![Integrated Science](http://s1.studyres.com/store/data/008591837_1-3b50d080f6b7c9b7331fb6ef31f7bffa-300x300.png)
Integrated Science
... planes in a series of collision B) Planetesimals grew into protoplanets C) Planetesimals became large enough to exert gravity on nearby objects D) Ball of gas and dust collided and grew ...
... planes in a series of collision B) Planetesimals grew into protoplanets C) Planetesimals became large enough to exert gravity on nearby objects D) Ball of gas and dust collided and grew ...
6.3 Gravity and Orbits
... distance between them Supporting Details Each planet in the solar system is drawn towards the sun by its gravity. Gravity is the force of attraction, or pull, between two objects. o Gravity is affected by: The mass of two objects The distance between the two objects Gravity is stronger whe ...
... distance between them Supporting Details Each planet in the solar system is drawn towards the sun by its gravity. Gravity is the force of attraction, or pull, between two objects. o Gravity is affected by: The mass of two objects The distance between the two objects Gravity is stronger whe ...
Neptune Nachman
... ❏ Temp. range of -151.1 through -201.1 degrees celsius on Neptune ❏ Temp. range of 10 through 20 degrees celsius on Earth ❏ Temp. range of 18.3 through 21.1 degrees celsius in Florida ...
... ❏ Temp. range of -151.1 through -201.1 degrees celsius on Neptune ❏ Temp. range of 10 through 20 degrees celsius on Earth ❏ Temp. range of 18.3 through 21.1 degrees celsius in Florida ...
INSTITUTO EDUCACIONAL SÃO JOÃO DA ESCÓCIA
... The Sun, eight planets and their moons, an asteroid belt and many comets and meteors are in our Solar System. The Sun is in the center.It is a large, bright object in the Solar System. Around the Sun there are planets,moons,dwarf planets, asteroids, comets, meteoroids, rocks, interplanetary dust and ...
... The Sun, eight planets and their moons, an asteroid belt and many comets and meteors are in our Solar System. The Sun is in the center.It is a large, bright object in the Solar System. Around the Sun there are planets,moons,dwarf planets, asteroids, comets, meteoroids, rocks, interplanetary dust and ...
Asteroids,Comets, Meteor ppt.
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
Asteroids,Comets, Meteor ppt.
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
Interesting Science Facts - Comets
... cloud of comets which lies approximately one light year from the Sun. ...
... cloud of comets which lies approximately one light year from the Sun. ...
Jupiter and Saturn
... • Form faster, and in a different way, compared to terrestrial planets: large enough to accumulate gas directly from the solar nebula • They are far from the Sun (in the case of the solar system) • So far, all known extrasolar planets are gas giants, but they are all close to their parent star (why? ...
... • Form faster, and in a different way, compared to terrestrial planets: large enough to accumulate gas directly from the solar nebula • They are far from the Sun (in the case of the solar system) • So far, all known extrasolar planets are gas giants, but they are all close to their parent star (why? ...
Day-39
... the solar wind interacting with ions of the nucleus. Dust tail created from solar wind and sunlight. Comet tails point away from the Sun. ...
... the solar wind interacting with ions of the nucleus. Dust tail created from solar wind and sunlight. Comet tails point away from the Sun. ...
The populations of comet-like bodies in the Solar system
... & Duncan 1997). Centaur orbits are typically planet-crossing and have relatively short dynamical lifetimes (∼106 yr). Chiron, which is one of a number of exceptionally large minor bodies with perihelia close to or within the orbit of Saturn, exhibits cometary activity (e.g. Luu & Jewitt 1990) and ev ...
... & Duncan 1997). Centaur orbits are typically planet-crossing and have relatively short dynamical lifetimes (∼106 yr). Chiron, which is one of a number of exceptionally large minor bodies with perihelia close to or within the orbit of Saturn, exhibits cometary activity (e.g. Luu & Jewitt 1990) and ev ...
