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File - Homeschooling Mommie
File - Homeschooling Mommie

... the largest planet in our solar system and the fifth planet from the Sun. It is so large that all of the other planets in the solar system could fit inside of it. Jupiter has the most natural satellites or moons of any planet. The count is currently at 63, although not all of them have been named. I ...
Name: Period : ______ The Universe – Life and Death of a Star How
Name: Period : ______ The Universe – Life and Death of a Star How

earth structure notes
earth structure notes

κβαντικη / ολιστικη αστρολογια
κβαντικη / ολιστικη αστρολογια

CO 2 Cycle
CO 2 Cycle

... carried sediment in the past several years…The atmosphere on Mars is so thin that liquid water cannot persist at the surface. However, researchers propose that water could remain liquid long enough, after breaking out from an underground source, to carry debris before totally evaporating and freezin ...
Barred Spiral Galaxy
Barred Spiral Galaxy

... •A white dwarf is a very small and cool, formed when middle size stars die ...
The H-R Diagram
The H-R Diagram

... larger, and more massive than the Sun. The Sun is near with an absolute magnitude of MV=+5 and a spectral type G2. Like all m.s. stars it is of luminosity class V. Those stars to the lower right are less massive, cooler, and smaller than the Sun. The main sequence contains about 80% of all stars. St ...
A NEW FAMILY OF PLANETS? “OCEAN
A NEW FAMILY OF PLANETS? “OCEAN

... Their composition is, in mass, 50% rocks and metals, 50% ices, as can be expected from the disc chemical composition; 2. the initial composition of ices is similar to that of comets, mostly H2O and some NH3 and CO2 . To simplify the photochemistry, we assume no CO nor CH4 . The latter condition shou ...
instructor notes: week 2
instructor notes: week 2

... another object. Synodic Period. The time taken for an object to cycle through its phases as viewed from Earth. Inferior planet. A planet orbiting inside Earth’s orbit. Superior planet. A planet orbiting outside Earth’s orbit. Prograde motion. When a planet’s RA increases nightly. Retrograde motion. ...
A105 –Stars and Galaxies
A105 –Stars and Galaxies

... Estimate the period of the orbit (the time for one complete orbit, or the time between maximums (or minimums) in the velocity curve). What is the length of the “year” of 51 Peg’s planet? Next, estimate the mass of 51 Peg’s planet. The following graph relates the mass of the planet to the range of ve ...
Astronomy 103 Exam 2 Review
Astronomy 103 Exam 2 Review

... Two
observers
have
two
clocks,
one
at
rest
on
the
Earth’s
 surface
and
one
at
rest
high
above
the
Earth’s
surface.

 Which
statement
is
correct?
 A. 
Each
observer
will
see
the
other's
clock
to
be
running
 slow
with
respect
to
the
observer's
own
clock.
 B. 
Each
observer
will
see
the
other's
clock
 ...
what is a comet? - Fireballs in the sky
what is a comet? - Fireballs in the sky

... Halley’s Comet is perhaps the most wellknown comet in the world. It returns to the inner solar system once every 76 years and has been recorded many times throughout history. The last time it visited the inner solar system was in 1986, and it won’t be visible again until 2061. Spacecraft that visite ...
ASTRONOMY 110G Review Questions for
ASTRONOMY 110G Review Questions for

winter
winter

... Portsmouth, NH ...
Comparative Planetology of the Outer Planets A Travel Guide to the
Comparative Planetology of the Outer Planets A Travel Guide to the

... formed together with Saturn because material would have been blown away by particle stream from hot Saturn at time of formation. ...
AD-5.1 Space - CAP Members
AD-5.1 Space - CAP Members

... the sun in 88 days and its temperature ranges from 800°F to - 300°F. It is a rocky, crusty surface with craters. There is no atmosphere, except for small amounts of helium and hydrogen. b. Venus – It is the closest planet to Earth, 67 million miles from the sun. It revolves around the sun in 225 day ...
Astronomy 2 Relativity and Gravitation
Astronomy 2 Relativity and Gravitation

Dec 2017 - What`s Out Tonight?
Dec 2017 - What`s Out Tonight?

... tens of thousands stars held together by their mutual gravity. All Galilean moons and cloud bands, easily visible at 50x. It is posof the globulars that can be seen in the sky are part of our Milky sible to see the moons with well-focused binoculars. Saturn is Way Galaxy, and there are about 200 of ...
FORMATION AND ORBIT OF HOT JUPITERS 1 Formation and Orbit
FORMATION AND ORBIT OF HOT JUPITERS 1 Formation and Orbit

Life and Earth Science Vocabulary 2015
Life and Earth Science Vocabulary 2015

... Planet Order (3.8D); Characteristics of Sun, Earth, and Moon, and Patterns in Moon Phases and Tides (5.8C and 4.8C) Sun: average sized star made of hot gases found at the center of our solar system Earth: the only planet with life; Earth has an atmosphere, weather, and liquid water Moon: Earth’s na ...
Introduction to Astronomy
Introduction to Astronomy

... 5. Will the Sun ever be straight overhead here in Massachusetts? Nope. The sun is only directly overhead if you live at the equator. Since Massachusetts is so far from the equator it will never be overhead. 6. What does the term “Land of the Midnight Sun” mean? What causes it? Land of the midnight s ...
EARTHSKY Why Earth has 4 seasons Some assume our planet`s
EARTHSKY Why Earth has 4 seasons Some assume our planet`s

... Earth’s distance from the sun does change throughout the year, and it’s logical to assume that an increase or decrease in a sun-planet distance could cause a cyclical change in the seasons. But – in the case of our planet – this change is too small to cause this change. Our seasons change due to our ...
Phys 214. Planets and Life
Phys 214. Planets and Life

... Jovian moons are typically made of ice and rock. The outer Solar System was cold enough to allow ices to condense along with metal and rock. The average densities of most jovian moons are significantly lower than that of Earth – they contain a lot of water ice. Within individual moons we see variati ...
Fingerprints in Starlight: Spectroscopy of Stars Inquiry Questions
Fingerprints in Starlight: Spectroscopy of Stars Inquiry Questions

Star Series PP 1 - Country Bible Church
Star Series PP 1 - Country Bible Church

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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.
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