The Scientific Revolution - Online
... The Heliocentric System offers a simple explanation for varying brightness and retrograde motion ...
... The Heliocentric System offers a simple explanation for varying brightness and retrograde motion ...
ppt
... Not clear how small brown dwarfs could be; could they be as small as “planets”? How do we distinguish planets and BDs? ...
... Not clear how small brown dwarfs could be; could they be as small as “planets”? How do we distinguish planets and BDs? ...
Helping to Make God Real: Creation Part II - Days 1-3
... to explain why you would or would not live there. (Provide 2 minutes for children to look at the handout and prepare their explanation.) Hold up your hand if you decided you should live on your planet? (Call on one or two with hands raised to provide an explanation. There probably will not be very m ...
... to explain why you would or would not live there. (Provide 2 minutes for children to look at the handout and prepare their explanation.) Hold up your hand if you decided you should live on your planet? (Call on one or two with hands raised to provide an explanation. There probably will not be very m ...
AST101 Lecture 16 Extra Solar Planets
... Direct searches are difficult because stars are so bright. ...
... Direct searches are difficult because stars are so bright. ...
Neptune - Mid-Pacific Institute
... Magnetic Field is off-centered and at a large angle to it’s rotation axis ...
... Magnetic Field is off-centered and at a large angle to it’s rotation axis ...
Exoplanets. I
... How did we find the planets? • Mercury, Venus, Mars, Jupiter, Saturn: orbital motion • Uranus: chance imaging (see by Galileo) • Neptune: predicted from gravitational perturbations; imaging • Pluto: orbital motion (guided by erroneous prediction) • Ceres, Vesta, Pallas, Juno: orbital motions • ...
... How did we find the planets? • Mercury, Venus, Mars, Jupiter, Saturn: orbital motion • Uranus: chance imaging (see by Galileo) • Neptune: predicted from gravitational perturbations; imaging • Pluto: orbital motion (guided by erroneous prediction) • Ceres, Vesta, Pallas, Juno: orbital motions • ...
Chapter 8
... The Roche limit of the Jovian planets (Distance of the rings from the planets, in planets radius) ...
... The Roche limit of the Jovian planets (Distance of the rings from the planets, in planets radius) ...
23.3 The Outer Planets
... Pluto: Planet X Pluto’s orbit is highly eccentric, causing it to occasionallyy travel inside the orbit of Neptune, where it resided from 1979 through February 1999. ...
... Pluto: Planet X Pluto’s orbit is highly eccentric, causing it to occasionallyy travel inside the orbit of Neptune, where it resided from 1979 through February 1999. ...
Earth in the Universe
... Evolution of Solar System • About 5 billion years old. Started as a gas cloud many times the size of today’s solar system. Gravitation caused the cloud to condense, most of the mass was pulled to the center and formed our sun. • After Earth and other planets were formed, their gravity pulled on oth ...
... Evolution of Solar System • About 5 billion years old. Started as a gas cloud many times the size of today’s solar system. Gravitation caused the cloud to condense, most of the mass was pulled to the center and formed our sun. • After Earth and other planets were formed, their gravity pulled on oth ...
Lecture 5 - Orbits, Sizes, Precession
... This means that Vega appears to move from +0.1″ to 0.1″ with respect to distant stars over a year’s observation D(pc) = 1/p(″) = 1/0.1 = 10 pc ...
... This means that Vega appears to move from +0.1″ to 0.1″ with respect to distant stars over a year’s observation D(pc) = 1/p(″) = 1/0.1 = 10 pc ...
Solar System 3
... relatively new designation for the region of the outer solar system beyond the orbit of Neptune (whose largest known member, by this designation, has (until recently) been Pluto). • The Kuiper Belt is also believed to be the primary home of most of the long-period comets. • In recent years, a signif ...
... relatively new designation for the region of the outer solar system beyond the orbit of Neptune (whose largest known member, by this designation, has (until recently) been Pluto). • The Kuiper Belt is also believed to be the primary home of most of the long-period comets. • In recent years, a signif ...
Chapter 27 PLANETS OF THE SOLAR SYSTEM
... approx. 5 billion years ago. (Rotating cloud from which sun &planets formed is called the solar nebula.) Center became hotter and denser due to forces from collisions and gravity. When temp=107 oC, hydrogen fusion began &Sol (THE SUN) formed. The sun contains 99% of the mass of the former solar nebu ...
