Jupiter Reading Comprehension Worksheet
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
File - Homeschooling Mommie
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
... Jupiter is a giant ball of gas, made up of mostly hydrogen and helium. Its stripes and swirls are cold, windy clouds of ammonia and water. The largest swirling area of gas on Jupiter is a hurricane-like storm that is known as the Great Red Spot. This storm has been raging on Jupiter for hundreds of ...
Chapter 8 Moons, Rings, and Plutoids
... The ringlets within the ring system of Saturn are thought to be ...
... The ringlets within the ring system of Saturn are thought to be ...
Saturn - Peterborough Astronomical Association
... The ice chunks continued to orbit Saturn. Today we see them as a series of rings. Some are as big as a house while others are no larger than grains of sand or bits of gravel. They are also thin and delicate. If you measured the diameter from the outside edge of one side to the outside edge opposite ...
... The ice chunks continued to orbit Saturn. Today we see them as a series of rings. Some are as big as a house while others are no larger than grains of sand or bits of gravel. They are also thin and delicate. If you measured the diameter from the outside edge of one side to the outside edge opposite ...
Lecture 08a: Galilean moons - Sierra College Astronomy Home Page
... Composition of large satellites – Jupiter’s big four: ordered higher density to lower density; – Rock, metal, and ice; – The ice in Jupiter’s satellites is H2O; satellites of outer planets include other ices such as NH3 and CO2. ...
... Composition of large satellites – Jupiter’s big four: ordered higher density to lower density; – Rock, metal, and ice; – The ice in Jupiter’s satellites is H2O; satellites of outer planets include other ices such as NH3 and CO2. ...
Lesson Title: Layers of the Earth
... orbits are closest together? Which ones are really spread out? Are the planets’ orbits spaced at equal distances from the sun? Explanation: Upon returning to the classroom, discuss the students’ responses to the questions. Important ideas to emerge from the discussion include the following: ...
... orbits are closest together? Which ones are really spread out? Are the planets’ orbits spaced at equal distances from the sun? Explanation: Upon returning to the classroom, discuss the students’ responses to the questions. Important ideas to emerge from the discussion include the following: ...
Eight Planets
... has the most highly varied and interesting terrain of any of the planets. There is evidence of erosion in many places on Mars including large floods and small river systems (right). ...
... has the most highly varied and interesting terrain of any of the planets. There is evidence of erosion in many places on Mars including large floods and small river systems (right). ...
Jupiter (Jove) was the King of the Gods
... o Galilean moons are easily visible with binoculars; a few bands and the Great Red Spot can be seen with a small telescope. o Jupiter has 67 known satellites (as of 2013): the four large Galilean moons plus many more small ones some of which have not yet been named: o Jupiter's satellites are named ...
... o Galilean moons are easily visible with binoculars; a few bands and the Great Red Spot can be seen with a small telescope. o Jupiter has 67 known satellites (as of 2013): the four large Galilean moons plus many more small ones some of which have not yet been named: o Jupiter's satellites are named ...
Chapter 9
... in the solar system with an equatorial diameter of 119,300 kilometers (74,130 miles). Much of what is known about the planet is due to the Voyager explorations in 1980-81. Saturn is visibly flattened at the poles, a result of the very fast rotation of the planet on its axis. Its day is 10 hours, 39 ...
... in the solar system with an equatorial diameter of 119,300 kilometers (74,130 miles). Much of what is known about the planet is due to the Voyager explorations in 1980-81. Saturn is visibly flattened at the poles, a result of the very fast rotation of the planet on its axis. Its day is 10 hours, 39 ...
Chapter 11 The Jovian Planets
... Physical size = angular size x (2 π x distance)/360 (Read textbook page 30) Once the distances have been determined it is possible to calculate the orbital radius of the satellites. The mass of the planets can be calculated by measuring the orbital radius and the orbital period of the satellites (an ...
... Physical size = angular size x (2 π x distance)/360 (Read textbook page 30) Once the distances have been determined it is possible to calculate the orbital radius of the satellites. The mass of the planets can be calculated by measuring the orbital radius and the orbital period of the satellites (an ...
Solar System Formation
... -1900 Moulton & Chamberlin : Critic of the KantLaplace model: angular momentum Problem -1916 Chamberlin : close encounter with a star takes matter from the Sun=>Formation of a spiral nebulae=>cooling of the nebulae and collisional accretion of planetesimals -1917 Jeans : another problem with Laplace ...
... -1900 Moulton & Chamberlin : Critic of the KantLaplace model: angular momentum Problem -1916 Chamberlin : close encounter with a star takes matter from the Sun=>Formation of a spiral nebulae=>cooling of the nebulae and collisional accretion of planetesimals -1917 Jeans : another problem with Laplace ...
