Unit 5: Review Game Questions
... 16) In the inner part of the nebula only metals and rocks were able to condense because of the high temperatures, whereas hydrogen compounds, although more abundant, were only able to condense in the cooler outer regions. 17) They were formed by condensation and accretion in a disk of gas around the ...
... 16) In the inner part of the nebula only metals and rocks were able to condense because of the high temperatures, whereas hydrogen compounds, although more abundant, were only able to condense in the cooler outer regions. 17) They were formed by condensation and accretion in a disk of gas around the ...
Earth is the third planet from the Sun. It is a rocky planet and the fifth
... one moon and no rings. © www.thecurriculumcorner.com ...
... one moon and no rings. © www.thecurriculumcorner.com ...
File
... earth, affecting the ocean tides, and slowing the Earth’s rotation with its gravity. The Earth and its solar system are part of a bigger area of space called the Milky Way galaxy. The Milky Way is a galaxy named this way because it appears in the sky as a “Milky” glowing band. In 1610 Galileo Galile ...
... earth, affecting the ocean tides, and slowing the Earth’s rotation with its gravity. The Earth and its solar system are part of a bigger area of space called the Milky Way galaxy. The Milky Way is a galaxy named this way because it appears in the sky as a “Milky” glowing band. In 1610 Galileo Galile ...
University of Manchester Primary PGCE Appendix I
... they have learned about The Solar System consists of the Sun and other bodies which orbit it (held in planets orbiting around the place by gravity) – includes planets, dwarf planets and asteroids. Sun and how this makes up N.B. gravity keeps them in place because they have been pulled towards the Su ...
... they have learned about The Solar System consists of the Sun and other bodies which orbit it (held in planets orbiting around the place by gravity) – includes planets, dwarf planets and asteroids. Sun and how this makes up N.B. gravity keeps them in place because they have been pulled towards the Su ...
Topic E: Astrophysics E1 Introduction to the Universe.
... http://solarsystem.nasa.gov/planets/profile.cfm?Object=Mars 1. What is the solar system? 2. What are planets? 3. What shape are their orbits? 4. How are the planes of their orbits orientated? 5. In what order are the planets? 6. Disregarding Pluto, which was probably not formed with the other planet ...
... http://solarsystem.nasa.gov/planets/profile.cfm?Object=Mars 1. What is the solar system? 2. What are planets? 3. What shape are their orbits? 4. How are the planes of their orbits orientated? 5. In what order are the planets? 6. Disregarding Pluto, which was probably not formed with the other planet ...
Ch. 3 The Solar System - Hillsdale Community Schools
... •The attractive force between two objects. •The strength depends on the mass of the object and the distance between the objects. ...
... •The attractive force between two objects. •The strength depends on the mass of the object and the distance between the objects. ...
Study regarding the landscape arrangement of the green space
... Material and Method Taking into account the Astronomic Observatory and its role, the alleys were designed according to the Tycho Brahe solar system pattern published on 1587. In the description of Tychonic system, the objects on the blue orbits (Moon, Sunday) gravitate around the Earth. The objects ...
... Material and Method Taking into account the Astronomic Observatory and its role, the alleys were designed according to the Tycho Brahe solar system pattern published on 1587. In the description of Tychonic system, the objects on the blue orbits (Moon, Sunday) gravitate around the Earth. The objects ...
The Planets
... • Like the asteroids in the inner solar system, most Kuiper belt comets move in nearly circular orbits that lie roughly in the same plane as the planets. ...
... • Like the asteroids in the inner solar system, most Kuiper belt comets move in nearly circular orbits that lie roughly in the same plane as the planets. ...
Outer or Jovian Planets - Academic Computer Center
... has a thin atmosphere. • Triton orbits backwards and at high inclination. This might mean that it was “captured” by Neptune. It might be a Kuiper belt object. May also be similar to Pluto. Unmanned missions to Neptune: Voyager 2 (1989) ...
