Teacher Guide pages
... An example of a celestial object that challenges the accepted classification system is Jupiter. In its composition Jupiter appears more like a star than a planet: it consists of a shell of gaseous hydrogen, almost 60,000 km (37,000 miles) thick, overlying a layer of liquid metal hydrogen formed by h ...
... An example of a celestial object that challenges the accepted classification system is Jupiter. In its composition Jupiter appears more like a star than a planet: it consists of a shell of gaseous hydrogen, almost 60,000 km (37,000 miles) thick, overlying a layer of liquid metal hydrogen formed by h ...
Phys 214. Planets and Life
... Many brown dwarfs in constellation Orion. Infrared image of a Jupiter-size planet orbiting a brown dwarf. Brown dwarfs are substellar objects with insufficient mass to sustain nuclear fusion in their cores. They have higher surface temperatures than planets and masses between 10to 80 times that of J ...
... Many brown dwarfs in constellation Orion. Infrared image of a Jupiter-size planet orbiting a brown dwarf. Brown dwarfs are substellar objects with insufficient mass to sustain nuclear fusion in their cores. They have higher surface temperatures than planets and masses between 10to 80 times that of J ...
Tackling the 5th Grade Science Test
... Key terms to know and remember: 1. Planets revolve around the sun in elliptical orbits. Some of the planets have moons and/or debris that orbit them. Comets, asteroids and meteoroids orbit the sun. 2. Asteroids are metallic, rocky bodies that orbit the sun but are too small to be classified as a pla ...
... Key terms to know and remember: 1. Planets revolve around the sun in elliptical orbits. Some of the planets have moons and/or debris that orbit them. Comets, asteroids and meteoroids orbit the sun. 2. Asteroids are metallic, rocky bodies that orbit the sun but are too small to be classified as a pla ...
NATS1311_091108_bw - The University of Texas at Dallas
... Ecclesiastical version - occurs when a season has four full Moons, rather than the usual three - the third is the Blue Moon - found only in February, May, August, and November, one month before the next equinox or solstice. The result of following rules laid down as part of the Gregorian calendar re ...
... Ecclesiastical version - occurs when a season has four full Moons, rather than the usual three - the third is the Blue Moon - found only in February, May, August, and November, one month before the next equinox or solstice. The result of following rules laid down as part of the Gregorian calendar re ...
Introduction To Global Positioning System and other Geo
... How fast are you moving and in what direction? In what direction should you go to get to some other specific location How long would it take at your speed to get there? Where have you been? ...
... How fast are you moving and in what direction? In what direction should you go to get to some other specific location How long would it take at your speed to get there? Where have you been? ...
The Sky Above: A First Look
... Students can research and report on one part of the solar system. Their report could focus on the sun, a planet, or a moon such as Jupiter's Io or Saturn's Miranda. Students can work in teams. As part of their reports, they can make posters and/or construct models of their subjects. Each student or ...
... Students can research and report on one part of the solar system. Their report could focus on the sun, a planet, or a moon such as Jupiter's Io or Saturn's Miranda. Students can work in teams. As part of their reports, they can make posters and/or construct models of their subjects. Each student or ...
Unit 12: The Formation of the Earth
... Brahmins of India believed that the earth was eternal, as did Aristotle. In early JudeoChristian cultures, estimates of the age of the solar system were based on the Bible. The traditional Jewish calendar starts from 3760 BCE, which is taken to be a date for the creation of the earth. In 1650, Angli ...
... Brahmins of India believed that the earth was eternal, as did Aristotle. In early JudeoChristian cultures, estimates of the age of the solar system were based on the Bible. The traditional Jewish calendar starts from 3760 BCE, which is taken to be a date for the creation of the earth. In 1650, Angli ...
Jupiter (a.k.a. "Jove") was the King of the Roman Gods and the
... the tops of clouds high in its atmosphere. Jupiter has high speed winds that whip by at more than 400 mph! These winds are trapped in the planet's wide bands of latitude. Each band has a slightly different chemical make-up and temperature from the others. This gives it a colour which is different fr ...
... the tops of clouds high in its atmosphere. Jupiter has high speed winds that whip by at more than 400 mph! These winds are trapped in the planet's wide bands of latitude. Each band has a slightly different chemical make-up and temperature from the others. This gives it a colour which is different fr ...
Solar system and eclipse
... 5. There's a recurring myth that pregnant women can't go outside during an eclipse. Astronomers from the Griffith Observatory in LA say they get dozens of calls about it when an eclipse happens, even though it seems irrational. But if one of your friends is pregnant, don't worry, you can invite them ...
