Solar System in Your Pocket
... Pull out a folded up completed sample of the solar system model. Point out that the planets never appear in a straight line like this model, which is an example of one of the limitations of this model. The planets would be found somewhere along a circle this far from the Sun. If there is a bulletin ...
... Pull out a folded up completed sample of the solar system model. Point out that the planets never appear in a straight line like this model, which is an example of one of the limitations of this model. The planets would be found somewhere along a circle this far from the Sun. If there is a bulletin ...
14. 1 A Travel Guide to the Outer Planets 14.2 Jupiter 14.3 Saturn
... • The rings of Neptune are made of dark icy particles in narrow hoops. Neptune's rings contain arcs produced by the gravitational influence of one or more moons. ...
... • The rings of Neptune are made of dark icy particles in narrow hoops. Neptune's rings contain arcs produced by the gravitational influence of one or more moons. ...
neptune - Robertson County School
... What does Neptune look like? The particles of icy methane in the clouds takes orange and red light waves and absorbs them, which leaves blue light waves to make an escape and create an outward reflection through our eyes. This is the process of how the sunlight is being reflected off to the atmosph ...
... What does Neptune look like? The particles of icy methane in the clouds takes orange and red light waves and absorbs them, which leaves blue light waves to make an escape and create an outward reflection through our eyes. This is the process of how the sunlight is being reflected off to the atmosph ...
Newton`s Laws of Motion and Planetary Orbits
... What does this have to do with solar system objects? Or astronomy? ...
... What does this have to do with solar system objects? Or astronomy? ...
1 Newton`s Laws of Motion…vocabulary
... • The solution to F=ma for a planet is an ellipse with the Sun at one focus (Kepler’s 1st Law) • The semimajor axis and orbital period are related by: Kepler’s 3rd Law (or is it?) ?????? ...
... • The solution to F=ma for a planet is an ellipse with the Sun at one focus (Kepler’s 1st Law) • The semimajor axis and orbital period are related by: Kepler’s 3rd Law (or is it?) ?????? ...
4.2 The planets and their satellites
... life. Moreover, there are asteroids with moons and comets that may still harbor the clues to how the Solar System and life on Earth formed. In the following chapters, we will present basic data about the Solar System and briefly summarize the results of space exploration, laboratory measurements and ...
... life. Moreover, there are asteroids with moons and comets that may still harbor the clues to how the Solar System and life on Earth formed. In the following chapters, we will present basic data about the Solar System and briefly summarize the results of space exploration, laboratory measurements and ...
Overview of the Solar System
... • distance to each planet known – Kepler’s and Newton’s Law, radar ranging • sidereal orbital period of each planet known – earth’s motion well understood • the sizes of the all planets are known – angular size • masses of all the planets known – the ones with observable moons, can use Newton’s Laws ...
... • distance to each planet known – Kepler’s and Newton’s Law, radar ranging • sidereal orbital period of each planet known – earth’s motion well understood • the sizes of the all planets are known – angular size • masses of all the planets known – the ones with observable moons, can use Newton’s Laws ...
Asteroids, meteorites, and comets
... The outer edge of our Solar System is not empty. There are many, many huge spheres of ice and rock out near Pluto's orbit. Astronomers call this huge group of planetoids "Kuiper Belt Objects", or "KBOs" for short. The Kuiper Belt is a bit like the asteroid belt, but much farther from the Sun. See ho ...
... The outer edge of our Solar System is not empty. There are many, many huge spheres of ice and rock out near Pluto's orbit. Astronomers call this huge group of planetoids "Kuiper Belt Objects", or "KBOs" for short. The Kuiper Belt is a bit like the asteroid belt, but much farther from the Sun. See ho ...
chapter12AsterioidsC..
... • Pluto will never hit Neptune, even though their orbits cross, because of 3:2 orbital resonance • Neptune orbits three times during the time Pluto orbits twice ...
... • Pluto will never hit Neptune, even though their orbits cross, because of 3:2 orbital resonance • Neptune orbits three times during the time Pluto orbits twice ...
Pluto is (still) not a planet
... Pluto and its large moon Charon have the largest parent-to-moon mass ratio in the Solar System. ...
... Pluto and its large moon Charon have the largest parent-to-moon mass ratio in the Solar System. ...
What are the components of our solar system? How would the solar
... a. Students use the model to describe that gravity is a predominantly inward-pulling force that can keep smaller/less massive objects in orbit around larger/more massive objects. b. Students use the model to describe that gravity causes a pattern of smaller/less massive objects orbiting around large ...
... a. Students use the model to describe that gravity is a predominantly inward-pulling force that can keep smaller/less massive objects in orbit around larger/more massive objects. b. Students use the model to describe that gravity causes a pattern of smaller/less massive objects orbiting around large ...
Kuiper Belt, Oort Cloud and TNOs
... 1943: Astronomer Kenneth Edgeworth suggests that a reservoir of comets and larger bodies resides beyond the planets. 1950: Astronomer Jan Oort theorizes that a vast population of comets may exist in a huge cloud on the distant edges of our solar system. 1951: Astronomer Gerard Kuiper predicts the ex ...
... 1943: Astronomer Kenneth Edgeworth suggests that a reservoir of comets and larger bodies resides beyond the planets. 1950: Astronomer Jan Oort theorizes that a vast population of comets may exist in a huge cloud on the distant edges of our solar system. 1951: Astronomer Gerard Kuiper predicts the ex ...
Neptune - TeacherLINK
... Uranus' orbit did not agree with theory, which led theorists to hypothesize about the existence of yet another planet, well beyond Uranus which perturbed the orbit of Uranus. Calculations were performed to reveal the approximate location followed by investigators at institutions in several countries ...