11/11/08 Chapter 9 The Outer Worlds… Jupiter Jupiter Jupiter`s
... respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in erup ...
... respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in erup ...
Chapter 9
... Interior of Uranus • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge suppor ...
... Interior of Uranus • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge suppor ...
637Lesson24
... from neutral N2 and ionized oxygen – similar to Titan. • Triton atmosphere made up predominately of N2. Methane is also present in the lower atmosphere. In addition further measurements have detected CO, CO2 and H. The H must be produced from methane, as on Titan, Uranus and Neptune. • The observed ...
... from neutral N2 and ionized oxygen – similar to Titan. • Triton atmosphere made up predominately of N2. Methane is also present in the lower atmosphere. In addition further measurements have detected CO, CO2 and H. The H must be produced from methane, as on Titan, Uranus and Neptune. • The observed ...
Ch10_Lecture
... Interior of Uranus • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge suppor ...
... Interior of Uranus • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge suppor ...
Discovery Uranus visible with naked eye(faint) discovered in 1781
... Pluto (and Charon) [figure 13.23, Plutoids.jpg] Pluto's discovery: additional perturbations of Uranus’s orbit → prediction by Lowell ~ 1905 Pluto found much smaller than predicted, via photographs ~ 1930 [discovering_pluto.jpg] ...
... Pluto (and Charon) [figure 13.23, Plutoids.jpg] Pluto's discovery: additional perturbations of Uranus’s orbit → prediction by Lowell ~ 1905 Pluto found much smaller than predicted, via photographs ~ 1930 [discovering_pluto.jpg] ...
Chapter 10 The Outer Worlds… Jupiter Jupiter Jupiter`s Interior
... respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in erup ...
... respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at least one of which originates from a geyser caught in erup ...
Solar System World Book at NASA A solar system is a group of
... 56 moons. The largest of Saturn's Pluto is so far from Earth that even powerful objects in the Oort cloud and the Kuiper belt may be chunks of rock moons, Titan, has an atmosphere telescopes reveal little detail of its surface. and ice known as planetesimals thicker than Earth's and a diameter The H ...
... 56 moons. The largest of Saturn's Pluto is so far from Earth that even powerful objects in the Oort cloud and the Kuiper belt may be chunks of rock moons, Titan, has an atmosphere telescopes reveal little detail of its surface. and ice known as planetesimals thicker than Earth's and a diameter The H ...
ring
... Jupiter: Key Concepts (1) Internal Structure: the interior of Jupiter is not uniform in density and temperature (2) Appearance: Jupiter‟s colored stripes are due to clouds formed at different levels in the atmosphere ...
... Jupiter: Key Concepts (1) Internal Structure: the interior of Jupiter is not uniform in density and temperature (2) Appearance: Jupiter‟s colored stripes are due to clouds formed at different levels in the atmosphere ...
largest and most massive planets [Figure 12
... Rings (both Jupiter and Saturn have ring systems) [figure 12-24, 25, 27, jupiter: figure 29,30] ...
... Rings (both Jupiter and Saturn have ring systems) [figure 12-24, 25, 27, jupiter: figure 29,30] ...
Pluto was discovered on February 18th 1930 by Clyde
... main gravitational body in the orbit. Many objects in our solar system have been classified as dwarf planets, the main ones being Pluto, Ceres and Eris. Pluto was discovered on February 18th 1930 by Clyde Tombaugh. Pluto is usually the farthest from the sun out of any of the main planets, however, d ...
... main gravitational body in the orbit. Many objects in our solar system have been classified as dwarf planets, the main ones being Pluto, Ceres and Eris. Pluto was discovered on February 18th 1930 by Clyde Tombaugh. Pluto is usually the farthest from the sun out of any of the main planets, however, d ...
Document
... • A Small World: Pluto is less than half the size of Mercury. • Reclassified: Since its discovery in 1930, Pluto has been called the ninth planet. However, in 2006, it was reclassified as a dwarf planet. ...
... • A Small World: Pluto is less than half the size of Mercury. • Reclassified: Since its discovery in 1930, Pluto has been called the ninth planet. However, in 2006, it was reclassified as a dwarf planet. ...
Neptune`s - P7
... Our solar system :The sun is at the centre of our solar system. It is a massive ball of gasses which produces as 100’000m hydrogen bombs exploding...every second! The nine planets of the solar system and more than 60 moons orbit the sun. ...
... Our solar system :The sun is at the centre of our solar system. It is a massive ball of gasses which produces as 100’000m hydrogen bombs exploding...every second! The nine planets of the solar system and more than 60 moons orbit the sun. ...