1 DATE DUE: Name: Ms. Terry J. Boroughs Geology 305 Section
... 13. The principle of uniformitarianism is also known as: A. The Principle of Inclusions. D. Answers A. and B. B. The principle of uniformity. E. Answers B. and C. C. “The present is the key to the past.” F. None of these 14. Nuclear fusion within the interior of stars occurs when the interior temper ...
... 13. The principle of uniformitarianism is also known as: A. The Principle of Inclusions. D. Answers A. and B. B. The principle of uniformity. E. Answers B. and C. C. “The present is the key to the past.” F. None of these 14. Nuclear fusion within the interior of stars occurs when the interior temper ...
Review for Exam 2
... 5) How long does it take for stars and planets to be born? 6) What is a brown dwarf? How does it change over 6me? 7) What is the boundary in mass between stars and brown dwarfs? 8) What 3 ...
... 5) How long does it take for stars and planets to be born? 6) What is a brown dwarf? How does it change over 6me? 7) What is the boundary in mass between stars and brown dwarfs? 8) What 3 ...
Properties of the Planets
... Sunrise on the Planets A simulation The next series of slides are meant to help you visualize the effect of the vast distances of the Solar System by simulating, in a simple way, what sunrise would look like from each planet, taking into account its distance from the Sun. At the bottom of each slid ...
... Sunrise on the Planets A simulation The next series of slides are meant to help you visualize the effect of the vast distances of the Solar System by simulating, in a simple way, what sunrise would look like from each planet, taking into account its distance from the Sun. At the bottom of each slid ...
Solar System Debris
... • Charon is less than 9 Pluto diameters away from Pluto (compare: Moon ¼ diameter of Earth, and 30 Earth diameters away from Earth) • Charon orbit is tilted 119o to Pluto’s orbit around the Sun (i.e. it is in the equatorial plane of Pluto) • Despite their small size, they are tidally looked in a 1:1 ...
... • Charon is less than 9 Pluto diameters away from Pluto (compare: Moon ¼ diameter of Earth, and 30 Earth diameters away from Earth) • Charon orbit is tilted 119o to Pluto’s orbit around the Sun (i.e. it is in the equatorial plane of Pluto) • Despite their small size, they are tidally looked in a 1:1 ...
Chapter 30 - Cloudfront.net
... Ring and Moons of Jupiter Galilean moon any one of the four largest satellites of Jupiter—Io, Europa, Ganymede, and Callisto - that were discovered by Galileo in 1610 In addition to the four large moons discovered by Galileo, scientists have observed dozens of smaller moons around Jupiter. Of ...
... Ring and Moons of Jupiter Galilean moon any one of the four largest satellites of Jupiter—Io, Europa, Ganymede, and Callisto - that were discovered by Galileo in 1610 In addition to the four large moons discovered by Galileo, scientists have observed dozens of smaller moons around Jupiter. Of ...
Solar System PPT
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
Lesson 2 - Verona Public Schools
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
- La Salle Elementary School
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
The Newtonian Revolution: The discovery of natural law
... apparently fixed stars, or (2) the stars are so vastly far away that their parallax motion is undetectably small with their technology. • The Greeks went with (1). Doh!…. They were wrong! – they should’ve gone with door #2!! ...
... apparently fixed stars, or (2) the stars are so vastly far away that their parallax motion is undetectably small with their technology. • The Greeks went with (1). Doh!…. They were wrong! – they should’ve gone with door #2!! ...
Lecture 3
... While the other three gas planets in the solar system - Jupiter, Uranus and Neptune - have rings orbiting around them, Saturn's are by far the largest and most spectacular. With a thickness of about 1 kilometer (3,200 feet) or less, they span up to 282,000 km. Named alphabetically in the order they ...
... While the other three gas planets in the solar system - Jupiter, Uranus and Neptune - have rings orbiting around them, Saturn's are by far the largest and most spectacular. With a thickness of about 1 kilometer (3,200 feet) or less, they span up to 282,000 km. Named alphabetically in the order they ...
Navigating by the Stars
... The orbits of the planets are ellipses with the Sun at one of the foci. This is now called Kepler's First Law or The Law of Ellipses. What is an ellipse? Glad you asked. An ellipse is a closed, curved shape that is defined by two foci. An ellipse is a like a flattened circle. In fact, if both of th ...
... The orbits of the planets are ellipses with the Sun at one of the foci. This is now called Kepler's First Law or The Law of Ellipses. What is an ellipse? Glad you asked. An ellipse is a closed, curved shape that is defined by two foci. An ellipse is a like a flattened circle. In fact, if both of th ...
