asteroids, comets - MSU Solar Physics
... Its orbit is highly eccentric; at times it is closer to the Sun than Neptune. Its orbit inclination is also much larger than other planets. Pluto rotates in the opposite direction from most other planets. Pluto is smaller than 7 satellites in the solar system. It has an average density of about 1900 ...
... Its orbit is highly eccentric; at times it is closer to the Sun than Neptune. Its orbit inclination is also much larger than other planets. Pluto rotates in the opposite direction from most other planets. Pluto is smaller than 7 satellites in the solar system. It has an average density of about 1900 ...
Unit 8: Space Study Guide
... Neptune: – This planet has six rings and 13 confirmed moons. Atmosphere of Neptune is made up of hydrogen, methane and helium. It is smallest of all the out planets. Saturn: – This planet has 7 known rings and 53 known moons. This planet is mostly made up of hydrogen and helium and has an atmosphere ...
... Neptune: – This planet has six rings and 13 confirmed moons. Atmosphere of Neptune is made up of hydrogen, methane and helium. It is smallest of all the out planets. Saturn: – This planet has 7 known rings and 53 known moons. This planet is mostly made up of hydrogen and helium and has an atmosphere ...
DIY Solar System
... The Solar System consists of the Sun and eight planets, their moons, and other non-stellar objects, such as asteroids. The four smaller inner planets—Mercury, Venus, Earth and Mars, also called the terrestrial planets—are primarily composed of rock and metal. The four outer planets, called the gas g ...
... The Solar System consists of the Sun and eight planets, their moons, and other non-stellar objects, such as asteroids. The four smaller inner planets—Mercury, Venus, Earth and Mars, also called the terrestrial planets—are primarily composed of rock and metal. The four outer planets, called the gas g ...
Full Size Astronomy Cards
... the objects in the Kuiper belt are much larger and much colder. These objects are short period comets (meaning they take less than 200 years to make a complete revolution) orbiting around Neptune. There are approximately 35,000 comets in the Kuiper belt. All these comets orbit close to Pluto and in ...
... the objects in the Kuiper belt are much larger and much colder. These objects are short period comets (meaning they take less than 200 years to make a complete revolution) orbiting around Neptune. There are approximately 35,000 comets in the Kuiper belt. All these comets orbit close to Pluto and in ...
Opposition of Saturn - Hong Kong Observatory
... Saturn revolves around the Sun with a period of about 29.5 years. Opposition of Saturn will occur about once every 378 days. The last Saturn opposition occurred on 18 December 2002 and the next occurrence will be on 1 January 2004. As Saturn has just passed the perihelion of its orbit in July 2003 ...
... Saturn revolves around the Sun with a period of about 29.5 years. Opposition of Saturn will occur about once every 378 days. The last Saturn opposition occurred on 18 December 2002 and the next occurrence will be on 1 January 2004. As Saturn has just passed the perihelion of its orbit in July 2003 ...
4 times that of earth
... orbit that brings them though the inner solar system and near the sun. • As they get close to the sun the ice melts an the comet gets a tail. ...
... orbit that brings them though the inner solar system and near the sun. • As they get close to the sun the ice melts an the comet gets a tail. ...
GEOL3025, Section 030 Lecture #11 31 August 2007
... AKA Jovian Planets (like Jupiter) Gas Giants: Jupiter & Saturn Ice Giants: Uranus & Neptune + Pluto (Rocky-Ice planet?) ...
... AKA Jovian Planets (like Jupiter) Gas Giants: Jupiter & Saturn Ice Giants: Uranus & Neptune + Pluto (Rocky-Ice planet?) ...
What Makes Up Our Solar System
... atmospheres, rings and lots of satellites. It is thought that these planets may have a small solid core as large as three to 20 Earth masses at their center. The Kuiper Belt The Kuiper Belt is a disk-shaped region past the orbit of Neptune extending roughly 30 to 50 AU from the Sun and contains many ...
... atmospheres, rings and lots of satellites. It is thought that these planets may have a small solid core as large as three to 20 Earth masses at their center. The Kuiper Belt The Kuiper Belt is a disk-shaped region past the orbit of Neptune extending roughly 30 to 50 AU from the Sun and contains many ...
Moons of the Outer Solar System
... Orbital resonances with other moons can maintain eccentric orbits and tidal heating. ...
... Orbital resonances with other moons can maintain eccentric orbits and tidal heating. ...
4. Formation of Solar Systems
... 1. Are Earth-like planets rare or common? — hot (or warm) jupiters would disrupt Earth’s orbit — many stars do not have hot (or warm) jupiters — not yet possible to detect Earth-like planets 2. Do Hot Jupiters imply the Nebular theory is wrong? — jovian planets cannot form inside frost line ...
... 1. Are Earth-like planets rare or common? — hot (or warm) jupiters would disrupt Earth’s orbit — many stars do not have hot (or warm) jupiters — not yet possible to detect Earth-like planets 2. Do Hot Jupiters imply the Nebular theory is wrong? — jovian planets cannot form inside frost line ...
