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No Slide Title
No Slide Title

... achieved by cooling or by a dynamical interaction. • Simulations show a large number of planets form from a single disc. • Only produces gaseous planets – rocky (terrestrial) planets are not formed. • Is not applicable to the solar system. • Could explain the directly imaged HR8799 system Dr. Matt B ...
Earth in space - Deakin University Blogs
Earth in space - Deakin University Blogs

... (Moon 3500 km and Earth 12 800 km) the ratio is approximately 4:1 (or, more accurately, 3.7:1). Using the models of Earth and the Moon (50:1 ratio), place them at a distance to represent the actual distance between Earth and the Moon. The actual distance is about thirty times Earth’s diameter. Place ...
Motion of the Earth and Moon – Part 2
Motion of the Earth and Moon – Part 2

... T: “Good, you rotate, I want you to stay in the same spot and spin in a circle. Do it slow so you don’t get dizzy.” S: student #1 will start spinning in circles. T: “Now you are the moon (referring to student #2), what will you do?” S: will respond, “walk around the earth and rotate on my axis” T: “ ...
Modeling Planet Distances
Modeling Planet Distances

... those distances in order to visualize the relative distances of the planets from one another and from the Sun. Explain that by constructing a scale model that will fit inside the classroom, they can get a better idea of the relative distances between planets in the Solar System. Ask, Do you think yo ...
Outline of Lecture on Copernican Revolution: 1. Source of word
Outline of Lecture on Copernican Revolution: 1. Source of word

... emerges as a completely unmotivated result. In fact, in Ptolemy’s model the periods in which also Jupiter and Saturn go around their individual epicycles are also, astonishingly, precisely one year. One would imagine that this accidental result would have caught someone’s attention. Ptolemy offers a ...
The Solar System - Geologisk Museum
The Solar System - Geologisk Museum

... of gravel, pebbles and ice, which was strong as concrete. We could not do much, but the visible dimensions indicated that the meteorite must weigh at least 15 t. Home again financial support for the future work should be found and plans made for the excavation and recovery of the meteorite. The Geol ...
Search for Other Worlds - Science fiction 20 years
Search for Other Worlds - Science fiction 20 years

... to view the corona of the Sun, but a new version of similar instruments are being used to find extrasolar planets around nearby stars. Coronagraphs can be attached to either ground based or space based telescopes. While stellar and solar coronagraphs are similar in concept, they are quite different ...
Mystery Detectives
Mystery Detectives

... *B. a metamorphic rock* ...
Outer Solar System Exploration
Outer Solar System Exploration

... observations that yielded contextual information on Io’s volcanoes and Jupiter’s clouds, for example. Future Juno-related science in particular can benefit from use of ground-based assets to find hotspots and to predict the location of major atmospheric features to facilitate targeting of Juno’s Jun ...
Planets in Our Solar System
Planets in Our Solar System

... audience to purchase real estate on a specific planet assigned to them. Groups will research their planet, create a presentation using google slides, and design a model of a home that can (in theory) sustain life on their planet. Standards Alignment This unit is aligned to Common Core State Standard ...
The Jupiter System
The Jupiter System

Planets, Moons, and Stars
Planets, Moons, and Stars

... Celsius). This is hot enough to melt Earth! The Sun is about 150 million kilometers (93 million miles) away from Earth. If you could travel there by car on a highway, it would take more than 160 years. Even though the Sun is that far away, it provides Earth with light and heat. Life on Earth could n ...
PTYS/ASTR 206
PTYS/ASTR 206

... the recently discovered Eris is larger than Pluto. • In 2006, Pluto was downgraded to a new class of objects called “dwarf planets” – But the debate rages on ...
Smallest Kuiper Belt Object Ever Detected
Smallest Kuiper Belt Object Ever Detected

... 1,000 km. Researchers have long suspected that these bodies exist, but previously lacked proof for objects of this size. They are believed to be the result of collisions among the members of the original Kuiper belt population. The detection of only one event actually reveals a deficit of sub-kilome ...
PLANETS
PLANETS

... • In the Solar System, NOT same composition as Sun • Presence of gas implies formation while gas was still prevalent Cores: Gas giants may have a rocky or metallic core—in fact, such a core is thought to be required for a gas giant to form. H and He: The majority of its mass is in the form of the ga ...
21trans-neptunian2s
21trans-neptunian2s

... Pluto and Charon are in a close, tidally locked orbit ...
90733 Internal v2 3.7 D1 Kuiper Belt Objects 2006
90733 Internal v2 3.7 D1 Kuiper Belt Objects 2006

... The Kuiper belt remained theory until in 1992 the first of the Kuiper Belt objects (KBOs) was discovered. This was a 200km wide body, called 1992QB1, found beyond Pluto. Several similar-sized objects were discovered quickly confirming that the Kuiper belt was real. The planet Pluto, discovered in 19 ...
EEn.1.1 Explain the Earth`s role as a body in space. EEn
EEn.1.1 Explain the Earth`s role as a body in space. EEn

Unit 3 Rocks Ch. 5 Lecture
Unit 3 Rocks Ch. 5 Lecture

... 2. the present physical features of Earth were formed by these same processes, at work over long periods of time. ...
Space BootCamp5.8D_Part1_AC
Space BootCamp5.8D_Part1_AC

... meteorites are pulled to its surface than to the Earth’s surface. There is more water on the Earth’s surface than on the moon’s surface. This water causes meteorites to explode. The moon has little or no atmosphere. Meteorites heading to Earth burn up in its atmosphere before hitting the ground. Met ...
Copernicus
Copernicus

... motion known as epicycles. • An epicycle is an orbit within an orbit • Having set up this model, Ptolemy then went on to describe the mathematics which he needed in the rest of the work. ...
Lab 3: The Galilean Revolution
Lab 3: The Galilean Revolution

... For that image, select the information window and record the system (not universal) date and time that the image was taken in Data Table 1 below. Also record the Julian date that the image was taken in Data Table 1, to the nearest 0.1 days. Adjust the max value and zoom in/out until you can easily s ...
View Diary of Astronomical Events - Astronomical Society of Singapore
View Diary of Astronomical Events - Astronomical Society of Singapore

Maria Makris Drorit Weiss SNC1D: Grade 9 Science, Academic
Maria Makris Drorit Weiss SNC1D: Grade 9 Science, Academic

... The purpose of this unit is to provide students with D1. Assess some of the costs, hazards, and benefits of space exploration and the contributions of Canadians to space research and an overview of the study of the universe as an introduction to astronomy. By the end of this unit, technology; studen ...
New Worlds Ahead: The Discovery of Exoplanets
New Worlds Ahead: The Discovery of Exoplanets

... by Kant and Laplace more that two hundred years ago, but, although correct, it has been for decades the subject of many debates. In this theory, the Solar system was formed by the collapse of an approximately spheric giant interstellar cloud of gas and dust, which eventually flattened in the plane p ...
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Late Heavy Bombardment



The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.
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