... has a thin atmosphere. • Triton orbits backwards and at high inclination. This might mean that it was “captured” by Neptune. It might be a Kuiper belt object. May also be similar to Pluto. Unmanned missions to Neptune: Voyager 2 (1989) ...
Earth
... diameter of about 1000 km, down to the size of pebbles. Sixteen asteroids have a diameter of 240 km or greater. They have been found inside Earth's orbit to beyond Saturn's orbit. Most, however, are contained within a main belt that exists between the orbits of Mars and Jupiter. Astronomers have cal ...
... diameter of about 1000 km, down to the size of pebbles. Sixteen asteroids have a diameter of 240 km or greater. They have been found inside Earth's orbit to beyond Saturn's orbit. Most, however, are contained within a main belt that exists between the orbits of Mars and Jupiter. Astronomers have cal ...
8.1 Touring the Night Sky Pg. 308 #1
... 4. Terrestrial planets are the 4 planets closest to the Sun. They have rocky surfaces similar to Earth’s. The next four planets are known as gas giants. They are called that because they are mostly made up of gases and liquids. 5. The difference between stars and planets are; stars are massive colle ...
... 4. Terrestrial planets are the 4 planets closest to the Sun. They have rocky surfaces similar to Earth’s. The next four planets are known as gas giants. They are called that because they are mostly made up of gases and liquids. 5. The difference between stars and planets are; stars are massive colle ...
Group: (list all members)
... about each planet that the groups should be familiar with. The teacher will explain that students should work together when coming up with the answer. iv. Once the group has agreed on an answer, it’s the job of the first person to run to the correct planet and tag the wall. Whichever group tags the ...
... about each planet that the groups should be familiar with. The teacher will explain that students should work together when coming up with the answer. iv. Once the group has agreed on an answer, it’s the job of the first person to run to the correct planet and tag the wall. Whichever group tags the ...
Understanding the Outer Planets and Planetary Atmospheres
... context: nothing on Earth is like it! What a wonderful surprise that the ringed planets are just as beautiful and scientifically compelling seen close-up. We now know that planetary rings, once thought unique to the planet Saturn, exist around all the giant planets. These rings are not solid objects ...
... context: nothing on Earth is like it! What a wonderful surprise that the ringed planets are just as beautiful and scientifically compelling seen close-up. We now know that planetary rings, once thought unique to the planet Saturn, exist around all the giant planets. These rings are not solid objects ...
Click www.ondix.com to visit our student-to
... The Sun is the richest source of electromagnetic energy in the solar system. It is because of its light and heat given off. The Sun's nearest known astral neighbor is Proxima Centauri, a red dwarf star that is about 4.3 light years away. The whole solar system, together with the local stars visible ...
... The Sun is the richest source of electromagnetic energy in the solar system. It is because of its light and heat given off. The Sun's nearest known astral neighbor is Proxima Centauri, a red dwarf star that is about 4.3 light years away. The whole solar system, together with the local stars visible ...
AN INTRODUCTION TO ASTRONOMY Dr. Uri Griv Department of Physics, Ben-Gurion University
... Explanation: Yes it does look like Saturn, but Saturn is only one of four giant ringed planets in our Solar System. And while Saturn has the brightest rings, this system of rings and moons actually belongs to planet Uranus, imaged here in near-infrared light by the Antu telescope at the ESO Paranal ...
... Explanation: Yes it does look like Saturn, but Saturn is only one of four giant ringed planets in our Solar System. And while Saturn has the brightest rings, this system of rings and moons actually belongs to planet Uranus, imaged here in near-infrared light by the Antu telescope at the ESO Paranal ...
How was the Solar System Formed?
... such as Iron and Nickel. Also called Terrestrial Planets. These planets lose their gases because gravity is not strong enough to hold gas. Dense Materials sink to the center of the planets. The planets form layers. Inner planets: Solid, Rocky , Dense, Hotter! ...
... such as Iron and Nickel. Also called Terrestrial Planets. These planets lose their gases because gravity is not strong enough to hold gas. Dense Materials sink to the center of the planets. The planets form layers. Inner planets: Solid, Rocky , Dense, Hotter! ...
