1000 Yard Solar System Model Worksheet
... 3) We want to know how far each object is from the prior one - it will make it easier to pace out the distances. Calculate and fill in those values in the next column. 4) In the last column we'll calculate the size of the object at the scale of the model. Divide the object diameter by the scale fact ...
... 3) We want to know how far each object is from the prior one - it will make it easier to pace out the distances. Calculate and fill in those values in the next column. 4) In the last column we'll calculate the size of the object at the scale of the model. Divide the object diameter by the scale fact ...
HW6 class solution
... 2. On the same graph, plot the gravitational acceleration of the satellite due to Earths gravity and the (maximum) gravitational acceleration of the satellite due to the Suns gravity as a function of the altitude of the satellite as measured from the surface of the Earth. Scale your plot so that the ...
... 2. On the same graph, plot the gravitational acceleration of the satellite due to Earths gravity and the (maximum) gravitational acceleration of the satellite due to the Suns gravity as a function of the altitude of the satellite as measured from the surface of the Earth. Scale your plot so that the ...
Skylights - May 2017 - Astronomical Society of Northern New England
... Venus at its best and brightest for the year in the morning sky, Jupiter just past its best for the year in the evening sky, some nice conjunctions of the moon with Venus, Mars, and Mercury, Saturn rising earlier each night and approaching its opposition next month, the brightest asteroid, Vesta, vi ...
... Venus at its best and brightest for the year in the morning sky, Jupiter just past its best for the year in the evening sky, some nice conjunctions of the moon with Venus, Mars, and Mercury, Saturn rising earlier each night and approaching its opposition next month, the brightest asteroid, Vesta, vi ...
- IIT Kanpur
... particles there did not combine to form the planets. Due to large distance from the Sun it should be very cold and like central part of the comets it should be consisting of dust and gases. This flat belt is called 'Couiper Belt'. Couiper assumed that all small period comets emerge from this belt. I ...
... particles there did not combine to form the planets. Due to large distance from the Sun it should be very cold and like central part of the comets it should be consisting of dust and gases. This flat belt is called 'Couiper Belt'. Couiper assumed that all small period comets emerge from this belt. I ...
Chapter 8 Moons, Rings, and Plutoids
... surface is water ice, possibly with liquid water below. Tidal forces stress and crack ice; water flows, keeping surface relatively flat. ...
... surface is water ice, possibly with liquid water below. Tidal forces stress and crack ice; water flows, keeping surface relatively flat. ...
ACTIVE ACCRETION——An Active Learning Game on Solar
... The current Condensation Theory of Solar System Formation* was the brain child of French philosopher Rene Descartes, who lived in the 17th century. In the 18th century, Pierre Simon de Laplace revised this theory. Both of these early astronomers based their theories on a disk-shaped solar nebula tha ...
... The current Condensation Theory of Solar System Formation* was the brain child of French philosopher Rene Descartes, who lived in the 17th century. In the 18th century, Pierre Simon de Laplace revised this theory. Both of these early astronomers based their theories on a disk-shaped solar nebula tha ...
solareclipsebundle-middleschool
... A. Students use the patterns they find in multiple types of data at varying scales to draw conclusions about the identifying characteristics of different categories of solar system objects (e.g., planets, meteors, asteroids, comets) based on their features, composition, and locations within the sola ...
... A. Students use the patterns they find in multiple types of data at varying scales to draw conclusions about the identifying characteristics of different categories of solar system objects (e.g., planets, meteors, asteroids, comets) based on their features, composition, and locations within the sola ...
this PDF file - Department of Physics and Astronomy
... g, at the planet’s surface. We will calculate the tidal acceleration for Jupiter and its moon Io, Saturn and its largest moon Titan, Uranus and its largest moon Titania, as well as Neptune and its largest moon Triton. Proceeding as before, the mass of the orbiting moon is M1 , the mass of the planet ...
... g, at the planet’s surface. We will calculate the tidal acceleration for Jupiter and its moon Io, Saturn and its largest moon Titan, Uranus and its largest moon Titania, as well as Neptune and its largest moon Triton. Proceeding as before, the mass of the orbiting moon is M1 , the mass of the planet ...
VIDEO WEB HIT HOMEWORK – part 2
... - Only 15%-20% of Earth’s Precambrian rock surfaces are exposed. The remaining rocks are buried by younger rocks and sediments. - Most of the Precambrian surfaces are composed of igneous and metamorphic rocks. - These types of rocks do not yield much evidence of geologic events of Earth’s past histo ...
... - Only 15%-20% of Earth’s Precambrian rock surfaces are exposed. The remaining rocks are buried by younger rocks and sediments. - Most of the Precambrian surfaces are composed of igneous and metamorphic rocks. - These types of rocks do not yield much evidence of geologic events of Earth’s past histo ...
planetas - gvlibraries.org
... the things that circle Saturn. 54 These things look like giant rings. 55 The large, beautiful rings of Saturn are made of particles of ice and rock that orbit the planet. 56 About 207 billion kilometers from us is the planet Uranus. 57 This very cold planet also has large rings, and it’s tilt ...
... the things that circle Saturn. 54 These things look like giant rings. 55 The large, beautiful rings of Saturn are made of particles of ice and rock that orbit the planet. 56 About 207 billion kilometers from us is the planet Uranus. 57 This very cold planet also has large rings, and it’s tilt ...
Refuges for Life in a - University of Arizona
... (which extends halfway to the nearest star). Other stars probably have similar retinues. Infrared observations of young nearby stars indicate that most are surrounded by excess dust, consistent with the presence of Kuiper-belt objects. More recently, detection of water vapor around the highly evolve ...
