Black Dwarf Presentation
... Black Dwarf Facts • Universe is too young to create black dwarfs • White dwarf decay length is unknown • No proof of existence • Matter would be extremely dense • Thought to be the final product of our Sun ...
... Black Dwarf Facts • Universe is too young to create black dwarfs • White dwarf decay length is unknown • No proof of existence • Matter would be extremely dense • Thought to be the final product of our Sun ...
Planets, Galaxies and Constellations
... but two and a half times that of all the other planets in the Solar System combined. Jupiter is a gas giant, along with Saturn. (Uranus and Neptune are ice giants.) Jupiter was known to astronomers of ancient times.The Romans named it after their god Jupiter. ...
... but two and a half times that of all the other planets in the Solar System combined. Jupiter is a gas giant, along with Saturn. (Uranus and Neptune are ice giants.) Jupiter was known to astronomers of ancient times.The Romans named it after their god Jupiter. ...
downloading
... largest known object in the classical Kuiper belt (KBO not in a confirmed resonance with Neptune). • The dwarf planet Pluto (39 AU average) is the largest known object in the Kuiper belt. When discovered in 1930, it was considered to be the ninth planet; this changed in 2006 with the adoption of a f ...
... largest known object in the classical Kuiper belt (KBO not in a confirmed resonance with Neptune). • The dwarf planet Pluto (39 AU average) is the largest known object in the Kuiper belt. When discovered in 1930, it was considered to be the ninth planet; this changed in 2006 with the adoption of a f ...
Lesson 3 The Solar System
... • Beyond the asteroid belt is another group of planets that includes Jupiter, Saturn, Uranus, and Neptune, known as the outer planets. • They are gas giants which are huge planets with a small, metallic core, and a thick atmosphere. • The gas giants all have rings and many moons. • They spin very ra ...
... • Beyond the asteroid belt is another group of planets that includes Jupiter, Saturn, Uranus, and Neptune, known as the outer planets. • They are gas giants which are huge planets with a small, metallic core, and a thick atmosphere. • The gas giants all have rings and many moons. • They spin very ra ...
Lesson 3 The Solar System - Delaware Valley School District
... • Beyond the asteroid belt is another group of planets that includes Jupiter, Saturn, Uranus, and Neptune, known as the outer planets. • They are gas giants which are huge planets with a small, metallic core, and a thick atmosphere. ...
... • Beyond the asteroid belt is another group of planets that includes Jupiter, Saturn, Uranus, and Neptune, known as the outer planets. • They are gas giants which are huge planets with a small, metallic core, and a thick atmosphere. ...
Unit 3 *The Solar System* 6th Grade Space Science
... System by characteristics, such as: shape, and appearance, what they orbit, how large they are, and how far away their orbits are from the Sun. ...
... System by characteristics, such as: shape, and appearance, what they orbit, how large they are, and how far away their orbits are from the Sun. ...
Our Solar System
... What’s in Our Solar System? • Our Solar System consists of a central star (the Sun), the nine planets orbiting the sun, moons, asteroids, comets, meteors, interplanetary gas, dust, and all the “space” in between them. • The nine planets of the Solar System are named for Greek and Roman Gods and ...
... What’s in Our Solar System? • Our Solar System consists of a central star (the Sun), the nine planets orbiting the sun, moons, asteroids, comets, meteors, interplanetary gas, dust, and all the “space” in between them. • The nine planets of the Solar System are named for Greek and Roman Gods and ...
Astro 18 - Planets and Planetary Systems
... 3) New Comet: A new comet is discovered and studies of its motion indicate that it orbits the Sun with a period of 100 years. a) Use Kepler's third law in its original form to find the comet's average distance from the Sun (i.e. find the semi-major axis of the comet's orbit). Be sure to include uni ...
... 3) New Comet: A new comet is discovered and studies of its motion indicate that it orbits the Sun with a period of 100 years. a) Use Kepler's third law in its original form to find the comet's average distance from the Sun (i.e. find the semi-major axis of the comet's orbit). Be sure to include uni ...
Keplar`s Laws of Planetary Motion
... Keplar devised three laws which describe the motions of the planets. Keplar's First Law Bodies move around the sun in elliptical orbits, with the sun at one focus. The other focus is empty. An ellipse is basically a squashed circle. All bodies orbit in an ellipse, although some are more elliptical t ...
