S-5-6-3_Pluto Graphic Organizer Why Isn`t Pluto a Planet
... Small size: Pluto is relatively tiny, having a mass about 1/500th that of Earth (in contrast, Mercury's mass is 1/20th that of Earth). In diameter, Pluto is 1/5th the size of Earth. Although puny on a planetary scale, Pluto is one of the largest objects inhabiting the Kuiper belt. Large moon: Pluto' ...
... Small size: Pluto is relatively tiny, having a mass about 1/500th that of Earth (in contrast, Mercury's mass is 1/20th that of Earth). In diameter, Pluto is 1/5th the size of Earth. Although puny on a planetary scale, Pluto is one of the largest objects inhabiting the Kuiper belt. Large moon: Pluto' ...
Unit - 2 The Earth and Its History- Students` Manual - CBSE
... own. They reflect the light they receive from the stars. The Earth is a planet and it receives its heat and light from the Sun. Asteroids: are a swarm of small bodies that revolve around the sun between the orbits of inner and outer planets, Mars and Jupiter. CERES is the largest asteroid. They are ...
... own. They reflect the light they receive from the stars. The Earth is a planet and it receives its heat and light from the Sun. Asteroids: are a swarm of small bodies that revolve around the sun between the orbits of inner and outer planets, Mars and Jupiter. CERES is the largest asteroid. They are ...
ASTR 150
... The orderly motions of our solar system are a direct result of the solar system’s birth in a spinning, flattened cloud of gas Not all mass falls in directly (radially). Why? All gas has a small spin that preferentially causes the formation of a flattened structure ...
... The orderly motions of our solar system are a direct result of the solar system’s birth in a spinning, flattened cloud of gas Not all mass falls in directly (radially). Why? All gas has a small spin that preferentially causes the formation of a flattened structure ...
Jupiter - QZAB Teachers
... •The third planet from the sun •Earth is the only place that life exist •Earth formed 4.54 billion years ago •Earth has it gedical history and orbit •Earth interacts with other objects in the outer space ...
... •The third planet from the sun •Earth is the only place that life exist •Earth formed 4.54 billion years ago •Earth has it gedical history and orbit •Earth interacts with other objects in the outer space ...
Formation of the Solar System
... Stars are too far away from the Sun, and direct imaging cannot detect planets near them Current strategy involves watching for the small gravitational tag the planet exerts on its star The tag can be detected using the Doppler effect ...
... Stars are too far away from the Sun, and direct imaging cannot detect planets near them Current strategy involves watching for the small gravitational tag the planet exerts on its star The tag can be detected using the Doppler effect ...
-1- I. Physical characteristics of the solar system The solar system
... (formulated by Bode in 1772). The relationship is derived by writing the series 0, 3, 6, 12 ....(obviously you are doubling each succeeding number), adding 4 to each number and dividing the result by 10. The first number in the series corresponds to Mercury. The results of these calculations can the ...
... (formulated by Bode in 1772). The relationship is derived by writing the series 0, 3, 6, 12 ....(obviously you are doubling each succeeding number), adding 4 to each number and dividing the result by 10. The first number in the series corresponds to Mercury. The results of these calculations can the ...
Lecture 1: Properties of the Solar System
... Planets and Sun revolve and orbit in a west-to-east direction. The planets obliquity (tilt of rotation axes to their orbits) are small. Uranus and Venus are exceptions. 4. The planets differ in composition. Their composition varies roughly with distance from the Sun: dense, metal-rich planets are in ...
... Planets and Sun revolve and orbit in a west-to-east direction. The planets obliquity (tilt of rotation axes to their orbits) are small. Uranus and Venus are exceptions. 4. The planets differ in composition. Their composition varies roughly with distance from the Sun: dense, metal-rich planets are in ...
Astro 1010 Planetary Astronomy Sample Questions for Exam 5
... d) located at the north pole of the planet. 2. The source of the magnetic fields of Jupiter and Saturn are a) currents in the molten nickel-iron outer core. b) permanent magnetization of the rocky inner core. c) air currents in the upper atmosphere. d) currents in the liquid metallic hydrogen layer. ...
... d) located at the north pole of the planet. 2. The source of the magnetic fields of Jupiter and Saturn are a) currents in the molten nickel-iron outer core. b) permanent magnetization of the rocky inner core. c) air currents in the upper atmosphere. d) currents in the liquid metallic hydrogen layer. ...
Pluto naomi
... Space Telescope observations suggest that the planet's density lies between 1.8 and 2.1 gm/cm3 which indicate that the planet is probably a mixture of 50 to 70 percent rock with the remainder being water and other ices much like Neptune’s moon Triton. • Pluto's composition is not very well known sin ...
... Space Telescope observations suggest that the planet's density lies between 1.8 and 2.1 gm/cm3 which indicate that the planet is probably a mixture of 50 to 70 percent rock with the remainder being water and other ices much like Neptune’s moon Triton. • Pluto's composition is not very well known sin ...
======= SPIRIT 2
... Place students into eight groups (one for each planet) and give each group a planet along with a guideline sheet. The guideline sheet will outline the specific information that the students need to include in their presentation. Student presentations will be conducted as a group with a visual aid, m ...
... Place students into eight groups (one for each planet) and give each group a planet along with a guideline sheet. The guideline sheet will outline the specific information that the students need to include in their presentation. Student presentations will be conducted as a group with a visual aid, m ...
Formation of the Solar System
... Stars are too far away from the Sun, and direct imaging cannot detect planets near them Current strategy involves watching for the small gravitational tag the planet exerts on its star The tag can be detected using the Doppler effect ...
