The Solar System
... Jupiter has four main moons, and dozens of smaller ones – there are 60 known moons so far ...
... Jupiter has four main moons, and dozens of smaller ones – there are 60 known moons so far ...
9 Intro to the Solar System
... What does distance from the Sun have to do with planet formation? • The Solar System is the name we give to our local cosmic backyard →A better way to think of it is all the stuff held sway by the Sun's gravity: The Sun itself, planets, moons, asteroids, comets, dust and very thin gas • If you took ...
... What does distance from the Sun have to do with planet formation? • The Solar System is the name we give to our local cosmic backyard →A better way to think of it is all the stuff held sway by the Sun's gravity: The Sun itself, planets, moons, asteroids, comets, dust and very thin gas • If you took ...
Mission to Planet X - The Education Fund
... planets. Since the mobile we make in this unit has planets that are to scale but not distances to scale, this video is perfect for teaching that aspect. Students will be amazed at the vast distance between the outlying planets Kids Astronomy: The Solar System This interactive site gives users a chan ...
... planets. Since the mobile we make in this unit has planets that are to scale but not distances to scale, this video is perfect for teaching that aspect. Students will be amazed at the vast distance between the outlying planets Kids Astronomy: The Solar System This interactive site gives users a chan ...
ph507-16-1exo1
... (often within a few per cent of an AU of one another). The Kepler-11 planetary system contains six transiting planets ranging in size from 1.8 to 4.2 times the radius of Earth. Five of these planets orbit in a tightly packed configuration with periods between 10 and 47 days. ...
... (often within a few per cent of an AU of one another). The Kepler-11 planetary system contains six transiting planets ranging in size from 1.8 to 4.2 times the radius of Earth. Five of these planets orbit in a tightly packed configuration with periods between 10 and 47 days. ...
Ecliptic 1 2 3 Three tell tale visual characteristics a planet:
... orbits, it is seen high in the west after sunset and sets around midnight. It is often said to be an “Evening Star” in the west. ...
... orbits, it is seen high in the west after sunset and sets around midnight. It is often said to be an “Evening Star” in the west. ...
Astronomical Units and Light Years #2
... While the sun is often referred to as the most important star within our solar system, it is certainly not the only one. There are too many stars for us to even begin to count. See how many you can count while gazing up at the sky on a clear night. Not only are there too many stars to count but, the ...
... While the sun is often referred to as the most important star within our solar system, it is certainly not the only one. There are too many stars for us to even begin to count. See how many you can count while gazing up at the sky on a clear night. Not only are there too many stars to count but, the ...
Why We Have Seasons
... - used Tycho’s data for the motion of mars to figure out the nature of planetary orbits - model was precice and did not require use of epicycles (<- no such thing as) - laws describe orbital shapes, changing speeds and the lengths of planetary years - Law #1~ orbits of planets are ellipses with sun ...
... - used Tycho’s data for the motion of mars to figure out the nature of planetary orbits - model was precice and did not require use of epicycles (<- no such thing as) - laws describe orbital shapes, changing speeds and the lengths of planetary years - Law #1~ orbits of planets are ellipses with sun ...
source - UC Berkeley Astronomy w
... are "aligned" by Coriolis forces (rotation). Aurorae – Charged particles can only travel along magnetic field lines. When solar wind particles reach the vicinity of a planet, they are captured by the magnetic field and funneled towards the poles (where the field lines originate). Eventually they hit ...
... are "aligned" by Coriolis forces (rotation). Aurorae – Charged particles can only travel along magnetic field lines. When solar wind particles reach the vicinity of a planet, they are captured by the magnetic field and funneled towards the poles (where the field lines originate). Eventually they hit ...
Astronomy 12 Final Review Sheet Sun
... are "aligned" by Coriolis forces (rotation). Aurorae – Charged particles can only travel along magnetic field lines. When solar wind particles reach the vicinity of a planet, they are captured by the magnetic field and funneled towards the poles (where the field lines originate). Eventually they hit ...
... are "aligned" by Coriolis forces (rotation). Aurorae – Charged particles can only travel along magnetic field lines. When solar wind particles reach the vicinity of a planet, they are captured by the magnetic field and funneled towards the poles (where the field lines originate). Eventually they hit ...
Chapter 29 Our Solar System
... 3. Relate gravity to the motions of celestial bodies. This means I can: Describe how mass, center of mass, and distance between 2 objects affects their gravitational pull on each other. 4. Compare and contrast the properties of the terrestrial planets. This means I can: a. Name the terrestrial plane ...
... 3. Relate gravity to the motions of celestial bodies. This means I can: Describe how mass, center of mass, and distance between 2 objects affects their gravitational pull on each other. 4. Compare and contrast the properties of the terrestrial planets. This means I can: a. Name the terrestrial plane ...
