Planet Project Jupiter
... Jupiter is known as the largest planet of all the other planets. It is a Jovian planet also known as an outer planet. The mass is 2.5 times greater than all other planets combined. Over a thousand earths could fit into its volume. It is the fifth planet from the sun ...
... Jupiter is known as the largest planet of all the other planets. It is a Jovian planet also known as an outer planet. The mass is 2.5 times greater than all other planets combined. Over a thousand earths could fit into its volume. It is the fifth planet from the sun ...
Slide 1
... asteroid — for instance, comets have recently been discovered there, and Ceres, once thought of only as an asteroid, is now also considered a dwarf http://www.space.com/51-asteroids-formation-discovery-and-exploration.html planet. ...
... asteroid — for instance, comets have recently been discovered there, and Ceres, once thought of only as an asteroid, is now also considered a dwarf http://www.space.com/51-asteroids-formation-discovery-and-exploration.html planet. ...
AUST – HORIZON AND BEYOND part 1
... Do stars move? Yes like us (our entire solar system) they are rotating around the centre of our galaxy. In relation to the size of the galaxy this movement is quite slow. ...
... Do stars move? Yes like us (our entire solar system) they are rotating around the centre of our galaxy. In relation to the size of the galaxy this movement is quite slow. ...
Unformatted file
... cooling down, the smaller will have cooled down before the larger, and will be further ahead in their development. Now Mars is very much smaller than the earth, and must have cooled at its surface millions of years before the earth did. Hence, if a story of life began on Mars at all, it began long b ...
... cooling down, the smaller will have cooled down before the larger, and will be further ahead in their development. Now Mars is very much smaller than the earth, and must have cooled at its surface millions of years before the earth did. Hence, if a story of life began on Mars at all, it began long b ...
Page 1 of 10 Name: Space Systems Learning Target #1: I CAN
... _____ 73. An exploding star, called a _______________ disturbed the cloud. _____ 74. The _______________ of dust and gas began to stick together. _____ 75. The cloud began to collapse. _____ 76. Near the center only ________________ material could stand the heat. _____ 77. This turned the cloud into ...
... _____ 73. An exploding star, called a _______________ disturbed the cloud. _____ 74. The _______________ of dust and gas began to stick together. _____ 75. The cloud began to collapse. _____ 76. Near the center only ________________ material could stand the heat. _____ 77. This turned the cloud into ...
Review 2
... Internal structure of our Sun and its chemical composition. What is the convection zone on the Sun and what are the granules and supergranules? What is the temperature in the Sun’s core? What is the photosphere, chromosphere and corona? What is their temperature and what causes their color? What is ...
... Internal structure of our Sun and its chemical composition. What is the convection zone on the Sun and what are the granules and supergranules? What is the temperature in the Sun’s core? What is the photosphere, chromosphere and corona? What is their temperature and what causes their color? What is ...
ASU Chain Reaction - Volume 3 - LeRoy Eyring Center For Solid
... the past few decades. Planetary geologists study the extreme conditions on Earth and other planets in an effort to understand what those bodies are like and how they formed. Astrobiologists study life under Earth’s most hostile conditions in an effort to predict where life might exist on other plane ...
... the past few decades. Planetary geologists study the extreme conditions on Earth and other planets in an effort to understand what those bodies are like and how they formed. Astrobiologists study life under Earth’s most hostile conditions in an effort to predict where life might exist on other plane ...
IN THE CENTRE OF THE SUN IT ABOUT 15 MILLION DEGREES
... • Data from Magellan's imaging radar shows that much of the surface of Venus is covered by lava flows. There are several large shield volcanoes (similar to Hawaii or Olympus Mons). • Recently announced findings indicate that Venus is still volcanically active, but only in a few hot spots; for the mo ...
... • Data from Magellan's imaging radar shows that much of the surface of Venus is covered by lava flows. There are several large shield volcanoes (similar to Hawaii or Olympus Mons). • Recently announced findings indicate that Venus is still volcanically active, but only in a few hot spots; for the mo ...
solar system? - Smithsonian Education
... Telescope has been busy taking images of planets in our solar system, never-before-seen stars, galaxies, and nebulae. Built with the most precise scientific instruments, it focuses its sight on OBJECTS DEEP IN SPACE. Its eight-footwide mirror collects more than 160,000 times the amount of light our ...
