red giant - Teacher Pages
... collapse inward c. Supergiant stars form supernovas d. Most of the stars in the Milky Way, which are relatively small, will end their lives as white dwarfs ...
... collapse inward c. Supergiant stars form supernovas d. Most of the stars in the Milky Way, which are relatively small, will end their lives as white dwarfs ...
The Size of the Solar System
... Using the information from table 2, draw a scale picture of your objects on plain white paper. If you have the Sun, you may need to tape some paper together. If your object is a moon, you should include your sketch on the same paper as the planet it orbits. Label the picture. Decide which end of the ...
... Using the information from table 2, draw a scale picture of your objects on plain white paper. If you have the Sun, you may need to tape some paper together. If your object is a moon, you should include your sketch on the same paper as the planet it orbits. Label the picture. Decide which end of the ...
The Solar System Sections 16.1-16.8
... Formation of the Solar System • Began with a large, swirling volume of cold gases and dust – a rotating solar nebula • Contracted under the influence of its own gravity – into a flattened, rotating disk • Further contraction produced the protosun and eventually accreted the planets • As particles m ...
... Formation of the Solar System • Began with a large, swirling volume of cold gases and dust – a rotating solar nebula • Contracted under the influence of its own gravity – into a flattened, rotating disk • Further contraction produced the protosun and eventually accreted the planets • As particles m ...
unit 2 test – the solar system: planets
... 43. ______ Has the coolest average temperature 44. ______ this planet radiates almost no internal heat 45. ______Contains the Great Dark Spot 46. ______Titan is its biggest moon 47. ______These TWO planets do not have any moons (yes, fill in TWO bubbles) 48. ______Has the warmest average temperature ...
... 43. ______ Has the coolest average temperature 44. ______ this planet radiates almost no internal heat 45. ______Contains the Great Dark Spot 46. ______Titan is its biggest moon 47. ______These TWO planets do not have any moons (yes, fill in TWO bubbles) 48. ______Has the warmest average temperature ...
DO IT YOURSELF SIMPLE TEMPLATE FORMAT
... See how the sun wobbles a bit. Why is that? The sun has an orbit too, but why is it so much smaller than the planet's orbit? You may have answered that the sun is more massive than the planet. To see if this matters, make the sun's mass 1000. How does that change the wobble? Why? Now make the sun's ...
... See how the sun wobbles a bit. Why is that? The sun has an orbit too, but why is it so much smaller than the planet's orbit? You may have answered that the sun is more massive than the planet. To see if this matters, make the sun's mass 1000. How does that change the wobble? Why? Now make the sun's ...
Killer Asteroids
... orbits around the Sun. It is believed that Trojans have been ‘locked’ in their orbits since early in the formation of the Solar System. To date, astronomers have found over 5 000 Trojans in Jupiter’s orbit, and only one in Earth’s orbit (2010 TK7). Beyond the Main Asteroid Belt, there are objects th ...
... orbits around the Sun. It is believed that Trojans have been ‘locked’ in their orbits since early in the formation of the Solar System. To date, astronomers have found over 5 000 Trojans in Jupiter’s orbit, and only one in Earth’s orbit (2010 TK7). Beyond the Main Asteroid Belt, there are objects th ...
solar system
... •The terrestrial worlds have weak magnetic fields, if any; •the jovian worlds all have strong magnetic fields. •The terrestrial worlds have only three moons among them; •the jovian worlds have many moons each, no two of them alike and none of them like our own. •Furthermore, all the jovian planets h ...
... •The terrestrial worlds have weak magnetic fields, if any; •the jovian worlds all have strong magnetic fields. •The terrestrial worlds have only three moons among them; •the jovian worlds have many moons each, no two of them alike and none of them like our own. •Furthermore, all the jovian planets h ...
Level 1 Solar system, Planets, Sun, Asteroid belt, Kuipler belt and
... 2. Our solar system is made up of the sun and everything that travels around it. This includes eight planets and their natural satellites such as Earth's moon; dwarf planets such as Pluto and Ceres; asteroids; comets and meteoroids 3. The sun is the center of our solar system. It contains almost all ...
