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Skymobile: Comet Demonstration
Skymobile: Comet Demonstration

... Raise your hands if you know something that is solid. (Take some answers). That’s right! Your desk is solid. Your chair is solid. Your pencil is solid. Your books are solid. Anything that you can hold, sit on or stand on is solid. Now I’m going to show you something else that is solid. (Take out an ...
Celestial Equator
Celestial Equator

... higher percentage of oceans, which reflect heat and light back into space more efficiently than do forested land masses. If the Earth’s orbit were very elliptical (like Mercury), then this effect would be more pronounced, and if, in addition, the Earth’s axis were not tilted, then the seasons would ...
From the Everett and Seattle Astronomical
From the Everett and Seattle Astronomical

... Mercury is the closest planet to our Sun, and the least explored of the socalled terrestrial planets, which are the four rocky inner planets that also include Venus, Earth, and Mars. Other than 3 flybys by Mariner 10 in 1974 and ’75, no other spacecraft have yet explored the first rock from the Sun. ...
Final Review Packet
Final Review Packet

... 81. Relative humidity is the ____________________ of air’s actual water-vapor content compared with the amount of ____________________ air can hold at that temperature and pressure. 82. If the water-vapor content of air remains the same, raising air temperature causes a(n) ____________________ in re ...
Chapter 7
Chapter 7

... •The metallic hydrogen is a superconductor. A superconductor conduct electricity with minimum or no resistance •Increasing temperature and pressure deeper in core •Jupiter shape is distorted, about 7% larger at equator. Caused by fast rotation (~10 hours) and large radius •Saturn less asymmetric – l ...
Geologic Time
Geologic Time

... When something is filled with atoms of rock material; this makes them very hard (rock). *Commonly found with wood. ...
Our View of the SS - MMSD Planetarium
Our View of the SS - MMSD Planetarium

... would be found in the Solar System beyond a simple, straight-line model. They wrongly assume that Venus and Mars are always the closest planets to the Earth. Their misconceptions become obvious by their questions when they see something like Jupiter and Venus close together in the sky: “How can Venu ...
4 Inner versus Outer Planets
4 Inner versus Outer Planets

... As gravity pulled matter into the center of the disk, the density and pressure at the center became intense. When the pressure in the center of the disk was high enough, nuclear fusion began. A star was born—the Sun. The burning star stopped the disk from collapsing further. Meanwhile, the outer par ...
58KB - NZQA
58KB - NZQA

... travelling faster than Earth. This collision caused both planets to melt and the outer layers of both planets to be ejected into space. A disk of orbiting material was formed and this matter eventually stuck together and formed the moon that now orbits around Earth. The ejected rock (the moon) staye ...
How strong is gravity on other planets?
How strong is gravity on other planets?

... gravitation, the gravitational attraction between two bodies can be expressed mathematically as F = G (m1m2/r2) – where F is the force, m1 and m2 are the masses of the objects interacting, r is the distance between the centers of the masses and G is the gravitational constant (6.674×10-11 N m2/kg2 ) ...
Geologic Time
Geologic Time

... When something is filled with atoms of rock material; this makes them very hard (rock). *Commonly found with wood. ...
138KB - NZQA
138KB - NZQA

... travelling faster than Earth. This collision caused both planets to melt and the outer layers of both planets to be ejected into space. A disk of orbiting material was formed and this matter eventually stuck together and formed the moon that now orbits around Earth. The ejected rock (the moon) staye ...
Compact Objects in the Solar System
Compact Objects in the Solar System

... object interaction, lower mass objects will often be ejected. •! At first, people won’t notice too much, even though the orbit starts to change somewhat. ...
Growing the Terrestrial Planets from the Gradual
Growing the Terrestrial Planets from the Gradual

... physical conditions (which might not have been satisfied everywhere in the disk), these concentrations become dense enough that they become gravitationally unstable and thus collapse to form planetesimals [11] with radii between ∼ 50 and ∼ 1000 km [10, 12]. This process can occur very quickly — on t ...
13 - Joe Griffin Media Ministries
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... direct, or prograde, motion. They wander across the sky westward, but since the orbit of Earth is much faster than those of the superior or outer planets, this causes periodic retrogradation. For example, Earth advances on Jupiter, draws even with it, and then passes it. This causes an optical illus ...
Exoplanet Discovery
Exoplanet Discovery

Formation of the Solar System
Formation of the Solar System

... iv. The hierarchy pattern of orbiting systems in the solar system was established early in its history as the disk of dust and gas was driven by gravitational forces to form moon-planet and planet-sun orbiting systems. c. Students use the model to describe that objects too far away from the sun do n ...
Part 2 of Test- Planet Flip Book
Part 2 of Test- Planet Flip Book

... d. The location in the solar system of your planet e. How long would its days and nights be? f. Describe the landscape/atmosphere g. Include any other fun information! ...
What it takes to make a planet
What it takes to make a planet

... next group should be called “dwarf planets” and even came up with the name “Plutons” for them, to retain something of the special character of Pluto – which turned out to be very unpopular. At the top end, we wanted to leave it vague. So our proposal had three categories: classical planets, dwarf pl ...
The cosmological distance ladder
The cosmological distance ladder

... We determined the size of the Earth. Our value was 1.4% smaller than the true value. We determined the distance to the Moon. Our value was 3.3% larger that the known mean distance. We determine the Earth-Sun distance. Our value was 6% larger than the true value. Rarely in science do we know the tru ...
Motion of Objects in Space
Motion of Objects in Space

... Bell Ringer- Write definition and term 1. Any large body (bigger than asteroid) that revolves around a star 2. Giant ball of burning gas held together by gravity 3. Rocky object that orbits sun and is smaller than asteroid 4. Small chunk of ice, dust, and rocky material 5. A piece of space rock that ...
Red Rovers - Sky Calls
Red Rovers - Sky Calls

... We know there is no standing water, such as lakes or ponds, Uranus and Neptune, too far on Mars. The air pressure is so low that any water would quickly to see or call, evaporate. Scientists believe that if water once existed on Mars, And tiny, dark Pluto, the last planet of all. there might still b ...
Space - School District #42
Space - School District #42

... to
your
desktop
and
import
them
into
kidpix
and
write
 facts
about
at
least
one
of
them
–
kpx
–
(
people
doing
 venus
or
mercury
need
to
choose
to
tell
us
something
else
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their
planet)I
also
have
them
drag
the
graphics
 from
the
website
to
the
desktop
and
then
once
they
are
in
 kidpix
I
have
t ...
Unit 1 Cycle 2: Interactions and Energy
Unit 1 Cycle 2: Interactions and Energy

... sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, (c) has not cleared the neighbourhood around its orbit, and (d) is not a satellite. (3) All other objects except satellites orbiting the Sun shall be referred to coll ...
exam1guide - Chemistry at Winthrop University
exam1guide - Chemistry at Winthrop University

... in old stars, star death for small and large stars, supernova and production of heavy elements, kilonovas, stars as agents of change in the universe. The Solar System: Earth’s Sun (Sol), hydrogen fusion, yellow star (surface temperature=6,000o C), Sol’s electromagnetic radiation, structure of Sol, r ...
< 1 ... 135 136 137 138 139 140 141 142 143 ... 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.
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