Chapter3 - The Science of Astronomy-ppt
... object remains in motion unless a force acts to stop it or change its direction. • Tycho’s observations of a comet and supernova showed that the heavens could change. • The lack of noticeable stellar parallax was simply due to the fact that the stars were much farther away than anyone had previously ...
... object remains in motion unless a force acts to stop it or change its direction. • Tycho’s observations of a comet and supernova showed that the heavens could change. • The lack of noticeable stellar parallax was simply due to the fact that the stars were much farther away than anyone had previously ...
presentation format
... Most elaborate geocentric model was developed by the astronomer Ptolemy Ptolemy made lots of small adjustments to the basic picture to try to better match the observed position of planets Always preserved Earth at center (geocentric) and circular orbits, but had some orbits off center, some orbit ...
... Most elaborate geocentric model was developed by the astronomer Ptolemy Ptolemy made lots of small adjustments to the basic picture to try to better match the observed position of planets Always preserved Earth at center (geocentric) and circular orbits, but had some orbits off center, some orbit ...
night watch - Warren Astronomical Society
... -2The best method for determining the radius of Pluto, as it is for Neptune, is to observe a stellar occultation. It was predicted that Pluto would pass near a 15th magnitude star in 1965, and so the passage was observed very closely by several observatories to see if the star would be occulted. We ...
... -2The best method for determining the radius of Pluto, as it is for Neptune, is to observe a stellar occultation. It was predicted that Pluto would pass near a 15th magnitude star in 1965, and so the passage was observed very closely by several observatories to see if the star would be occulted. We ...
p35-KIDS_Layout 1
... Neptune has a faint and fragmented ring system (labeled “arcs”), which was first detected during the 1960s and confirmed by Voyager 2. Moons Neptune has 14 known moons. Triton is the largest Neptunian moon, comprising more than 99.5% of the mass in orbit around Neptune, and it is the only one massiv ...
... Neptune has a faint and fragmented ring system (labeled “arcs”), which was first detected during the 1960s and confirmed by Voyager 2. Moons Neptune has 14 known moons. Triton is the largest Neptunian moon, comprising more than 99.5% of the mass in orbit around Neptune, and it is the only one massiv ...
What makes a planet habitable?
... That’s not the end of the story. While the size and composition of both planets and stars are important, so is time. Big bright stars burn out far more quickly than smaller ones. The brightest burn for only a few million years, then flame out. Meanwhile, our sun has been shining steadily for 4.5 bill ...
... That’s not the end of the story. While the size and composition of both planets and stars are important, so is time. Big bright stars burn out far more quickly than smaller ones. The brightest burn for only a few million years, then flame out. Meanwhile, our sun has been shining steadily for 4.5 bill ...
Day-26
... newly forming star that was much hotter than the protoSun. What would we expect about its planets? A. The planets orbit at random angles around the star. B. Rocky planets might be formed over a wider range of distances than in our Solar System. C. The star would be “naked,” without a surrounding dis ...
... newly forming star that was much hotter than the protoSun. What would we expect about its planets? A. The planets orbit at random angles around the star. B. Rocky planets might be formed over a wider range of distances than in our Solar System. C. The star would be “naked,” without a surrounding dis ...
Jovian Planets
... occupy orbits in the outer solar system at distances ranging from 5 (Jupiter) to 30 (Neptune) times the Earth’s distance from the Sun. Unlike the terrestrial planets that make up our inner solar system—Mercury, Venus, Earth, and Mars—the Jovian planets do not have solid surfaces. Instead, they are c ...
... occupy orbits in the outer solar system at distances ranging from 5 (Jupiter) to 30 (Neptune) times the Earth’s distance from the Sun. Unlike the terrestrial planets that make up our inner solar system—Mercury, Venus, Earth, and Mars—the Jovian planets do not have solid surfaces. Instead, they are c ...
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.