... 5. There's a recurring myth that pregnant women can't go outside during an eclipse. Astronomers from the Griffith Observatory in LA say they get dozens of calls about it when an eclipse happens, even though it seems irrational. But if one of your friends is pregnant, don't worry, you can invite them ...
here
... • The Solar System refers to the Sun and the surrounding planets, asteroids, comets, etc. • The scale of things: – It takes light about 11 hours to travel across the Solar system. This is 0.001265 years. – It takes light about 4.3 years to travel from the Sun to the nearest star. – It takes light ab ...
... • The Solar System refers to the Sun and the surrounding planets, asteroids, comets, etc. • The scale of things: – It takes light about 11 hours to travel across the Solar system. This is 0.001265 years. – It takes light about 4.3 years to travel from the Sun to the nearest star. – It takes light ab ...
doc
... S4E1. Students will compare and contrast the physical attributes of stars, star patterns, and planets. S4E2. Students will model the position and motion of the earth in the solar system and will explain the role of relative position and motion in determining sequence of the phases of the moon. Under ...
... S4E1. Students will compare and contrast the physical attributes of stars, star patterns, and planets. S4E2. Students will model the position and motion of the earth in the solar system and will explain the role of relative position and motion in determining sequence of the phases of the moon. Under ...
the earth in space - North Salem Schools Teachers Module
... B. The movements of planets across the nighttime sky is not uniform 1. The reason planets have non-uniform motion is that they really are moving in space - stars only look like they’re moving 2. Planets rotate while they revolve a. we know this because features on the planets surface vary in a predi ...
... B. The movements of planets across the nighttime sky is not uniform 1. The reason planets have non-uniform motion is that they really are moving in space - stars only look like they’re moving 2. Planets rotate while they revolve a. we know this because features on the planets surface vary in a predi ...
Study Notes Lesson 13 Gravitational Interactions
... Near the surface of Earth, g = 9.8 m/s2. The g is a vector quantity, for it has both magnitude (strength) and direction. Gravitational field vector g and acceleration due to gravity g have the same magnitude and their units are equivalent: m/s2. The numerical value of g at Earth’s surface depends on ...
... Near the surface of Earth, g = 9.8 m/s2. The g is a vector quantity, for it has both magnitude (strength) and direction. Gravitational field vector g and acceleration due to gravity g have the same magnitude and their units are equivalent: m/s2. The numerical value of g at Earth’s surface depends on ...
CH6.5.Ast1001.F13.EDS
... Jupiter-like planets should not form inside the frost line (at << 5 AU). • The discovery of “hot Jupiters” has forced a reexamination of nebular theory. • “Planetary migration” or gravitational encounters may explain “hot Jupiters.” ...
... Jupiter-like planets should not form inside the frost line (at << 5 AU). • The discovery of “hot Jupiters” has forced a reexamination of nebular theory. • “Planetary migration” or gravitational encounters may explain “hot Jupiters.” ...
Slide 1
... Oldest light we can pick up = Shows us the farthest back in time…14 byo From a time when the Universe wasn’t cold and dark…it was a firestorm of radiation and elementary particles which these later form the planets & galaxies As the Universe was stretched through expansion… so were the wavelengths o ...
... Oldest light we can pick up = Shows us the farthest back in time…14 byo From a time when the Universe wasn’t cold and dark…it was a firestorm of radiation and elementary particles which these later form the planets & galaxies As the Universe was stretched through expansion… so were the wavelengths o ...
A PowerPoint on Lunar Grazing Occultations
... • (If the objects are comparable in size, it’s usually called an “eclipse” instead) • As the moon moves through it’s orbit, it passes in front of distant stars or planets. This essentially casts a shadow on the Earth and from within this shadow, you can watch the star approach the moon and wink off ...
... • (If the objects are comparable in size, it’s usually called an “eclipse” instead) • As the moon moves through it’s orbit, it passes in front of distant stars or planets. This essentially casts a shadow on the Earth and from within this shadow, you can watch the star approach the moon and wink off ...
the Voyage Visitor Guide
... What does the model tell you? Voyager 2 passed by Uranus in January 1986. On the scale of this model, Voyager 2 was traveling about 200 feet per year. Can you determine when Voyager 2 arrived at Neptune? The model Neptune is about 500 feet from the model Uranus. At 200 feet per year, it would take 2 ...
... What does the model tell you? Voyager 2 passed by Uranus in January 1986. On the scale of this model, Voyager 2 was traveling about 200 feet per year. Can you determine when Voyager 2 arrived at Neptune? The model Neptune is about 500 feet from the model Uranus. At 200 feet per year, it would take 2 ...