A Comet Nucleus
... with Neptune. That is, they make 2 complete orbits around the Sun for every 3 orbits by Neptune. This is a stable situation into which they were captured from somewhat different orbits. The Kuiper belt is the last remnant of the Solar nebula and the planet formation process. Planet formation proceed ...
... with Neptune. That is, they make 2 complete orbits around the Sun for every 3 orbits by Neptune. This is a stable situation into which they were captured from somewhat different orbits. The Kuiper belt is the last remnant of the Solar nebula and the planet formation process. Planet formation proceed ...
Astronomy - Ascent Academies of Utah Blogging System Sites
... • The name comet comes from the Latin word cometa which means "long-haired". • The earliest known record of a comet sighting was made by an astrologer of the Chinese court in 1059 B.C. • Comets are thought to originate from the Kuiper Belt and beyond. ...
... • The name comet comes from the Latin word cometa which means "long-haired". • The earliest known record of a comet sighting was made by an astrologer of the Chinese court in 1059 B.C. • Comets are thought to originate from the Kuiper Belt and beyond. ...
Neptune - Super Teacher Worksheets
... made up mainly of frozen methane gas. Like the other “gas giant” planets, winds that blow Neptune’s clouds around are very strong. Scientists say winds reach speeds of up to 700 miles an hour (about 1,120 kilometers per hour). Neptune isn’t quite as cold as Uranus, but its largest moon, Triton, is e ...
... made up mainly of frozen methane gas. Like the other “gas giant” planets, winds that blow Neptune’s clouds around are very strong. Scientists say winds reach speeds of up to 700 miles an hour (about 1,120 kilometers per hour). Neptune isn’t quite as cold as Uranus, but its largest moon, Triton, is e ...
27.2 Models of the Solar System (p 691
... It wasn’t until 1543 that an astronomer named ___________________ proposes a ______ ________ or Sun-centered model of the solar system. His explanation to why planets were moving backwards was that each planet orbited the _________ at a different ________, causing faster moving planets to ________ s ...
... It wasn’t until 1543 that an astronomer named ___________________ proposes a ______ ________ or Sun-centered model of the solar system. His explanation to why planets were moving backwards was that each planet orbited the _________ at a different ________, causing faster moving planets to ________ s ...
Scale Model Solar System (with Pluto)
... Scale Model Solar System (with Pluto) Supplemental Teaching Activity (6th-8th) Montana Space Public Outreach Team ...
... Scale Model Solar System (with Pluto) Supplemental Teaching Activity (6th-8th) Montana Space Public Outreach Team ...
Activity #1: The Mass Density Profile of the Solar System
... (j) Triton has a thin atmosphere of nitrogen and Titan has a thick atmosphere of methane. Why do these substances dominate their respective atmospheres? Hint: Consider the various phases in which water can be found on Earth. ...
... (j) Triton has a thin atmosphere of nitrogen and Titan has a thick atmosphere of methane. Why do these substances dominate their respective atmospheres? Hint: Consider the various phases in which water can be found on Earth. ...
Origin of Solar System Study Guide
... terrestrial planets). When astronomers see a rocky or icy surface with few craters, they know that the surface is new. For example, the moon and Mercury are very old surfaces – they are marked with craters – while Europa and the Earth show far fewer craters. Earth’s and Europa’s surfaces are, due to ...
... terrestrial planets). When astronomers see a rocky or icy surface with few craters, they know that the surface is new. For example, the moon and Mercury are very old surfaces – they are marked with craters – while Europa and the Earth show far fewer craters. Earth’s and Europa’s surfaces are, due to ...
The Outer Planets
... Dwarf planets are round and orbits the sun, like a planet, but it has not cleared out the neighborhood around its orbit Dwarf planet classification was created in 2006 when an object larger than Pluto and farther from the sun was discovered At that time Pluto was reclassified as a dwarf planet a ...
... Dwarf planets are round and orbits the sun, like a planet, but it has not cleared out the neighborhood around its orbit Dwarf planet classification was created in 2006 when an object larger than Pluto and farther from the sun was discovered At that time Pluto was reclassified as a dwarf planet a ...
