Chapter 12 Asteroids, Comets, and Dwarf Planets What are
... Why are there very few asteroids beyond Jupiter’s orbit? A. There was no rocky material beyond Jupiter’s orbit. B. The heaviest rocks sank towards the center of the solar system. C. Ice could form in the outer solar system. D. A passing star probably stripped away all of those asteroids, even if the ...
... Why are there very few asteroids beyond Jupiter’s orbit? A. There was no rocky material beyond Jupiter’s orbit. B. The heaviest rocks sank towards the center of the solar system. C. Ice could form in the outer solar system. D. A passing star probably stripped away all of those asteroids, even if the ...
Construct Planetary Orbits Around the Sun Student Activity Sheet
... 1. Place a blank sheet of paper on top of the cardboard and place two thumbtacks or pins about 3 cm apart. 2. Tie the string into a circle with a circumference of 15 to 20 cm. Loop the string around the thumbtacks. With someone holding the tacks or pins, place a pencil inside the loop and pull it ta ...
... 1. Place a blank sheet of paper on top of the cardboard and place two thumbtacks or pins about 3 cm apart. 2. Tie the string into a circle with a circumference of 15 to 20 cm. Loop the string around the thumbtacks. With someone holding the tacks or pins, place a pencil inside the loop and pull it ta ...
Decline of Western Civilization (extended) knowledge of ancient
... Earth Rotates: Daily motion of Sun, Moon, Stars and Planets [diurnal.avi] Inferior Planet overtakes Earth: Planet undergoes retrograde motion Earth overtakes Superior Planet : Planet undergoes retrograde motion Moon’s motion about Earth: Phases of the Moon (and occasional eclipses) [eclipser_shadows ...
... Earth Rotates: Daily motion of Sun, Moon, Stars and Planets [diurnal.avi] Inferior Planet overtakes Earth: Planet undergoes retrograde motion Earth overtakes Superior Planet : Planet undergoes retrograde motion Moon’s motion about Earth: Phases of the Moon (and occasional eclipses) [eclipser_shadows ...
Document
... stars revolve around the Earth which is fixed) “Geocentric Universe”: fixed relationship between stars Ptolemy (c. 100 A.D.) refined the system introduced (most notably) by Hipparchus to explain the observed motions of the stars and planets. Copernicus (1473-1543) proposed a heliocentric model of pl ...
... stars revolve around the Earth which is fixed) “Geocentric Universe”: fixed relationship between stars Ptolemy (c. 100 A.D.) refined the system introduced (most notably) by Hipparchus to explain the observed motions of the stars and planets. Copernicus (1473-1543) proposed a heliocentric model of pl ...
Homework 2 (Due Sept 18, 2014)
... this chamber, a feather would fall at the same rate as a rock.! c. When an astronaut goes on a space walk outside the Space Station, she will quickly ! float away from the station unless she has a tether holding her to the station.! d. If the Sun were magically replaced with a giant rock that had pr ...
... this chamber, a feather would fall at the same rate as a rock.! c. When an astronaut goes on a space walk outside the Space Station, she will quickly ! float away from the station unless she has a tether holding her to the station.! d. If the Sun were magically replaced with a giant rock that had pr ...
Unit Review Name
... 25. Describe two examples of services that satellites provide to people on Earth. (2 ...
... 25. Describe two examples of services that satellites provide to people on Earth. (2 ...
Models of the Solar System
... planets were discovered with the aid of telescopes: • Uranus in 1781 • Neptune in 1846 • Pluto in 1930 (Pluto was later reclassified as a dwarf ...
... planets were discovered with the aid of telescopes: • Uranus in 1781 • Neptune in 1846 • Pluto in 1930 (Pluto was later reclassified as a dwarf ...
Grade 3 Social Studies
... What is the Solar System? Our solar system is the Sun and the planets that orbit, or spin, around it. The Sun is really a star that is only about 93,000,000 miles from us. Until 2006 we had nine known planets, Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. Astronomers then ...
... What is the Solar System? Our solar system is the Sun and the planets that orbit, or spin, around it. The Sun is really a star that is only about 93,000,000 miles from us. Until 2006 we had nine known planets, Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. Astronomers then ...
Chapter 4 Gravitation and the Waltz of the Planets
... 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 toward the Earth? ...
... 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 toward the Earth? ...
The Sun and Planets Homework Solutions 4.
... millisecond pulsar1 and is most likely made of crystalline carbon, a material with far greater density than diamond. The eccentricity of its orbit is not known precisely, we only know that it is less than 0.06. For this problem, assume a semi-major axis of 0.004 AU and an eccentricity of 0.06. c) HD ...
... millisecond pulsar1 and is most likely made of crystalline carbon, a material with far greater density than diamond. The eccentricity of its orbit is not known precisely, we only know that it is less than 0.06. For this problem, assume a semi-major axis of 0.004 AU and an eccentricity of 0.06. c) HD ...
PPT
... Apparent Motions of the Planets: Like the Sun and Moon, the planets move on the celestial sphere with respect to the background of stars. Most of the time a planet moves eastward in direct or prograde motion, in the same direction as the Sun and the Moon, but from time to time it moves westward in r ...