... approx. 5 billion years ago. (Rotating cloud from which sun &planets formed is called the solar nebula.) Center became hotter and denser due to forces from collisions and gravity. When temp=107 oC, hydrogen fusion began &Sol (THE SUN) formed. The sun contains 99% of the mass of the former solar nebu ...
lecture3
... science – a correct theory should have some ‘beauty’. This notion continues today; ‘beauty’ guides our models.) ...
... science – a correct theory should have some ‘beauty’. This notion continues today; ‘beauty’ guides our models.) ...
The Center of It All
... Approximately 109 planet Earths would fit on the surface of the sun and more than one million planets Earths would fit inside the sun. The sun is often personified in mythologies: Greeks call is Helios and the Romans call it Sol. In Japan it is called Amaterasu. The sun is 70 % hydrogen, 28% h ...
... Approximately 109 planet Earths would fit on the surface of the sun and more than one million planets Earths would fit inside the sun. The sun is often personified in mythologies: Greeks call is Helios and the Romans call it Sol. In Japan it is called Amaterasu. The sun is 70 % hydrogen, 28% h ...
Coursework 6 File
... 1. A planet of mass Mp forms around a star with mass M∗ with separation r, and an orbiting satellite forms around the planet with semimajor axis asat . By considering the tidal acceleration exerted by the central star on the planet–satellite system (that acts to pull them apart), and the gravitation ...
... 1. A planet of mass Mp forms around a star with mass M∗ with separation r, and an orbiting satellite forms around the planet with semimajor axis asat . By considering the tidal acceleration exerted by the central star on the planet–satellite system (that acts to pull them apart), and the gravitation ...
... waning- when the moon is getting smaller/less light. waxing- when the moon is getting larger/brighter. telescope- a tool that makes objects appear larger. elliptical- an oval/egg shaped orbit. lunar- means moon. Pluto- a former planet that is the smallest and farthest in our solar system. Jupiter- l ...
Mercury Venus Mars Jupiter Saturn Uranus Neptune Type (rocky or
... least 63 moons, the 4 main top), Great White Spot (like these moons are irregular largest one in the solar ones are called Galilean Jupiter's Great White Spot 13 known rings, 27 in shape. Triton, is its most system. It also has 2 Satellites - one of the main known moons, Named notable and only circu ...
... least 63 moons, the 4 main top), Great White Spot (like these moons are irregular largest one in the solar ones are called Galilean Jupiter's Great White Spot 13 known rings, 27 in shape. Triton, is its most system. It also has 2 Satellites - one of the main known moons, Named notable and only circu ...
A Survey of the Planets Mercury Difficult to observe
... by Voyager 2 (1989). (Five rings known.) Satellites -- current known total is 8 Two prior to Voyager (Nereid, Triton) Voyager discovered six Triton (D=2700 km) In a retrograde orbit! (Captured?) Thin N2, CH4 atmosphere Bright icy (N2, CH4) surface Geyser-like eruptions? Voyager 2 flyby, 1989. Neptun ...
... by Voyager 2 (1989). (Five rings known.) Satellites -- current known total is 8 Two prior to Voyager (Nereid, Triton) Voyager discovered six Triton (D=2700 km) In a retrograde orbit! (Captured?) Thin N2, CH4 atmosphere Bright icy (N2, CH4) surface Geyser-like eruptions? Voyager 2 flyby, 1989. Neptun ...
ASTR2050 Intro A&A NAMES: ____________________ ____________________ Work sheet
... Build a scale model of the solar system, including the sizes and orbital radii of the sun and planets. Most of the data you need can be found in Kutner, Appendices B and D, and Figure 17.3. Show the units in the following lists. 1. What celestial object did you use to set the scale, and what did you ...
... Build a scale model of the solar system, including the sizes and orbital radii of the sun and planets. Most of the data you need can be found in Kutner, Appendices B and D, and Figure 17.3. Show the units in the following lists. 1. What celestial object did you use to set the scale, and what did you ...
DO IT YOURSELF SIMPLE TEMPLATE FORMAT
... Our Solar System consists of many types of objects circling around the Sun, held in their orbits by gravity. Name all of the objects you can think of that orbit the Sun. Write down what you know about each one. This activity will look specifically at planets, which are relatively large objects circl ...
... Our Solar System consists of many types of objects circling around the Sun, held in their orbits by gravity. Name all of the objects you can think of that orbit the Sun. Write down what you know about each one. This activity will look specifically at planets, which are relatively large objects circl ...
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.