... Keplar devised three laws which describe the motions of the planets. Keplar's First Law Bodies move around the sun in elliptical orbits, with the sun at one focus. The other focus is empty. An ellipse is basically a squashed circle. All bodies orbit in an ellipse, although some are more elliptical t ...
Astro 18-- Planets and Planetary Systems – Fall 2010 Homework 2
... 3) New Comet: A new comet is discovered and studies of its motion indicate that it orbits the Sun with a period of 100 years. a) Use Kepler's third law in its original form to find the comet's average distance from the Sun (i.e. find the semi-major axis of the comet's orbit). Be sure to include uni ...
... 3) New Comet: A new comet is discovered and studies of its motion indicate that it orbits the Sun with a period of 100 years. a) Use Kepler's third law in its original form to find the comet's average distance from the Sun (i.e. find the semi-major axis of the comet's orbit). Be sure to include uni ...
The Whole Darn Thing!
... Terrestrial planets form inside the ice line. Dense, small, no rings/moons, little H and He. Jovian planets form outside the ice line. Light, large, moons/rings, mostly H and He. Mercury, Venus, Earth, Mars, ice line, asteroid belt, Jupiter, Saturn, Uranus, Neptune, Kuiper belt Besides planets, we h ...
... Terrestrial planets form inside the ice line. Dense, small, no rings/moons, little H and He. Jovian planets form outside the ice line. Light, large, moons/rings, mostly H and He. Mercury, Venus, Earth, Mars, ice line, asteroid belt, Jupiter, Saturn, Uranus, Neptune, Kuiper belt Besides planets, we h ...
Conjunctions an Oppositions
... Planets without a telescope look just like stars Except, they move relative to the stars ...
... Planets without a telescope look just like stars Except, they move relative to the stars ...
Conjunctions an Oppositions
... Planets without a telescope look just like stars Except, they move relative to the stars ...
... Planets without a telescope look just like stars Except, they move relative to the stars ...
The Planet Hike - City of Dripping Springs
... beginning of the Kuiper Belt. KBO’s are Kuiper Belt Objects, which are large bodies of ice and rocks. ...
... beginning of the Kuiper Belt. KBO’s are Kuiper Belt Objects, which are large bodies of ice and rocks. ...
28.1-notes - Stout Middle School
... space between the stars. These clouds mostly consist of hydrogen gas, helium gas with small amounts of other elements and dust. (basically clouds of gas & dust) At first the collapse of an interstellar cloud is slow, but it gradually accelerates and the cloud becomes much denser than its center. If ...
... space between the stars. These clouds mostly consist of hydrogen gas, helium gas with small amounts of other elements and dust. (basically clouds of gas & dust) At first the collapse of an interstellar cloud is slow, but it gradually accelerates and the cloud becomes much denser than its center. If ...
The Solar System
... thought that the Main Belt was the debris ring left over from a destroyed planet. But it’s much more likely that such a planet was, in fact, prevented from ever forming by Jupiter’s strong gravitational pull. There is no scientific explanation for Bode’s law, and it may well be a simple mathematical ...
... thought that the Main Belt was the debris ring left over from a destroyed planet. But it’s much more likely that such a planet was, in fact, prevented from ever forming by Jupiter’s strong gravitational pull. There is no scientific explanation for Bode’s law, and it may well be a simple mathematical ...
File
... Visited by Pioneer 10 in 1973, then Pioneer 11, Voyager 1 and 2, Ulysses, Cassini-Huygens, and Galileo orbited it for 8 years ...
... Visited by Pioneer 10 in 1973, then Pioneer 11, Voyager 1 and 2, Ulysses, Cassini-Huygens, and Galileo orbited it for 8 years ...
Describing the Solar System File
... that of mars and Jupiter are thousands of asteroids. Asteroids could be the remains of a smashed up planet or moon. Asteroids are lumps of rock ranging from a tennis ball in size up to 700km across. It is thought that Jupiter’s gravity keeps the asteroids smeared out around this belt and stops ...
... that of mars and Jupiter are thousands of asteroids. Asteroids could be the remains of a smashed up planet or moon. Asteroids are lumps of rock ranging from a tennis ball in size up to 700km across. It is thought that Jupiter’s gravity keeps the asteroids smeared out around this belt and stops ...
The Planets
... • Saturn’s rings are more noticeable than the other planets’. • Saturn is smaller than Jupiter, but larger than Uranus and Neptune. ...
... • Saturn’s rings are more noticeable than the other planets’. • Saturn is smaller than Jupiter, but larger than Uranus and Neptune. ...