... Telescope has been busy taking images of planets in our solar system, never-before-seen stars, galaxies, and nebulae. Built with the most precise scientific instruments, it focuses its sight on OBJECTS DEEP IN SPACE. Its eight-footwide mirror collects more than 160,000 times the amount of light our ...
Class Hours Instructor Dr. Kent Montgomery
... describe what we can observe with the unaided eye and how these simple observations have been used to create models of the solar system. It will also include a brief historical overview of the significant astronomical events and people in the past. The second part of this course will focus on the pr ...
... describe what we can observe with the unaided eye and how these simple observations have been used to create models of the solar system. It will also include a brief historical overview of the significant astronomical events and people in the past. The second part of this course will focus on the pr ...
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 ...
Chapter 1: Origin of the earth
... the rate of retreat, we can calculate that all the pieces must have been together about 14 Ga ago. For some time after the Big Bang, the universe consisted only of gaseous hydrogen and helium – there were no stars or galaxies. All other elements were created during the life and death of stars. Norma ...
... the rate of retreat, we can calculate that all the pieces must have been together about 14 Ga ago. For some time after the Big Bang, the universe consisted only of gaseous hydrogen and helium – there were no stars or galaxies. All other elements were created during the life and death of stars. Norma ...
The Solar System (Ch. 6 in text) The solar system consists of the Sun
... Best for close-in (so short period, high velocity) massive planets. B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far fr ...
... Best for close-in (so short period, high velocity) massive planets. B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far fr ...
AST301.Ch6.15.SolarSystems - University of Texas Astronomy
... Best for close-in (so short period, high velocity) massive planets. B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far fr ...
... Best for close-in (so short period, high velocity) massive planets. B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far fr ...
Planets of the Solar System Information
... the largest of all the planets, with a diameter of 142 800 km. It takes 11.9 Earth years to complete one revolution around the sun. Jupiter has the fastest spin of all the planets. It rotates once every 10 hours and its swirling core is almost as hot as the sun. This is why Jupiter has the strongest ...
... the largest of all the planets, with a diameter of 142 800 km. It takes 11.9 Earth years to complete one revolution around the sun. Jupiter has the fastest spin of all the planets. It rotates once every 10 hours and its swirling core is almost as hot as the sun. This is why Jupiter has the strongest ...
Transcript - Cheap Astronomy
... 1600 after voicing the view that not only did the Earth orbit the Sun, but it was likely that other planets orbited other stars and could well harbour other life. A few years after that, Galileo began reporting some hard core observations collected through his telescope – showing that Jupiter had mo ...
... 1600 after voicing the view that not only did the Earth orbit the Sun, but it was likely that other planets orbited other stars and could well harbour other life. A few years after that, Galileo began reporting some hard core observations collected through his telescope – showing that Jupiter had mo ...
Compare the following sets of stars using the words: BRIGHTER or
... Sun-like Star -> red giant -> planetary nebula -> white dwarf ...
... Sun-like Star -> red giant -> planetary nebula -> white dwarf ...
astronomy - Mr. Barnard
... (2) neutron star (4) white dwarf ____5. The explosion of a massive star near the end of its life is known as a (1) nebula (3) nova (2) supernova (4) pulsar ____6. According to our present theories of stellar evolution, our sun will change next into (1) a white dwarf (3) a red giant (2) a black hole ...
... (2) neutron star (4) white dwarf ____5. The explosion of a massive star near the end of its life is known as a (1) nebula (3) nova (2) supernova (4) pulsar ____6. According to our present theories of stellar evolution, our sun will change next into (1) a white dwarf (3) a red giant (2) a black hole ...
Quadratic Functions
... known bodies, scientists can speculate on the composition of these unknown bodies because of the similarities to known bodies explored by rovers. Planetary Motion Mathematically, the planets can be modeled by Kepler’s Laws of Planetary Motion. There are 3 distinct laws that Kepler discovered. The fi ...
... known bodies, scientists can speculate on the composition of these unknown bodies because of the similarities to known bodies explored by rovers. Planetary Motion Mathematically, the planets can be modeled by Kepler’s Laws of Planetary Motion. There are 3 distinct laws that Kepler discovered. The fi ...
Formation and evolution of the Solar System
The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.