CS3_Ch 2 - Leon County Schools
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
... Dwarf Planets (cont.) • Unlike a planet, a dwarf planet has objects similar in mass orbiting nearby or crossing its orbital path. • Ceres is the smallest dwarf planet with a diameter of about 950 km. • Pluto is so far from the Sun that it takes about 248 years to complete one orbit. • Eris is the l ...
search for extrasolar planets
... controlled for beam combination • Example: five four-telescope interferometers (8m each), hundreds of km apart • Goal: many resolution elements across disk of planets found by TPF ...
... controlled for beam combination • Example: five four-telescope interferometers (8m each), hundreds of km apart • Goal: many resolution elements across disk of planets found by TPF ...
William Borucki
... hours to over 1000 days and orbital distances range from 0.01 AU to many AU. Several planets have been discovered orbiting binary stars and one in a triple-star system. Preliminary estimates of the size distribution suggest two populations; one for large planets formed when gas and dust were abundan ...
... hours to over 1000 days and orbital distances range from 0.01 AU to many AU. Several planets have been discovered orbiting binary stars and one in a triple-star system. Preliminary estimates of the size distribution suggest two populations; one for large planets formed when gas and dust were abundan ...
The Solar Sytem (Story Book)
... length of its day and the tilt of its axis are similar to those of Earth. Mars takes about two years to circle the Sun at an average distance of 228 million km (141.7 million mi). The possibility of life on Mars, now or in the distant past, is one of the major questions in astronomy. More space prob ...
... length of its day and the tilt of its axis are similar to those of Earth. Mars takes about two years to circle the Sun at an average distance of 228 million km (141.7 million mi). The possibility of life on Mars, now or in the distant past, is one of the major questions in astronomy. More space prob ...
Which object is a meteor?
... (must be an asteroid) • Not Object 4 because it is not in space (meteorite?) • CORRECT ANSWER: Object 3 (a meteor is a streak of light produced by friction with air when an object (rock) from space enters a planet’s atmosphere) ...
... (must be an asteroid) • Not Object 4 because it is not in space (meteorite?) • CORRECT ANSWER: Object 3 (a meteor is a streak of light produced by friction with air when an object (rock) from space enters a planet’s atmosphere) ...
1 HoNoRS227 Examination #3 Name
... Because the star is so close that we should have received radio signals from the planet years ago. C Because the radio signals cannot penetrate the Earth’s atmosphere from outer space. D Because we are able to hear radio waves, this should have been discovered long ago. *E Because massive blue giant ...
... Because the star is so close that we should have received radio signals from the planet years ago. C Because the radio signals cannot penetrate the Earth’s atmosphere from outer space. D Because we are able to hear radio waves, this should have been discovered long ago. *E Because massive blue giant ...
May 8, 2012 - Plummer Pumas Science
... The Sun’s temperature was much hotter and it was much larger. __________________________________________________________________________________________________ __________________________________________________________________________________________________ ________________________________________ ...
... The Sun’s temperature was much hotter and it was much larger. __________________________________________________________________________________________________ __________________________________________________________________________________________________ ________________________________________ ...
FIT_colloq_2nov2012
... (1) A “planet” is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit. (2) A “dwarf planet” is a cele ...
... (1) A “planet” is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit. (2) A “dwarf planet” is a cele ...
The Sun and planets
... On our stage, the role of main actor cannot but be conferred to the Sun, a star like many others in space, but very special for us because from the remains of its formation all the planets and the smaller bodies that rotate around it, and of which we are a part, have originated. The Sun is so big th ...
... On our stage, the role of main actor cannot but be conferred to the Sun, a star like many others in space, but very special for us because from the remains of its formation all the planets and the smaller bodies that rotate around it, and of which we are a part, have originated. The Sun is so big th ...
The core of the Sun is
... It was produced by nuclear fusion in stars. It was made by our Sun. It was made by nuclear fission of uranium and other radioactive ...
... It was produced by nuclear fusion in stars. It was made by our Sun. It was made by nuclear fission of uranium and other radioactive ...
File
... Earth and Neptune differences Earth: is the only planet in our solar system known to harbor life. All of the things we need to survive are provided under a thin layer of atmosphere that separates us from the uninhabitable void of space. Earth is made up of complex, interactive systems that are ofte ...
... Earth and Neptune differences Earth: is the only planet in our solar system known to harbor life. All of the things we need to survive are provided under a thin layer of atmosphere that separates us from the uninhabitable void of space. Earth is made up of complex, interactive systems that are ofte ...
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.