Space – Our Solar System
... • No longer considered a Planet • Is the second most massive known dwarf planet in the Solar System (after Eris) • Pluto's mass is less than 0.24 percent that of the Earth • Its diameter is roughly 66% that of our Moon ...
... • No longer considered a Planet • Is the second most massive known dwarf planet in the Solar System (after Eris) • Pluto's mass is less than 0.24 percent that of the Earth • Its diameter is roughly 66% that of our Moon ...
The Outer Planets
... Beyond the orbit of Mars, the solar system becomes a very strange place of huge gaseous planets, peculiar ring systems, and many strange moons. The three outermost planets—Uranus, Neptune, and Pluto—were discovered only after the invention of the telescope. ...
... Beyond the orbit of Mars, the solar system becomes a very strange place of huge gaseous planets, peculiar ring systems, and many strange moons. The three outermost planets—Uranus, Neptune, and Pluto—were discovered only after the invention of the telescope. ...
Solar System Study Guide
... Saturn: A planet with 100s rings (made of dust, ice & rock), takes 29.5 years to orbit the Sun. Neptune: The beautiful blue/green planet (due to methane gas), strong winds (up to 1,300 mph), and takes 165 years to orbit the Sun. Uranus: The planet that spins on its side (horizontal), has many moons ...
... Saturn: A planet with 100s rings (made of dust, ice & rock), takes 29.5 years to orbit the Sun. Neptune: The beautiful blue/green planet (due to methane gas), strong winds (up to 1,300 mph), and takes 165 years to orbit the Sun. Uranus: The planet that spins on its side (horizontal), has many moons ...
Planet and Space Web Search
... 5) What is between Mars and Jupiter? ______________________________ 6) Go to the top of the web page. There is a button labeled “Planets.” Click on each of the different planets and read about them. Write one interesting fact about each planet. Planet Name: ________________ Fact: ...
... 5) What is between Mars and Jupiter? ______________________________ 6) Go to the top of the web page. There is a button labeled “Planets.” Click on each of the different planets and read about them. Write one interesting fact about each planet. Planet Name: ________________ Fact: ...
Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite. That is, it is in direct orbit of the Sun, and is massive enough for its shape to be in hydrostatic equilibrium under its own gravity, but has not cleared the neighborhood around its orbit.The term dwarf planet was adopted in 2006 as part of a three-way categorization of bodies orbiting the Sun, brought about by an increase in discoveries of objects farther away from the Sun than Neptune that rivaled Pluto in size, and finally precipitated by the discovery of an even more massive object, Eris. The exclusion of dwarf planets from the roster of planets by the IAU has been both praised and criticized; it was said to be the ""right decision"" by astronomer Mike Brown, who discovered Eris and other new dwarf planets, but has been rejected by Alan Stern, who had coined the term dwarf planet in 1990.The International Astronomical Union (IAU) currently recognizes five dwarf planets: Ceres, Pluto, Haumea, Makemake, and Eris. Brown criticizes this official recognition: ""A reasonable person might think that this means that there are five known objects in the solar system which fit the IAU definition of dwarf planet, but this reasonable person would be nowhere close to correct.""It is suspected that another hundred or so known objects in the Solar System are dwarf planets. Estimates are that up to 200 dwarf planets may be found when the entire region known as the Kuiper belt is explored, and that the number may exceed 10,000 when objects scattered outside the Kuiper belt are considered. Individual astronomers recognize several of these, and in August 2011 Mike Brown published a list of 390 candidate objects, ranging from ""nearly certain"" to ""possible"" dwarf planets. Brown currently identifies eleven known objects – the five accepted by the IAU plus 2007 OR10, Quaoar, Sedna, Orcus, 2002 MS4 and Salacia – as ""virtually certain"", with another dozen highly likely. Stern states that there are more than a dozen known dwarf planets.However, only two of these bodies, Ceres and Pluto, have been observed in enough detail to demonstrate that they actually fit the IAU's definition. The IAU accepted Eris as a dwarf planet because it is more massive than Pluto. They subsequently decided that unnamed trans-Neptunian objects with an absolute magnitude brighter than +1 (and hence a diameter of ≥838 km assuming a geometric albedo of ≤1) are to be named under the assumption that they are dwarf planets. The only two such objects known at the time, Makemake and Haumea, went through this naming procedure and were declared to be dwarf planets. The question of whether other likely objects are dwarf planets has never been addressed by the IAU. The classification of bodies in other planetary systems with the characteristics of dwarf planets has not been addressed.