4 Kepler`s Laws - NMSU Astronomy
... Now we will use the Planets and Satellites program to examine Kepler’s laws. It is possible that the program will already be running when you get to your computer. If not, however, you will have to start it up. If your TA gave you a CDROM, then you need to insert the CDROM into the CDROM drive on yo ...
... Now we will use the Planets and Satellites program to examine Kepler’s laws. It is possible that the program will already be running when you get to your computer. If not, however, you will have to start it up. If your TA gave you a CDROM, then you need to insert the CDROM into the CDROM drive on yo ...
Lecture notes - itü | fizik mühendisliği
... • Moons are like little planets that encircle the real planets. • Usually, they are much smaller than planets. • Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. >63 for Jupiter). • Mars (2), Saturn (>34), Uranus (>27), Neptun (>13 ...
... • Moons are like little planets that encircle the real planets. • Usually, they are much smaller than planets. • Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. >63 for Jupiter). • Mars (2), Saturn (>34), Uranus (>27), Neptun (>13 ...
Planetary Orbit Simulator – Student Guide
... occur when creating a simulator rather than any true physical limitations. We have limited the semi-major axis to 50 AU since that covers most of the objects in which we are interested in our solar system and have limited eccentricity to 0.7 since the ellipses would be hard to fit on the screen for ...
... occur when creating a simulator rather than any true physical limitations. We have limited the semi-major axis to 50 AU since that covers most of the objects in which we are interested in our solar system and have limited eccentricity to 0.7 since the ellipses would be hard to fit on the screen for ...
How the Solar System formed
... • Moons are like little planets that encircle the real planets. • Usually, they are much smaller than planets. • Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. >63 for Jupiter). • Mars (2), Saturn (>34), Uranus (>27), Neptun (>13 ...
... • Moons are like little planets that encircle the real planets. • Usually, they are much smaller than planets. • Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. >63 for Jupiter). • Mars (2), Saturn (>34), Uranus (>27), Neptun (>13 ...
How the Solar System formed
... • Moons are like little planets that encircle the real planets. • Usually, they are much smaller than planets. • Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. >63 for Jupiter). • Mars (2), Saturn (>34), Uranus (>27), Neptun (>13 ...
... • Moons are like little planets that encircle the real planets. • Usually, they are much smaller than planets. • Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. >63 for Jupiter). • Mars (2), Saturn (>34), Uranus (>27), Neptun (>13 ...
Q3.2.a The gravitational force exerted by a planet on one of its
... itself in a block of mass 0.50 kg that is sitting at rest on a very slippery sheet of ice. Which equation will correctly give the final speed vf_BLOCK of the block? 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.04 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK ...
... itself in a block of mass 0.50 kg that is sitting at rest on a very slippery sheet of ice. Which equation will correctly give the final speed vf_BLOCK of the block? 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.04 kg) *vf_BLOCK 1) (0.04 kg)*(800 m/s) = (0.50 kg) *vf_BLOCK ...
Satellite system (astronomy)
A satellite system is a set of gravitationally bound objects in orbit around a planetary mass object or minor planet. Generally speaking, it is a set of natural satellites (moons), although such systems may also consist of bodies such as circumplanetary disks, ring systems, moonlets, minor-planet moons and artificial satellites any of which may themselves have satellite systems of their own. Some satellite systems have complex interactions with both their parent and other moons, including magnetic, tidal, atmospheric and orbital interactions such as orbital resonances and libration. Individually major satellite objects are designated in Roman numerals. Satellite systems are referred to either by the possessive adjectives of their primary (e.g. ""Jovian system""), or less commonly by the name of their primary (e.g. ""Jupiter system""). Where only one satellite is known, or it is a binary orbiting a common centre of gravity, it may be referred to using the hyphenated names of the primary and major satellite (e.g. the ""Earth-Moon system"").Many Solar System objects are known to possess satellite systems, though their origin is still unclear. Notable examples include the largest satellite system, the Jovian system, with 67 known moons (including the large Galilean moons) and the Saturnian System with 62 known moons (and the most visible ring system in the Solar System). Both satellite systems are large and diverse. In fact all of the giant planets of the Solar System possess large satellite systems as well as planetary rings, and it is inferred that this is a general pattern. Several objects farther from the Sun also have satellite systems consisting of multiple moons, including the complex Plutonian system where multiple objects orbit a common center of mass, as well as many asteroids and plutinos. Apart from the Earth-Moon system and Mars' system of two tiny natural satellites, the other terrestrial planets are generally not considered satellite systems, although some have been orbited by artificial satellites originating from Earth.Little is known of satellite systems beyond the Solar System, although it is inferred that natural satellites are common. J1407b is an example of an extrasolar satellite system. It is also theorised that Rogue planets ejected from their planetary system could retain a system of satellites.