... Stars are too far away from the Sun, and direct imaging cannot detect planets near them Current strategy involves watching for the small gravitational tag the planet exerts on its star The tag can be detected using the Doppler effect ...
The Outer Planets
... • Gravitational compression causes Jupiter to radiate more heat than it absorbs from the sun. • Heat is probably left over from the original collapse of the primordial nebula to form the Solar System • internal heat source drives the complex weather patterns in its atmosphere, unlike the Earth where ...
... • Gravitational compression causes Jupiter to radiate more heat than it absorbs from the sun. • Heat is probably left over from the original collapse of the primordial nebula to form the Solar System • internal heat source drives the complex weather patterns in its atmosphere, unlike the Earth where ...
workbook - teacher version
... a. Less than one year b. Every year c. More than one year NOTE: It takes Earth one year to revolve completely around the Sun, and it takes Jupiter 12 years because it is much farther from the Sun (see previous question). Since Earth and Jupiter are on opposite sides of the Sun in the diagram, it wil ...
... a. Less than one year b. Every year c. More than one year NOTE: It takes Earth one year to revolve completely around the Sun, and it takes Jupiter 12 years because it is much farther from the Sun (see previous question). Since Earth and Jupiter are on opposite sides of the Sun in the diagram, it wil ...
Is Anyone Out There? Solving the Drake Equation
... This is well known to astronomers… Ns = 200-400 billion = 2 to 4 × 1011 So far, so good… ...
... This is well known to astronomers… Ns = 200-400 billion = 2 to 4 × 1011 So far, so good… ...
Now - National Geographic Magazine, UK
... That one-to-two resonance wasn’t stable like the one between Neptune and Pluto; it was a brief, vigorous yank on the spring. As Jupiter and Saturn approached and pulled each other repeatedly at the same point in their orbits, those near-circular orbits were stretched into the ellipses we see today. ...
... That one-to-two resonance wasn’t stable like the one between Neptune and Pluto; it was a brief, vigorous yank on the spring. As Jupiter and Saturn approached and pulled each other repeatedly at the same point in their orbits, those near-circular orbits were stretched into the ellipses we see today. ...
The Diversity of Exoplanets – Statistical results I: mass
... Distribution, mass, separation – from RV Technique Very important for statistics = Radial Velocities: numbers, mass and orbital elements of planets. 51 Peg b proved the existence of extrasolar planets, but this planet had half the mass of Jupiter and was much heavier than expected Many of the later ...
... Distribution, mass, separation – from RV Technique Very important for statistics = Radial Velocities: numbers, mass and orbital elements of planets. 51 Peg b proved the existence of extrasolar planets, but this planet had half the mass of Jupiter and was much heavier than expected Many of the later ...
File
... 1. How much of Earth is water? How much of Earth is land? 70% of Earth is water. 30% of Earth is land. 2. Name 3 or 4 things that make Earth unique compared to other planets. Earth has humans, a breathable atmosphere, suitable temperature, and liquid water. 3. Why is Earth important when stu ...
... 1. How much of Earth is water? How much of Earth is land? 70% of Earth is water. 30% of Earth is land. 2. Name 3 or 4 things that make Earth unique compared to other planets. Earth has humans, a breathable atmosphere, suitable temperature, and liquid water. 3. Why is Earth important when stu ...
Eight Planets
... Saturn is the sixth planet from the Sun and the second largest. Galileo was the first to observe it with a telescope in 1610. Like Jupiter, Saturn is a gas planet, about 75% hydrogen and 25% helium. Saturn's rings, unlike the rings of the other planets, are very bright. ...
... Saturn is the sixth planet from the Sun and the second largest. Galileo was the first to observe it with a telescope in 1610. Like Jupiter, Saturn is a gas planet, about 75% hydrogen and 25% helium. Saturn's rings, unlike the rings of the other planets, are very bright. ...
What are the Jovian Planets? Characteristics of Jovian Planets
... Storms on Saturn • Large storms are rarer • Connected with seasons • ~ every 30 years outbreak of spots are seen in the equatorial ...
... Storms on Saturn • Large storms are rarer • Connected with seasons • ~ every 30 years outbreak of spots are seen in the equatorial ...
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), ...
Our solar system
... below. The way you choose to perform each task is up to you as long as all of the settings or conditions have been applied correctly. When completed, the document will be two pages long. The document will contain a bulleted list, a SmartArt, a picture, a textbox, and a table. Two illustrations have ...
... below. The way you choose to perform each task is up to you as long as all of the settings or conditions have been applied correctly. When completed, the document will be two pages long. The document will contain a bulleted list, a SmartArt, a picture, a textbox, and a table. Two illustrations have ...
The Jovian Planets + Pluto and the TNOs Jupiter 12 of Jupiter`s
... ☼ A cold, blue world only seen by naked eye under most favourable conditions. Discovered telescopically by Wm. Herschel in 1781. Blue colour due to CH4 absorption. Overall composition like Jupiter ☼ Rotation axis at 98° to ecliptic ☼ Magnetic field odd:- inclined at 55° to poles and well off-centre ...
... ☼ A cold, blue world only seen by naked eye under most favourable conditions. Discovered telescopically by Wm. Herschel in 1781. Blue colour due to CH4 absorption. Overall composition like Jupiter ☼ Rotation axis at 98° to ecliptic ☼ Magnetic field odd:- inclined at 55° to poles and well off-centre ...