Twinkle, twinkle little star, how I wonder what you are. Up
... I’m Mercury, I’m Mercury, the closest to the sun. I’m Mercury, I’m Mercury, the closest to the sun. Venus (spoken) I’m Venus, shining so bright. I’m Venus, shining so bright. Earth (spoken) For what it’s worth (snap snap) I’m the Earth. (snap snap) For what it’s worth (snap snap) I’m the Earth. (sna ...
... I’m Mercury, I’m Mercury, the closest to the sun. I’m Mercury, I’m Mercury, the closest to the sun. Venus (spoken) I’m Venus, shining so bright. I’m Venus, shining so bright. Earth (spoken) For what it’s worth (snap snap) I’m the Earth. (snap snap) For what it’s worth (snap snap) I’m the Earth. (sna ...
1 Chapter 2 - University of Minnesota
... 1) Except for a truly negligible precession, the direction of the earth’s rotation axis remains fixed in space, providing us with an invaluably constant frame of reference. 2) The earth’s rotation axis is used to define the north and south celestial poles, and also the celestial equator. 3) The nort ...
... 1) Except for a truly negligible precession, the direction of the earth’s rotation axis remains fixed in space, providing us with an invaluably constant frame of reference. 2) The earth’s rotation axis is used to define the north and south celestial poles, and also the celestial equator. 3) The nort ...
Planets - AState.edu
... Included: As students come into the classroom. I will have a model of the solar system on a table where all students can see the model. “Can anyone tell me what is sitting on the table? That’s right it is the solar system. What is our solar system mainly made of? Planets, the asteroid belt, stars, s ...
... Included: As students come into the classroom. I will have a model of the solar system on a table where all students can see the model. “Can anyone tell me what is sitting on the table? That’s right it is the solar system. What is our solar system mainly made of? Planets, the asteroid belt, stars, s ...
charts_set_6
... A passing star may dislodge Oort cloud objects, plunging them into Solar System, where they become long-period comets. If a Kuiper Belt object's orbit takes it close to, e.g., Neptune, its orbit may be changed and it may plunge towards the inner Solar System and become a short-period comet. ...
... A passing star may dislodge Oort cloud objects, plunging them into Solar System, where they become long-period comets. If a Kuiper Belt object's orbit takes it close to, e.g., Neptune, its orbit may be changed and it may plunge towards the inner Solar System and become a short-period comet. ...
Magnetic fields
... to let you explore the Solar System in more detail. We’re going to do this by imagining it’s the far future. Mankind has colonized space and can safely transport people to other places in the solar system. Your job is going to be to create a tourist brochure for a location in the Solar System where ...
... to let you explore the Solar System in more detail. We’re going to do this by imagining it’s the far future. Mankind has colonized space and can safely transport people to other places in the solar system. Your job is going to be to create a tourist brochure for a location in the Solar System where ...
2nd Leaflet: A Tour of the Human Orrery
... arrived at the planet on 2004 July 1, and will orbit Saturn for at least four years. Saturn is most famous for its distinctive ring system. For many years these rings seemed to be unique in the known solar system. However, faint rings were discovered around Uranus in 1977, and shortly thereafter als ...
... arrived at the planet on 2004 July 1, and will orbit Saturn for at least four years. Saturn is most famous for its distinctive ring system. For many years these rings seemed to be unique in the known solar system. However, faint rings were discovered around Uranus in 1977, and shortly thereafter als ...
Guided Notes
... Inner Planets – Mercury, Venus, Earth, Mars Asteroid Belt – asteroids and dwarf planet Ceres Outer Planets- Jupiter, Saturn, Uranus, Neptune Kuiper Belt-Pluto, Eris, 800 other objects (AKA Trans-Neptunian Objects or TNOs) Oort Cloud- comets, ice, and dust at the outer limits of the solar system ...
... Inner Planets – Mercury, Venus, Earth, Mars Asteroid Belt – asteroids and dwarf planet Ceres Outer Planets- Jupiter, Saturn, Uranus, Neptune Kuiper Belt-Pluto, Eris, 800 other objects (AKA Trans-Neptunian Objects or TNOs) Oort Cloud- comets, ice, and dust at the outer limits of the solar system ...