... Apparent Motions of the Planets: Like the Sun and Moon, the planets move on the celestial sphere with respect to the background of stars. Most of the time a planet moves eastward in direct or prograde motion, in the same direction as the Sun and the Moon, but from time to time it moves westward in r ...
Sample Midterm
... Planet Pickett. The planet orbits another star just like the Sun and can only be observed telescopically. Assume that astronomers have been able to determine that it orbits with a semi-major axis of 10 AU and has a mass of 90 Earths. Further observations reveal that the planet has at least 8 satelli ...
... Planet Pickett. The planet orbits another star just like the Sun and can only be observed telescopically. Assume that astronomers have been able to determine that it orbits with a semi-major axis of 10 AU and has a mass of 90 Earths. Further observations reveal that the planet has at least 8 satelli ...
Possible patterns in the distribution of planetary formation regions
... still some residuals. The plot in Fig. 2 shows that there appears to be a symmetry of the data around Jupiter and the oscillation can be accurately fitted by means of a 5-degree polynomial fit, which is also shown in Fig. 2. The rms of the residuals of the polynomial fit is just 3%, which is quite g ...
... still some residuals. The plot in Fig. 2 shows that there appears to be a symmetry of the data around Jupiter and the oscillation can be accurately fitted by means of a 5-degree polynomial fit, which is also shown in Fig. 2. The rms of the residuals of the polynomial fit is just 3%, which is quite g ...
28_starships
... calculations were wrong, and Pluto, turned out to be smaller than Earth's Moon — too small to account for the perturbations, in any case. In June 1978, James W. Christy noticed that in one image, Pluto's point of light seemed to have a bump on it. He went back and looked at other photographs and Plu ...
... calculations were wrong, and Pluto, turned out to be smaller than Earth's Moon — too small to account for the perturbations, in any case. In June 1978, James W. Christy noticed that in one image, Pluto's point of light seemed to have a bump on it. He went back and looked at other photographs and Plu ...
Chapter 24: The Solar System Study Guide
... 1. The inner planets are also known as gas giants. 2. It takes the inner planets less time to orbit the Earth than it takes the outer planets. 3. Mercury’s lack of an atmosphere causes it to experience extreme day and night temperatures. 4. Mercury has two moons. 5. Mercury has many craters on its s ...
... 1. The inner planets are also known as gas giants. 2. It takes the inner planets less time to orbit the Earth than it takes the outer planets. 3. Mercury’s lack of an atmosphere causes it to experience extreme day and night temperatures. 4. Mercury has two moons. 5. Mercury has many craters on its s ...
Inferior planets.
... March 13, 1781. By 1790 it was realized that its orbit was not as expected. Conclusion: another unknown planet was “perturbing” its motion. • 1845- Adams calculated a position for the unknown planet and sent it to the Astronomer Royal Airy. Airy gave him a test problem to check him out, but Adams re ...
... March 13, 1781. By 1790 it was realized that its orbit was not as expected. Conclusion: another unknown planet was “perturbing” its motion. • 1845- Adams calculated a position for the unknown planet and sent it to the Astronomer Royal Airy. Airy gave him a test problem to check him out, but Adams re ...
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 ...
23.3 Note Guide The Outer Planets In 2004, the space probe
... The _____________________________ probe, carried into space by the Cassini orbiter, will descend to Titan’s surface for further studies In this section, we’ll take a clue from Cassini and explore the outer planets—Jupiter, Saturn, Neptune, Uranus, and Pluto ...
... The _____________________________ probe, carried into space by the Cassini orbiter, will descend to Titan’s surface for further studies In this section, we’ll take a clue from Cassini and explore the outer planets—Jupiter, Saturn, Neptune, Uranus, and Pluto ...
etlife_exoplanets - University of Glasgow
... We can tell that planets are there by the effect they have on their star. ...
... We can tell that planets are there by the effect they have on their star. ...
Additional Exercises for Chapter 4 Computations of Copernicus and
... 58. Which of the equations of Section 4.7 confirms that the locations of the two positions of a planet at which its distance to the Sun are least (the perihelion position) and greatest (the aphelion position) are both on the major axis? How does it confirm this? 59. Use the data from Table 4.2 to co ...
... 58. Which of the equations of Section 4.7 confirms that the locations of the two positions of a planet at which its distance to the Sun are least (the perihelion position) and greatest (the aphelion position) are both on the major axis? How does it confirm this? 59. Use the data from Table 4.2 to co ...
Space is Big…
... The Sun 1,390,000 km - 1 solar diameter (108.97 X the Earth) Sirus (WHITE STAR)1.7 solar diameter Pollux - 9.1 solar diameter Arcturus - 26 solar diameter ...
... The Sun 1,390,000 km - 1 solar diameter (108.97 X the Earth) Sirus (WHITE STAR)1.7 solar diameter Pollux - 9.1 solar diameter Arcturus - 26 solar diameter ...
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.