• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
T2 Precambrian Geology Homework KEY
T2 Precambrian Geology Homework KEY

... 14) The largest belt of folded rocks indicating Proterozoic continental collisions is called the: a) Grenville Orogen. b) Trans-Hudson Orogen.. c) Mazatal Orogen. d) Wopmay Orogen 15) The last major Proterozoic collision before assembly of Rodinia is recorded by rocks in the: a) Grenville Orogen.. ...
*Do you know why the Outer Planets are called the “Gassy Giants
*Do you know why the Outer Planets are called the “Gassy Giants

... *In 2006, the International Astronomical Union (IAU) defined a planet as : a celestial body which: is in orbit around the Sun, has sufficient mass to assume hydrostatic equilibrium (a nearly round shape), and has "cleared the neighborhood" around its orbit. *Pluto does not have all of those classifi ...
The Basics of the Universe
The Basics of the Universe

... to its dusty terrain that has gone through oxidation. Mars is about half of the size of the Earth, and has a thin atmosphere. There is ice scattered around the planet. Two rovers, named Opportunity and Spirit, have roamed the landscape, searching for signs of life. So far, none has been found, even ...
Some space objects are visible to the human eye.
Some space objects are visible to the human eye.

... The movements of planets and other nearby objects are visible from Earth. A jet plane travels at a greater speed and altitude than a bird. Yet if a bird and a plane flew overhead at the same time, you might think that the bird was faster. You would have this impression because the farther away a mov ...
Dating the Universe
Dating the Universe

... interstellar dust particles in this part of our galaxy – This cloud collapsed under its own gravity and spun into a disk – Most of the mass fell into the center of the disk and formed the Sun – A tiny fraction of the leftovers formed the planets, moons, etc. ...
Lecture 3 - Night Sky and Motion of the Earth around the Sun
Lecture 3 - Night Sky and Motion of the Earth around the Sun

... Angular Measure for Small Angles 1º = 60 arcminutes = 60′ 1′ = 60 arcseconds = 60″ e.g., On January 1, 2004, the planet Saturn had an angular diameter of 19.7″ as viewed from Earth. ...
File
File

... 17. Over time, a significant amount of geological activity, such as plate tectonics, the rock cycle, and erosion, has occurred on the Earth and continues to occur today. There is evidence, however, that some geological activity once occurred on other planets or moons as well. The presence of solidif ...
second grade - Math/Science Nucleus
second grade - Math/Science Nucleus

... effect) making the surface of Venus the hottest in the Solar System, about 750oK. Venus rotates very slowly, taking 243 days to complete one turn. It is named for the Roman goddess of love. Earth is a little more than 12,000 kilometers in diameter. It differs from the other planets because it has l ...
Exploring the Solar System - The Federation of Galaxy Explorers
Exploring the Solar System - The Federation of Galaxy Explorers

... Meteor Crater near Winslow, Arizona. Asteroids are material left over from the formation of the solar system. One theory suggests that they are the remains of a planet that was destroyed in a massive collision long ago. More likely, asteroids are material that never coalesced into a planet. In fact, ...
Warm Up - Cloudfront.net
Warm Up - Cloudfront.net

... The main results of the earth’s rotation are night and day  There are two kinds of days!  Mean Solar day – time interval from one noon to the next (~ 24 hours)  Sidereal day – the time it takes for the Earth to make one complete rotation with respect to a star other than our sun (23 hours, 26 min ...
lecture 2
lecture 2

... between the Earth and the Sun • A lunar eclipse occurs when the Earth moves between the Sun and the Moon and the Moon moves through the Earth’s shadow • In ancient cultures eclipses were bad omens ...
Modeling Sizes of Planets
Modeling Sizes of Planets

... 1) What is the difference between the planets in the inner solar system (Mercury to Mars) and the planets beyond Mars? If you like, speculate about why there is a difference. [Answer suggestions: The inner planets (Mercury, Venus, Earth, and Mars) are all small compared to the outer planets (Jupiter ...
Table of contents Overview of the Solar System
Table of contents Overview of the Solar System

... physics, a body close to a bigger one accelerates faster around it. This is the same for Mercury; it has the fastest orbital period around the Sun. It takes 175,97 Earth days for one orbit. Since it is so close to the Sun, the temperature of its surface reaches 450 degrees Celsius during the days. D ...
Planet Saturn
Planet Saturn

... Revolution Period about the Sun Equatorial Radius Equatorial Circumference ...
The booklet - Cosmos
The booklet - Cosmos

... physics, a body close to a bigger one accelerates faster around it. This is the same for Mercury; it has the fastest orbital period around the Sun. It takes 175,97 Earth days for one orbit. Since it is so close to the Sun, the temperature of its surface reaches 450 degrees Celsius during the days. D ...
Planet Saturn
Planet Saturn

... Revolution Period about the Sun Equatorial Radius Equatorial Circumference ...
Formation and differentiation of the Earth
Formation and differentiation of the Earth

... Temperature gradients in the planetary nebula ...
THE PLANETS C - White-Thomson Publishing Services
THE PLANETS C - White-Thomson Publishing Services

... there were nine planets in our ...
Unit XII Study Guide
Unit XII Study Guide

... c. the inward pull of gravity and outward push of thermal pressure are balanced. d. Nuclear fusion is a stabilizing process. ____ 16. For the sun to be stable, the inward and outward forces within the sun must be a. In equilibrium. b. part of the fusion reaction. c. Focused in the core. d. balanced ...
a closer look at the planets
a closer look at the planets

... • Largest moon is TITAN. It is the only moon in the solar system to have an atmosphere composed of ...
The Outer Planets
The Outer Planets

... Uranus: The Sideways Planet Instead of being generally perpendicular to the plane of its orbit, Uranus’s axis of rotation lies nearly parallel with the plane of its orbit  Uranus has a set of at least nine distinct ...
`It`s Raining, It`s Pouring`
`It`s Raining, It`s Pouring`

... eminent philosophers including Hippocrates, Plato and Aristotle, seem to have had knowledge of the basic outline of the system. However, some of their basic understanding of the hydrologic or water cycle was incorrect, and, in 1500, scientist, artist, and great thinker Leonardo da Vinci used observa ...
What Is a Planet? Pluto and Its Place in the Solar System
What Is a Planet? Pluto and Its Place in the Solar System

... • Uranus discovered with telescope 1781 • Four asteroids discovered 1801-1807 – Ceres, Pallas, Juno, Vesta – They were called planets! ...
Astro 205 Ch. 2
Astro 205 Ch. 2

... •   “Occam’s  Razor”  is  a  principle  which  states  that   simplicity  is  an  important  part  of  scienBfic  theory.   ...
Notes
Notes

... features such as sinuous rilles which are probably exposed lava tubes. Tectonic activity indicated by fault features, but there is no evidence of plate tectonics either past or present. Moonquakes originate mainly from a depth of ~1000km, suggesting that beneath this level the temperature/pressure c ...
< 1 ... 197 198 199 200 201 202 203 204 205 ... 385 >

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.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report