3. the galilean revolution: earth`s place in the
... 1. Select the better of the two images. 2. For that image, select the information window and record the system (not universal) date and time that the image was taken in Data Table 1. Also record the Julian date that the image was taken in Data Table 1, to the nearest 0.1 days. 3. Adjust the max valu ...
... 1. Select the better of the two images. 2. For that image, select the information window and record the system (not universal) date and time that the image was taken in Data Table 1. Also record the Julian date that the image was taken in Data Table 1, to the nearest 0.1 days. 3. Adjust the max valu ...
Powerpoint - BU Imaging Science
... • Asteroids are small, rocky bodies that orbit the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. ...
... • Asteroids are small, rocky bodies that orbit the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. ...
Our Planetary System (Chapter 7)
... • Asteroids are small, rocky bodies that orbit the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. ...
... • Asteroids are small, rocky bodies that orbit the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. ...
Kepler`s Third Law
... Because the planets do not move in exact circles, Copernicus followed Ptolemy in introducing small epicycles to describe deviations from circular orbits. The result was that Copernicus’ full system was as complicated as Ptolemy’s and no more accurate. ...
... Because the planets do not move in exact circles, Copernicus followed Ptolemy in introducing small epicycles to describe deviations from circular orbits. The result was that Copernicus’ full system was as complicated as Ptolemy’s and no more accurate. ...
Lesson 2 Power Notes Outline
... Upon plotting the orbit of Mars, Kepler saw that it was a deformed circle. ...
... Upon plotting the orbit of Mars, Kepler saw that it was a deformed circle. ...
Scale
... planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune! This gives you an idea of just how far our planets are from each other. However, we can make a scale model of the distances between the planets using almost anything as our reference. I ...
... planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune! This gives you an idea of just how far our planets are from each other. However, we can make a scale model of the distances between the planets using almost anything as our reference. I ...
Chapter-27-ppt from Christy
... Strong winds caused by differences in temperature between day and night Causing strong dust storms ...
... Strong winds caused by differences in temperature between day and night Causing strong dust storms ...
strange new Worlds - Scholars at Princeton
... swells up to become a gas giant. However, this threshold mass can only be achieved in distant, colder regions of the disk, where the supply of solid materials is enhanced by ices of water, methane, and ammonia. In other words, giant planets only form beyond the star system’s “snow line,” where there ...
... swells up to become a gas giant. However, this threshold mass can only be achieved in distant, colder regions of the disk, where the supply of solid materials is enhanced by ices of water, methane, and ammonia. In other words, giant planets only form beyond the star system’s “snow line,” where there ...
Birth of Science
... moves at the same speed in the same direction. Newton’s Second Law tells how to find the motion if there is a ...
... moves at the same speed in the same direction. Newton’s Second Law tells how to find the motion if there is a ...
Relative Sizes and Colors of Planets in the Solar System
... 8. A window will open. In the right section of this window where it says Label Options, check the box next to the X axis and uncheck any other box. Click close and you should see the planet name next to each planet. 9. Save your file by clicking on the little blue disk and continue with part C. C. F ...
... 8. A window will open. In the right section of this window where it says Label Options, check the box next to the X axis and uncheck any other box. Click close and you should see the planet name next to each planet. 9. Save your file by clicking on the little blue disk and continue with part C. C. F ...
The Outer Planets
... • All are not very dense (b/c made of gas) • Why do the outer planets share these similarities? • Why don’t the outer planets have more in common with the inner planets? ...
... • All are not very dense (b/c made of gas) • Why do the outer planets share these similarities? • Why don’t the outer planets have more in common with the inner planets? ...
File
... Earth: I am the third planet from the Sun. I am a rocky planet whose surface is covered mostly by water. I have continents, mountains, valleys, and active volcanoes. I have an atmosphere that creates a variety of weather and protects my surface from the harsh environment of space. Thus, I am proud ...
... Earth: I am the third planet from the Sun. I am a rocky planet whose surface is covered mostly by water. I have continents, mountains, valleys, and active volcanoes. I have an atmosphere that creates a variety of weather and protects my surface from the harsh environment of space. Thus, I am proud ...
Finding the Small Moons of the Outer Planets
... satellites smaller than about 10 km had ever been detected around any planet, though several earlier photographic surveys had attempted to probe this faint regime. It was thought that friction with an early disk of gas and dust around the giant planets may have preferentially removed all the smaller ...
... satellites smaller than about 10 km had ever been detected around any planet, though several earlier photographic surveys had attempted to probe this faint regime. It was thought that friction with an early disk of gas and dust around the giant planets may have preferentially removed all the smaller ...
Pocket Solar System - Skynet Junior Scholars
... the other “Pluto”. Even though Pluto has been reclassified as a dwarf planet it serves as a useful reference point here. We can use it as the first example of such a dwarf planet ever found. Now, lightly draw and label the planets in between. Where do you think they go?” Once they have predicted, tu ...
... the other “Pluto”. Even though Pluto has been reclassified as a dwarf planet it serves as a useful reference point here. We can use it as the first example of such a dwarf planet ever found. Now, lightly draw and label the planets in between. Where do you think they go?” Once they have predicted, tu ...