... 2. Our solar system is made up of the sun and everything that travels around it. This includes eight planets and their natural satellites such as Earth's moon; dwarf planets such as Pluto and Ceres; asteroids; comets and meteoroids 3. The sun is the center of our solar system. It contains almost all ...
Solar System Study Guide 1
... Mars is self-sterilizing. Biologists believe the Sun’s ultraviolet radiation, the dryness of the soil, and the soil chemistry prevent formation of living organisms in the soil. Mars has shown itself to be the most Earth-like of all of the planets. It has polar ice caps that grow and recede wit ...
... Mars is self-sterilizing. Biologists believe the Sun’s ultraviolet radiation, the dryness of the soil, and the soil chemistry prevent formation of living organisms in the soil. Mars has shown itself to be the most Earth-like of all of the planets. It has polar ice caps that grow and recede wit ...
Name the terms - St John Brebeuf
... 1. The patterns in the sky that are not official constellations are called ____________________. 2. The Aquila, Cassiopeia, and Orion are all examples of ____________________. 3. A ______ is a star in its final phases of life, when it explodes to many times its original size. 4. Objects that are lo ...
... 1. The patterns in the sky that are not official constellations are called ____________________. 2. The Aquila, Cassiopeia, and Orion are all examples of ____________________. 3. A ______ is a star in its final phases of life, when it explodes to many times its original size. 4. Objects that are lo ...
Use the Force
... forces, inertia and gravity. The sun’s gravity pulls the planets inward and the inertia of the moving planets pulls the planets in a perpendicular direction (see image). Neither force is great enough to overcome the other. Therefore, the planets are locked in orbit around our sun. ...
... forces, inertia and gravity. The sun’s gravity pulls the planets inward and the inertia of the moving planets pulls the planets in a perpendicular direction (see image). Neither force is great enough to overcome the other. Therefore, the planets are locked in orbit around our sun. ...
Creature Adaptations for the Universe
... mantle, which is made of liquid molecular hydrogen and helium. Below that, the inner mantle is made of liquid metallic hydrogen. It is very hot - more than 54,000 degrees Fahrenheit. Saturn, Uranus, and Neptune are gas giants similar to Jupiter. They are made of hydrogen and helium, mostly in liqui ...
... mantle, which is made of liquid molecular hydrogen and helium. Below that, the inner mantle is made of liquid metallic hydrogen. It is very hot - more than 54,000 degrees Fahrenheit. Saturn, Uranus, and Neptune are gas giants similar to Jupiter. They are made of hydrogen and helium, mostly in liqui ...
Astronomy Library wk 4 .cwk (WP)
... As far as the motion of the planets is concerned, Tycho’s system is equivalent to Copernicus’. Tycho’s model soon replaced Ptolemy’s as the most ...
... As far as the motion of the planets is concerned, Tycho’s system is equivalent to Copernicus’. Tycho’s model soon replaced Ptolemy’s as the most ...
Interactive Tutorial Activities in ASTR 310
... discovered using one of three methods: measuring Doppler shifts B) b has a smaller diameter, takes the same amount of of the star, observing dips in the lightcurve of the star or seeing C) a and b are the same age, the age of the Moon time as a to orbit D) a is older than b because a has had many fl ...
... discovered using one of three methods: measuring Doppler shifts B) b has a smaller diameter, takes the same amount of of the star, observing dips in the lightcurve of the star or seeing C) a and b are the same age, the age of the Moon time as a to orbit D) a is older than b because a has had many fl ...
AP Physics - Universal Gravitation
... 5.A projectile is launched from the surface of a planet (mass = M, radius = R). What minimum launch speed is required if the projectile is to rise to a height of 2R above the surface of the planet? Disregard any dissipative effects of the atmosphere. A) B) C) D) E) 6. What is the kinetic energy of ...