... Uranus' orbit did not agree with theory, which led theorists to hypothesize about the existence of yet another planet, well beyond Uranus which perturbed the orbit of Uranus. Calculations were performed to reveal the approximate location followed by investigators at institutions in several countries ...
Solar System Data Sheet
... Gas Giants – Jupiter, Saturn, Uranus, Neptune Classical Planets (seen without a telescope) – Mercury, Venus, Mars, Jupiter, Saturn Modern Planets (seen with a telescope) – Uranus, Neptune Inferior Planets (having an orbit between Earth and the Sun) – Mercury, Venus Superior Planets (having an orbit ...
... Gas Giants – Jupiter, Saturn, Uranus, Neptune Classical Planets (seen without a telescope) – Mercury, Venus, Mars, Jupiter, Saturn Modern Planets (seen with a telescope) – Uranus, Neptune Inferior Planets (having an orbit between Earth and the Sun) – Mercury, Venus Superior Planets (having an orbit ...
205 Tiffany Science
... Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. All of these planets orbit the Sun, the only star in the solar system. When they orbit, they revolve around the Sun. When they rotate, the planets spin on their axis. Meteorites are masses of rock and metal that float around in space. If an astronau ...
... Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. All of these planets orbit the Sun, the only star in the solar system. When they orbit, they revolve around the Sun. When they rotate, the planets spin on their axis. Meteorites are masses of rock and metal that float around in space. If an astronau ...
Comets, Asteroids, and Meteors
... Comets Because their orbits are so elliptical, few pass near Earth and when they do they are only seen briefly. • Since comets have an orbit, we usually will see the same comet every several years. Ex: Haley’s comets passes by Earth every 76 years. Last seen: 1986, next seen 2062. ...
... Comets Because their orbits are so elliptical, few pass near Earth and when they do they are only seen briefly. • Since comets have an orbit, we usually will see the same comet every several years. Ex: Haley’s comets passes by Earth every 76 years. Last seen: 1986, next seen 2062. ...
Celestial Motions - Norwich High School
... What keeps objects in orbit? the force that attracts a body toward the center of any other physical body having mass. ...
... What keeps objects in orbit? the force that attracts a body toward the center of any other physical body having mass. ...
Clearing stage: Oort cloud formation
... this 3km-planetesimal was thrown out in the giant impacts era from Saturn-Neptune region into the Oort cloud, then wandered closer to Uranus/Jupiter & has recently been perturbed by Jupiter (5 orbits ago) to become a short-period comet ...
... this 3km-planetesimal was thrown out in the giant impacts era from Saturn-Neptune region into the Oort cloud, then wandered closer to Uranus/Jupiter & has recently been perturbed by Jupiter (5 orbits ago) to become a short-period comet ...
Meteorite
... the solar system. • Ice could form in the outer solar system. • A passing star probably stripped away all of ...
... the solar system. • Ice could form in the outer solar system. • A passing star probably stripped away all of ...
Worksheet 1
... b. material ejected by volcanic eruptions of the moons of the outer planets c. condensation of gas in the Sun’s hot outer atmosphere d. small icy bodies in the extreme outer parts of the Solar System that are disturbed into orbits that bring them closer to the Sun e. luminous clouds in the Earth’s u ...
... b. material ejected by volcanic eruptions of the moons of the outer planets c. condensation of gas in the Sun’s hot outer atmosphere d. small icy bodies in the extreme outer parts of the Solar System that are disturbed into orbits that bring them closer to the Sun e. luminous clouds in the Earth’s u ...
Seminar topics - Studentportalen
... Origin of sungrazers: a frequent cometary end-state Astron. Astrophys. 257, 315-322 (1992) ...
... Origin of sungrazers: a frequent cometary end-state Astron. Astrophys. 257, 315-322 (1992) ...
Document
... Inside Meteorites Many meteors contain spherical “chondrules”. The formation of these has been mysterious, but a recent Berkeley theory shows how they might have been melted by the young Sun. ...
... Inside Meteorites Many meteors contain spherical “chondrules”. The formation of these has been mysterious, but a recent Berkeley theory shows how they might have been melted by the young Sun. ...
Scattered disc
The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets, a subset of the broader family of trans-Neptunian objects. The scattered-disc objects (SDOs) have orbital eccentricities ranging as high as 0.8, inclinations as high as 40°, and perihelia greater than 30 astronomical units (4.5×109 km; 2.8×109 mi). These extreme orbits are thought to be the result of gravitational ""scattering"" by the gas giants, and the objects continue to be subject to perturbation by the planet Neptune.Although the closest scattered-disc objects approach the Sun at about 30–35 AU, their orbits can extend well beyond 100 AU. This makes scattered objects among the most distant and coldest objects in the Solar System. The innermost portion of the scattered disc overlaps with a torus-shaped region of orbiting objects traditionally called the Kuiper belt, but its outer limits reach much farther away from the Sun and farther above and below the ecliptic than the Kuiper belt proper.Because of its unstable nature, astronomers now consider the scattered disc to be the place of origin for most periodic comets in the Solar System, with the centaurs, a population of icy bodies between Jupiter and Neptune, being the intermediate stage in an object's migration from the disc to the inner Solar System. Eventually, perturbations from the giant planets send such objects towards the Sun, transforming them into periodic comets. Many Oort cloud objects are also thought to have originated in the scattered disc. Detached objects are not sharply distinct from scattered disc objects, and some such as Sedna have sometimes been considered to be included in this group.