Saturn
... Second largest planet, after Jupiter Lowest density of all the planets Gravity on Saturn is about 1.08 times the gravity on Earth On Tuesday Jan. 11th the Cassini spacecraft passed within 69 kilometers (43 miles) of the surface of Rhea ...
... Second largest planet, after Jupiter Lowest density of all the planets Gravity on Saturn is about 1.08 times the gravity on Earth On Tuesday Jan. 11th the Cassini spacecraft passed within 69 kilometers (43 miles) of the surface of Rhea ...
Exam 3
... The rings of all the Jovian planets are found near to the planet, while moons are found farther out. This is because a) moons which are too near the planet will be torn apart by differential gravity forces b) moons too close to the planet will colide with one another and break each other apart c) mo ...
... The rings of all the Jovian planets are found near to the planet, while moons are found farther out. This is because a) moons which are too near the planet will be torn apart by differential gravity forces b) moons too close to the planet will colide with one another and break each other apart c) mo ...
ESS Solar System Astronomy Exam
... A.)past or B.)future? Astronomers estimate that the nebular cloud from which our solar system formed contained about two to three times the mass of the Sun and was about 100 astronomical units (AU) across. This massive loosely-bound cloud of dust, ice particles, and gases (primarily hydrogen and hel ...
... A.)past or B.)future? Astronomers estimate that the nebular cloud from which our solar system formed contained about two to three times the mass of the Sun and was about 100 astronomical units (AU) across. This massive loosely-bound cloud of dust, ice particles, and gases (primarily hydrogen and hel ...
THE PLANETS
... You’ve studied the Solar System in lower grades, so this is just a review. We will create a chart for this information, but first, look over the next few slides and keep these in mind while we’re working on this lesson. ...
... You’ve studied the Solar System in lower grades, so this is just a review. We will create a chart for this information, but first, look over the next few slides and keep these in mind while we’re working on this lesson. ...
Categorizing Solar System Objects
... Ida, asteroid –Ida is one of the over 100,000 asteroids in the asteroid belt. Jupiter, planet – Jupiter is the largest planet in the Solar System. Luna, satellite of Earth – Mars, planet – Mathilde, asteroid – Neptune, planet – Phobos, satellite of Mars – This is one of Mars’ two small moons (the ot ...
... Ida, asteroid –Ida is one of the over 100,000 asteroids in the asteroid belt. Jupiter, planet – Jupiter is the largest planet in the Solar System. Luna, satellite of Earth – Mars, planet – Mathilde, asteroid – Neptune, planet – Phobos, satellite of Mars – This is one of Mars’ two small moons (the ot ...
Minor Members of the Solar System
... Charon is classified as its moon Has two known smaller moons, Nix and Hydra ...
... Charon is classified as its moon Has two known smaller moons, Nix and Hydra ...
Test and answer key - Solar Physics and Space Weather
... The following 10 questions, from 41 to 50, are voluntary questions that are intended to improve the teaching and learning of this course in the future. I appreciate your cooperation. Your answer to these 10 questions (or the lack of answers) will not affect your grade in this exam, since your grade ...
... The following 10 questions, from 41 to 50, are voluntary questions that are intended to improve the teaching and learning of this course in the future. I appreciate your cooperation. Your answer to these 10 questions (or the lack of answers) will not affect your grade in this exam, since your grade ...
PLANETS
... participant. The frosting is placed on the waxed paper. 4) Using the knife, put some frosting "glue" on one side of the butterscotch candy, representing the Sun. Place this candy at the center of the plate. 5) Using the same method, have students affix each of the eight planets to its appropriate or ...
... participant. The frosting is placed on the waxed paper. 4) Using the knife, put some frosting "glue" on one side of the butterscotch candy, representing the Sun. Place this candy at the center of the plate. 5) Using the same method, have students affix each of the eight planets to its appropriate or ...
Planetary Science - Laboratory for Atmospheric and Space Physics
... the study of Mars. Studies indicate that the Martian atmosphere has changed greatly over time, from a thicker atmosphere to the thin atmosphere we see now. What happened to the Martian atmosphere? Why did it change so dramatically? These are questions we will help address through the LASP-led NASA M ...