A glimpse at the formation of our Solar System
... could merge in planet-sized objects, helped by their own gravitational attraction. Temperatures varied across the disk, being higher closer to the Sun than further out. While water was gaseous in the inner regions, it was solid ice beyond a certain radius called the “snow line”. Beyond this radius, ...
... could merge in planet-sized objects, helped by their own gravitational attraction. Temperatures varied across the disk, being higher closer to the Sun than further out. While water was gaseous in the inner regions, it was solid ice beyond a certain radius called the “snow line”. Beyond this radius, ...
15.5 BLM
... “gas giants,” all contain hydrogen and helium. They all have many moons and are surrounded by a set of rings. Jupiter has an enormous storm, larger than Earth, called the Great Red Spot. Saturn has the most spectacular rings. Viewed from Earth, Uranus rotates from top to bottom, because its axis of ...
... “gas giants,” all contain hydrogen and helium. They all have many moons and are surrounded by a set of rings. Jupiter has an enormous storm, larger than Earth, called the Great Red Spot. Saturn has the most spectacular rings. Viewed from Earth, Uranus rotates from top to bottom, because its axis of ...
Formation of solar system HW
... elsewhere in the galaxy, such as in the Large Magellanic cloud 160,000 light years away. Although we can't know for sure, astronomers think that our early solar system looked very much like this. ...
... elsewhere in the galaxy, such as in the Large Magellanic cloud 160,000 light years away. Although we can't know for sure, astronomers think that our early solar system looked very much like this. ...
MINOR Members of the Solar System
... solar system, 2. material from the asteroid belt, or 3. the solid remains of comets that once traveled near Earth’s orbit A few meteoroids are believed to be fragments of the moon, or possibly Mars, that were ejected when an ...
... solar system, 2. material from the asteroid belt, or 3. the solid remains of comets that once traveled near Earth’s orbit A few meteoroids are believed to be fragments of the moon, or possibly Mars, that were ejected when an ...
A201 – Solutions #5
... current techniques. a) Earth-sized planets in Earth-sized orbits, b) Jupiter-sized planets in Jupiter-sized orbits, c) Earth-sized planets in Jupiter-sized orbits, d) Jupiter-sized planets in Earth-sized orbits. Justify the order of each entry. [10 marks] Solution: One way to order these is d), b), ...
... current techniques. a) Earth-sized planets in Earth-sized orbits, b) Jupiter-sized planets in Jupiter-sized orbits, c) Earth-sized planets in Jupiter-sized orbits, d) Jupiter-sized planets in Earth-sized orbits. Justify the order of each entry. [10 marks] Solution: One way to order these is d), b), ...
1698 - Lunar and Planetary Institute
... of Neptune from features (i) to (iv). The orbital period of Neptune could be obtained from continuous observation of the motion of the dark spot around the Sun. With the known orbital period, the orbital location of Neptune could easily be obtained using Kepler‘s Laws. The mass of Neptune could be e ...
... of Neptune from features (i) to (iv). The orbital period of Neptune could be obtained from continuous observation of the motion of the dark spot around the Sun. With the known orbital period, the orbital location of Neptune could easily be obtained using Kepler‘s Laws. The mass of Neptune could be e ...
Formation of the Kuiper Belt by Long Time
... Figures 1 and 2 summarize the final distributions of their semimajor axes, eccentricities and inclinations after 2 × 108 years of integration for different values of β. For clarity, the final orbital elements a, e and i have been averaged over the last two million years in the integrations. Figures ...
... Figures 1 and 2 summarize the final distributions of their semimajor axes, eccentricities and inclinations after 2 × 108 years of integration for different values of β. For clarity, the final orbital elements a, e and i have been averaged over the last two million years in the integrations. Figures ...
Scattered disc
![](https://commons.wikimedia.org/wiki/Special:FilePath/Eris_and_dysnomia2.jpg?width=300)
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.