Unit 1: Astronomy Project
... For the week of February 11-14th, you should describe in a literate, four-page essay what a year on your planet is like. What does your sun look like in your sky (its size, its color, its brightness)? How do you tell time (days, months, seasons, years, etc.)? How high can you jump? What do(es) your ...
... For the week of February 11-14th, you should describe in a literate, four-page essay what a year on your planet is like. What does your sun look like in your sky (its size, its color, its brightness)? How do you tell time (days, months, seasons, years, etc.)? How high can you jump? What do(es) your ...
Mercury - School
... Distance = distance from sun compared to Earth Mass = mass of the planet compared to the mass of the Earth Diameter = distance from one side of the planet to the other through the centre of the planet. ...
... Distance = distance from sun compared to Earth Mass = mass of the planet compared to the mass of the Earth Diameter = distance from one side of the planet to the other through the centre of the planet. ...
some interesting facts about planets
... named after the Roman gods,like Mars was the god of war. ...
... named after the Roman gods,like Mars was the god of war. ...
Gravity
... 5. What paths do the planets follow as they move around the Sun? 6. What fundamental laws of nature explain the motions of objects on Earth as well as the motions of the planets? 7. Why don’t the planets fall into the Sun? 8. What keeps the same face of the Moon always pointed ...
... 5. What paths do the planets follow as they move around the Sun? 6. What fundamental laws of nature explain the motions of objects on Earth as well as the motions of the planets? 7. Why don’t the planets fall into the Sun? 8. What keeps the same face of the Moon always pointed ...
Explore the Solar System - Museum of Science, Boston
... because the forming planet has accreted or cleared out most of the nearby available material. ...
... because the forming planet has accreted or cleared out most of the nearby available material. ...
title of lesson plan - Discovery Education
... - What are some of its geological traits? - How many moons does the planet have? - How long is the planet's “day”? How long is its “year”? - What is the surface gravity like on the planet? - How did scientists learn about the planet? - Who first discovered the planet? When? - Over the course of hist ...
... - What are some of its geological traits? - How many moons does the planet have? - How long is the planet's “day”? How long is its “year”? - What is the surface gravity like on the planet? - How did scientists learn about the planet? - Who first discovered the planet? When? - Over the course of hist ...
Solar system topics
... Amazingly enough, we have found a number of meteorites on the Earth that came from Mars. One fell in Nakhla, Egypt, in 1911. It weighed 10 kg. The most famous one (ALH84001) was discovered in the Allan Hills of Antarctica. It is dated to be 4.5 billion years old. In a remarkable paper published in ...
... Amazingly enough, we have found a number of meteorites on the Earth that came from Mars. One fell in Nakhla, Egypt, in 1911. It weighed 10 kg. The most famous one (ALH84001) was discovered in the Allan Hills of Antarctica. It is dated to be 4.5 billion years old. In a remarkable paper published in ...
Largest moon in the solar system
... Second largest dwarf planet in the solar system. Pluto’s companion, Charon , is half the size & doesn’t orbit around Pluto. Pluto & Charon are small enough to fit inside the United States. Pluto is smaller than the Earth's moon. Some astronomers believe that Pluto was once a moon of Neptune bu ...
... Second largest dwarf planet in the solar system. Pluto’s companion, Charon , is half the size & doesn’t orbit around Pluto. Pluto & Charon are small enough to fit inside the United States. Pluto is smaller than the Earth's moon. Some astronomers believe that Pluto was once a moon of Neptune bu ...
Beyond Mnemonics: Pluto and the Nature of Science
... to the Earth; the combined mass of the Kuiper Belt is predicted to be significantly less than that of our planet. Reasoning and Controversy The debate on Pluto’s status reached a new level and urgency after the 2005 announcement that UB 313 is larger than Pluto (Brown et al., 2005), but astronomers ...
... to the Earth; the combined mass of the Kuiper Belt is predicted to be significantly less than that of our planet. Reasoning and Controversy The debate on Pluto’s status reached a new level and urgency after the 2005 announcement that UB 313 is larger than Pluto (Brown et al., 2005), but astronomers ...
Powerpoint for today
... (for circular orbits, a=radius). Translation: the larger a planet's orbit, the longer the period. ...
... (for circular orbits, a=radius). Translation: the larger a planet's orbit, the longer the period. ...
Class 2 Solar System Characteristics Formation Exosolar Planets
... dust can be detected because it absorbs ordinary starlight and re-emits it as infrared radiation. Features in dust disks may suggest the presence of planets. * Eclipsing binary: In an eclipsing double star system, the planet can be detected by finding variability in minima as it goes back and forth. ...
... dust can be detected because it absorbs ordinary starlight and re-emits it as infrared radiation. Features in dust disks may suggest the presence of planets. * Eclipsing binary: In an eclipsing double star system, the planet can be detected by finding variability in minima as it goes back and forth. ...
Planets beyond Neptune
Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.