... 5.A projectile is launched from the surface of a planet (mass = M, radius = R). What minimum launch speed is required if the projectile is to rise to a height of 2R above the surface of the planet? Disregard any dissipative effects of the atmosphere. A) B) C) D) E) 6. What is the kinetic energy of ...
Jupiter – key facts Largest and most massive planet in the Solar
... surface indicates that it is an ancient surface, not subject to renewal by erupFons from an interior mantle. The galilean satellites are believed to have formed in a disc of gas and rocks that su ...
... surface indicates that it is an ancient surface, not subject to renewal by erupFons from an interior mantle. The galilean satellites are believed to have formed in a disc of gas and rocks that su ...
Visit www.sciencea-z.com www.sciencea-z.com
... of wonder and perspective. They can ponder and appreciate Earth’s crucial position in our solar system, which makes this planet such an ideal place for us to live. Students may also consider how small our entire world is compared to some of our fellow planets, the Sun, and the vastness of space. For ...
... of wonder and perspective. They can ponder and appreciate Earth’s crucial position in our solar system, which makes this planet such an ideal place for us to live. Students may also consider how small our entire world is compared to some of our fellow planets, the Sun, and the vastness of space. For ...
Lecture14: Solar System Debris
... composed of ice and rock. • Its radius and mass are not accurately known - it is so small even HST does not view it well. Pluto-Charon binary by HST: they are apart by only 0.9” ...
... composed of ice and rock. • Its radius and mass are not accurately known - it is so small even HST does not view it well. Pluto-Charon binary by HST: they are apart by only 0.9” ...
Probeseiten 2 PDF
... of a century, no fewer than five new planets (including Uranus) had been discovered – and the Himmelpolizei would undoubtedly find more. But that proved easier said than done. A fifth object (Astraea) was not discovered between the orbits of Mars and Jupiter until December 1845. Neither Herschel, Pi ...
... of a century, no fewer than five new planets (including Uranus) had been discovered – and the Himmelpolizei would undoubtedly find more. But that proved easier said than done. A fifth object (Astraea) was not discovered between the orbits of Mars and Jupiter until December 1845. Neither Herschel, Pi ...
The story of Mercury and Vulcan, as told by Einstein The
... The story of Mercury and Vulcan, as told by Einstein By C. Pantelidou (ICCUB) ...
... The story of Mercury and Vulcan, as told by Einstein By C. Pantelidou (ICCUB) ...
THE SOLAR SYSTEM An Overview Astronomy is the study of the
... in the center representing the sun. The planets all orbit the sun on a relatively thin plane with the exception of Pluto. Pluto's orbit takes it well above and below the plane of the solar system. Time is expressed as either sidereal or synodic. A sidereal period for a planet would be the time betwe ...
... in the center representing the sun. The planets all orbit the sun on a relatively thin plane with the exception of Pluto. Pluto's orbit takes it well above and below the plane of the solar system. Time is expressed as either sidereal or synodic. A sidereal period for a planet would be the time betwe ...
Chapter 7: Our Planetary System Chapter 8: Formation of the Solar
... What are the general characteristics of the various bodies in the solar system? What can we learn by comparing the planets to one another? What features of our solar system provide clues to how it formed? What is Mike Brown’s argument against Pluto and Eris being classified as planets? What are the ...
... What are the general characteristics of the various bodies in the solar system? What can we learn by comparing the planets to one another? What features of our solar system provide clues to how it formed? What is Mike Brown’s argument against Pluto and Eris being classified as planets? What are the ...
SEM 1.4_Astronomy
... The Earth’s moon is a rocky satellite that is about one-quarter the diameter of the Earth and one-eighth the mass of the Earth. It is highly cratered and it lacks an atmosphere. Therefore, there is no erosion to eliminate traces of impacts from space objects. The Moon revolves around the Earth once ...
... The Earth’s moon is a rocky satellite that is about one-quarter the diameter of the Earth and one-eighth the mass of the Earth. It is highly cratered and it lacks an atmosphere. Therefore, there is no erosion to eliminate traces of impacts from space objects. The Moon revolves around the Earth once ...
Definition of planet
The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.