... the study of Mars. Studies indicate that the Martian atmosphere has changed greatly over time, from a thicker atmosphere to the thin atmosphere we see now. What happened to the Martian atmosphere? Why did it change so dramatically? These are questions we will help address through the LASP-led NASA M ...
The Solar System
... The Scale of the Solar System 2 • We can now use radar to determine the distance to Venus. • When Venus is at its greatest elongation (the furthest from the Sun when viewed from Earth), we can use trigonometry to determine the distance from the Sun to the Earth – Radar gives distance, d, to Venus. ...
... The Scale of the Solar System 2 • We can now use radar to determine the distance to Venus. • When Venus is at its greatest elongation (the furthest from the Sun when viewed from Earth), we can use trigonometry to determine the distance from the Sun to the Earth – Radar gives distance, d, to Venus. ...
8. Welcome to the Solar System
... largest being Ceres at about 1,000 km in diameter, (remember that the diameter of the Earth is about 12,800 km) and only another five or so having diameters over 300 km. • There are roughly 200 or so with diameters over 100 km. There may be on the order of a million with a diameter of kilometer or m ...
... largest being Ceres at about 1,000 km in diameter, (remember that the diameter of the Earth is about 12,800 km) and only another five or so having diameters over 300 km. • There are roughly 200 or so with diameters over 100 km. There may be on the order of a million with a diameter of kilometer or m ...
solar system - cayugascience
... largest being Ceres at about 1,000 km in diameter, (remember that the diameter of the Earth is about 12,800 km) and only another five or so having diameters over 300 km. • There are roughly 200 or so with diameters over 100 km. There may be on the order of a million with a diameter of kilometer or m ...
... largest being Ceres at about 1,000 km in diameter, (remember that the diameter of the Earth is about 12,800 km) and only another five or so having diameters over 300 km. • There are roughly 200 or so with diameters over 100 km. There may be on the order of a million with a diameter of kilometer or m ...
The Solar System
... • NASA scientists now believe that the dark material is lag (residue) from the sublimation (evaporation) of water ice on the surface of Iapetus,possibly darkened further upon exposure to sunlight. Because of its slow rotation of 79 days (equal to its revolution and the longest in the Saturnian syst ...
... • NASA scientists now believe that the dark material is lag (residue) from the sublimation (evaporation) of water ice on the surface of Iapetus,possibly darkened further upon exposure to sunlight. Because of its slow rotation of 79 days (equal to its revolution and the longest in the Saturnian syst ...
Planetary Debate - TXESS Revolution
... Challenge: You are a tour operator for Galaxy Guides promoting tourist travel (could be real or virtual tourism) to the planetary body or bodies which you have been assigned. 1. Day one –team assignments (4 or 5 participants). Team 1: Team 2: Team 3: Team 4: Team 5: Team 6: Team 7: Team 8: Team 9: ...
... Challenge: You are a tour operator for Galaxy Guides promoting tourist travel (could be real or virtual tourism) to the planetary body or bodies which you have been assigned. 1. Day one –team assignments (4 or 5 participants). Team 1: Team 2: Team 3: Team 4: Team 5: Team 6: Team 7: Team 8: Team 9: ...
The Jovian Planets
... They both formed far from the Sun where ices were very common, so their cores are rich in ices. They probably grew slowly since collisions would be slower and less frequent that far from the Sun. It is thought that they didn’t gather as much gas as Jupiter and Saturn. So they are mostly core with “t ...
... They both formed far from the Sun where ices were very common, so their cores are rich in ices. They probably grew slowly since collisions would be slower and less frequent that far from the Sun. It is thought that they didn’t gather as much gas as Jupiter and Saturn. So they are mostly core with “t ...
ppt
... Low-energy collisions => planetesimals formed and grew Within 5 AU, the accreting particles were composed of CAIs, silicates, Fe, Ni. At distance > 5 AU, just inside Jupiter’s present-day orbit, water-ice could form and be included in planetesimals. Further out, ~30 AU, methane-ice could form and b ...
... Low-energy collisions => planetesimals formed and grew Within 5 AU, the accreting particles were composed of CAIs, silicates, Fe, Ni. At distance > 5 AU, just inside Jupiter’s present-day orbit, water-ice could form and be included in planetesimals. Further out, ~30 AU, methane-ice could form and b ...