... (which extends halfway to the nearest star). Other stars probably have similar retinues. Infrared observations of young nearby stars indicate that most are surrounded by excess dust, consistent with the presence of Kuiper-belt objects. More recently, detection of water vapor around the highly evolve ...
class14
... Jovian planets all have rings because they possess many small moons close-in. Impacts on these moons are random. Saturn’s incredible rings may be an “accident” of our time. ...
... Jovian planets all have rings because they possess many small moons close-in. Impacts on these moons are random. Saturn’s incredible rings may be an “accident” of our time. ...
Phys 214. Planets and Life
... Despite the generally extremely high temperature of its surface, observations strongly suggest that ice exists on Mercury. Floors of deep craters near the poles are never exposed to direct sunlight, and have temperatures lower than the global average. Water ice strongly reflects radar, and observati ...
... Despite the generally extremely high temperature of its surface, observations strongly suggest that ice exists on Mercury. Floors of deep craters near the poles are never exposed to direct sunlight, and have temperatures lower than the global average. Water ice strongly reflects radar, and observati ...
Earth Science
... universe, Visual, radio, and x-ray telescopes collect information from across the entire spectrum of electromagnetic waves; computers handle data and complicated computations to interpret them; space probes and back data and materials from remote parts of the solar system; and accelerators give suba ...
... universe, Visual, radio, and x-ray telescopes collect information from across the entire spectrum of electromagnetic waves; computers handle data and complicated computations to interpret them; space probes and back data and materials from remote parts of the solar system; and accelerators give suba ...
MS The Solar System
... Meanwhile, the outer parts of the disk were cooling off. Small pieces of dust started clumping together. These clumps collided and combined with other clumps. Larger clumps attracted smaller clumps with their gravity. Eventually, all these pieces grew into the planets and moons that we find in our s ...
... Meanwhile, the outer parts of the disk were cooling off. Small pieces of dust started clumping together. These clumps collided and combined with other clumps. Larger clumps attracted smaller clumps with their gravity. Eventually, all these pieces grew into the planets and moons that we find in our s ...
Kepler`s Laws of Planetary Motion
... The distance of the planet from the star can then be determined by measuring the angle between the observed position of the perihelion and the observed position of the planet (q). PERIOD (T) - the time for one complete revolution around the sun. – Can be used to predict when the planet will pass any ...
... The distance of the planet from the star can then be determined by measuring the angle between the observed position of the perihelion and the observed position of the planet (q). PERIOD (T) - the time for one complete revolution around the sun. – Can be used to predict when the planet will pass any ...
How common are habitable planets?
... brightness. From among the 150,000 stars were Earth-size, that is, one to two times the photographed every 30 minutes for four years, diameter of Earth and orbiting their star at a NASA's Kepler team reported more than 3,000 distance where they are heated to lukewarm planet candidates. Many of these ...
... brightness. From among the 150,000 stars were Earth-size, that is, one to two times the photographed every 30 minutes for four years, diameter of Earth and orbiting their star at a NASA's Kepler team reported more than 3,000 distance where they are heated to lukewarm planet candidates. Many of these ...
Jupiter`s Galilean Moons
... Again, with the exception of Callisto, all the cores are surrounded by rock (shown in brown) shells. Io’s rock or silicate shell extends to the surface, while the rock layers of Ganymede and Europa (drawn to correct relative scale) are in turn surrounded by shells of water in ice or liquid form (sho ...
... Again, with the exception of Callisto, all the cores are surrounded by rock (shown in brown) shells. Io’s rock or silicate shell extends to the surface, while the rock layers of Ganymede and Europa (drawn to correct relative scale) are in turn surrounded by shells of water in ice or liquid form (sho ...
7-12 Script - Geophysical Institute
... orbits to ellipses. Galileo further solidified evidence for the model when he observed the moons of Jupiter. Showing that objects orbit other planets (not just Earth) supported the idea that not everything was in orbit around us. If time allows: See JUPITER'S MOONS as you would through a telescope a ...
... orbits to ellipses. Galileo further solidified evidence for the model when he observed the moons of Jupiter. Showing that objects orbit other planets (not just Earth) supported the idea that not everything was in orbit around us. If time allows: See JUPITER'S MOONS as you would through a telescope a ...
A travel guide to Mars
... can cover the entire planet and last for months. Mars once had rivers, lakes, and maybe even oceans like the Earth does. But water did not remain liquid very long, and is now trapped as ice mixed with dust at the poles and inside the rocks. Today we can only see traces of the ancient dried-up water ...
... can cover the entire planet and last for months. Mars once had rivers, lakes, and maybe even oceans like the Earth does. But water did not remain liquid very long, and is now trapped as ice mixed with dust at the poles and inside the rocks. Today we can only see traces of the ancient dried-up water ...
objects
... Weight can change if an object is located on another object in space, for example, the Moon or Mars. The mass of that larger object determines the pull of gravity and therefore the weight of the object. Weight may change due to the change in gravitational force, but mass stays the same. ...
... Weight can change if an object is located on another object in space, for example, the Moon or Mars. The mass of that larger object determines the pull of gravity and therefore the weight of the object. Weight may change due to the change in gravitational force, but mass stays the same. ...
Page pour l`impression
... present. These locations are in resonance with Jupiter . The role of Jupiter has been to eject the bodies in resonance with the planet. The 3:2 resonance with Neptune plays the inverse role. At the location of this resonance, numerous bodies piled up, including Pluto. This resonance is stable. The r ...
... present. These locations are in resonance with Jupiter . The role of Jupiter has been to eject the bodies in resonance with the planet. The 3:2 resonance with Neptune plays the inverse role. At the location of this resonance, numerous bodies piled up, including Pluto. This resonance is stable. The r ...
Late Heavy Bombardment
The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.