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Distances in Space Vocabulary
Distances in Space Vocabulary

... represents another object (stars, planets, etc.) in space. Each object in space will not move thru space but expand with space like the raisins move away from each other as the dough rises. The raisins don’t move on their own thru the rising dough. ...
The Solar System
The Solar System

... Meteoroids  which  burn  up  in  the  atmosphere  of  a  space  body,  such  as  the  Earth,  prior  to  impacting  on   the  surface.   ...
SPACE QUIZ
SPACE QUIZ

... Match the words A, B, C and D in the table below with the missing words. telescope Astronomers use devices called …(i)………………… to allow them to observe different objects. These devices may be positioned on the Earth or on satellites (ii)…………………… in space. Astronomers observe galaxies distant (iii)……… ...
Our Place in Space
Our Place in Space

... planets orbited around it. Group 4: Astronomers finally learned that Earth is one of at least eight other planets that travel around the Sun. Group 5: The Sun is a star at the center of the Solar System. It isn’t the biggest or the brightest star in our galaxy, but it is the star closest to Earth. G ...
GO 1_ Early Theorieso Of Space And Technology
GO 1_ Early Theorieso Of Space And Technology

... • 1610 Galileo Galilei gave further proof looking through a telescope. ...
Chapter 13 Lesson 3 Notes
Chapter 13 Lesson 3 Notes

... Define universe and galaxy ...
Space Trivia Questions - Trivia Questions World
Space Trivia Questions - Trivia Questions World

... Scientists used various methods to estimate its age. These included methods such as measuring the composition of matter and energy density in the universe. Scientists also studied the oldest objects in space to help calculate its age. For example, they measured the age of some of the oldest known st ...
Light year - TeacherWeb
Light year - TeacherWeb

...  Light year – the distance light can travel in a year (9.5 trillion km or 5.88 trillion miles / year - that’s 12 “0”s!!!) Just for Interest:  Light travels about 300,000 km (186,000 miles) per second  The North Star is 431 light years from Earth  Our nearest star, Proxima Centauri, is 4.28 light ...
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... Because wavelengths expand with the universe, the wavelength of the black-body radiation increases with time and the temperature decreases. The temperature of the radiation changes as a-1 . Q: When a very distant gamma-ray burster sent its light out z = 8, was the radiation hot enough to melt ice? ...
MSci Projects
MSci Projects

... Magnetometers are one of the most popular and productive instruments used in space and planetary research since they are small, light, robust, and scientifically productive. We can use magnetic field data for studies ranging from basic plasma physics in space through to probing the interior structur ...
Celestial Objects
Celestial Objects

... a) red shiftshift- shift toward longer red wavelengths of energy showing that an object is moving AWAY from Earth 1) the farther away the galaxy, the greater the red shift 2) almost all galaxies show a red shiftshiftproof that the universe is expanding (Edwin Hubble was the first to realize this!) ...
Workshop Tutorials for Physics Solutions to MR12: Gravity and
Workshop Tutorials for Physics Solutions to MR12: Gravity and

... 1. The radius of the Earth is approximately 6,400 km. The International Space Station orbits at an altitude approximately 400 km above the Earth’s surface, or at a radius of around 6,800 km from the Earth’s centre. Hence the force of gravity experienced by the space station and its occupants is almo ...
mr12sol
mr12sol

... 1. The radius of the Earth is approximately 6,400 km. The International Space Station orbits at an altitude approximately 400 km above the Earth’s surface, or at a radius of around 6,800 km from the Earth’s centre. Hence the force of gravity experienced by the space station and its occupants is almo ...
Section 17.1 - CPO Science
Section 17.1 - CPO Science

... and all objects that are gravitationally bound to the sun. • The solar system is roughly divided into the inner planets (Mercury, Venus, Earth, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and ...
STARS In your textbook, read about the properties of the Sun and
STARS In your textbook, read about the properties of the Sun and

... 6. Stars on the main sequence produce energy by fusing hydrogen into----' 7. As a contracts, its rotation forces it into a disk shape with a hot condensed object at the center, which will become a new stsr. 8. During a the entire portion of the star is blown off in a massive explosion! What are Gala ...
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... 4. How big is the Earth? Is its radius 4241 km, 6371 km or 8763 km? [6371] 5. Say one of the Guide Laws NO REPEATS – THEY HAVE TO GIVE A NEW ONE 6. Say one of the Guide Laws 7. Say one of the Guide Laws 8. Name three Harry Potter Characters. 9. Recite the Promise 10. Recite the Promise 11. Name 6 di ...
Terms - HULK SCIENCE
Terms - HULK SCIENCE

... Planets inside the asteroid belt (terrestrial) Planets outside the asteroid belt (gas) A force determined by mass that holds objects in orbit Planets made of land (inner planets) Mercury, Venus, Earth, Mars Planets made of gas (outer planets) Jupiter, Saturn, Uranus, Neptune ...
ppt of lecture - July Lectures
ppt of lecture - July Lectures

... (3) Very uniform on large scales, but seeds of galaxy formation ...
6th Grade Review II - pams
6th Grade Review II - pams

... • The moon appears to go through phases, because one side is always lit. • The phases of the moon are: new, waxing crescent, first quarter, waxing gibbous, full, waning gibbous, last quarter, and waning crescent. ...
Diversity of Life Card Game
Diversity of Life Card Game

... This game is an excellent engagement activity for learners to begin thinking about our place in space and the relative sizes of objects in the universe. When facilitating this game, get participants to think. Strive to be “a guide on the side” by encouraging questions, asking your own questions, and ...
The Solar System - MHS-Integrated
The Solar System - MHS-Integrated

... elements from which stars and solar systems are built. ...
The most important questions to study for the exam
The most important questions to study for the exam

... situation of matter from space hitting the Earth and its atmosphere? • Space matter hits the Earth only at certain times each year in so-called meteor showers, with a wide range of particle sizes, some of which reaches the Earth's surface. • Matter is falling continuously onto the Earth and its atmo ...
384 kb
384 kb

... remarks. And “terraforming Mars may become an important topic as we learn more about the planet. Travelling to Mars is already under discussion at space agencies, but anything beyond Mars is not practical. As to travelling to planets around other stars… I do not see that as feasible.” Closer collabo ...
ASTR 2020, Spring 2015 Professor Jack Burns Final Exam
ASTR 2020, Spring 2015 Professor Jack Burns Final Exam

... 25. Earth and Venus both presumably had similar gases outgassed from their volcanoes. Explain how their atmospheres ended up so different. A: The main factor in this is that Venus is closer to the Sun than the Earth. This led to a runaway greenhouse effect. The runaway greenhouse effect evaporated a ...
Name_______________________Period_________Date
Name_______________________Period_________Date

...  The disk of dust and gas that formed the Sun and planets is known as the solar nebula.  Dense concentration at center became the Sun.  Temperature differed, Hotter at center and cooler at edges disk  Due to temp differences different compounds were able to condense depending on distance from Su ...
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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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