sun passes the celestial equator at one of two points – on or around the 21st of March and 23rd of September Galaxy – a spiral island of stars in space – our galaxy is called th ...
... Equinox – the two days in which the day on earth is equally divided between 12hrs of sunlight and darkness, caused as the sun passes the celestial equator at one of two points – on or around the 21st of March and 23rd of September Galaxy – a spiral island of stars in space – our galaxy is called th ...
Bang To Sol - Transcript
... of the way out on one of the spiral arms of the Milky Way. Our sun and its planets condensed under the pressure of gravity until the sun was hot and dense enough to light its own nuclear fires. The inner planets are small and rocky with heavy elements while the outer planets tend to be large gas gia ...
... of the way out on one of the spiral arms of the Milky Way. Our sun and its planets condensed under the pressure of gravity until the sun was hot and dense enough to light its own nuclear fires. The inner planets are small and rocky with heavy elements while the outer planets tend to be large gas gia ...
The Solar System - Teacher Bulletin
... The Solar System includes: The sun The eight official planets At least three draft planets More than 130 satellites of the planets A large number of small bodies The interplanetary medium. ...
... The Solar System includes: The sun The eight official planets At least three draft planets More than 130 satellites of the planets A large number of small bodies The interplanetary medium. ...
Key Words – Year 7 - Space Word Meaning axis Imaginary vertical
... The path that a planet takes around the Sun, or the path that a moon or satellite takes around a planet. ...
... The path that a planet takes around the Sun, or the path that a moon or satellite takes around a planet. ...
Using the Earth Science Reference Table: Inferred Properties of the
... Using the Earth Science Reference Table: Inferred Properties of the Earth’s Interior Directions: Use the “Inferred Properties of the Earth’s Interior” diagram on page 10 in the Earth Science Reference Tables to answer the following questions. Some questions may require you to use your notes or textb ...
... Using the Earth Science Reference Table: Inferred Properties of the Earth’s Interior Directions: Use the “Inferred Properties of the Earth’s Interior” diagram on page 10 in the Earth Science Reference Tables to answer the following questions. Some questions may require you to use your notes or textb ...
Place the following objects in order from largest to smallest:
... are located around individual stars in a galaxy. Our solar system is located on the outer edge of a spiral galaxy called the Milky Way. ...
... are located around individual stars in a galaxy. Our solar system is located on the outer edge of a spiral galaxy called the Milky Way. ...
Chapter 7: An Extraordinary Beginning: The Hadean and Archean
... mostly of silicate minerals and metals, so are much denser o The outer or Jovian planets (Jupiter, Saturn, Uranus, and Neptune) are composed of gas and are larger than the terrestrial planets As the planets were coalescing, so was the sun o It reached the temperatures and pressures at which hydrog ...
... mostly of silicate minerals and metals, so are much denser o The outer or Jovian planets (Jupiter, Saturn, Uranus, and Neptune) are composed of gas and are larger than the terrestrial planets As the planets were coalescing, so was the sun o It reached the temperatures and pressures at which hydrog ...
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.