• 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
Astronomy 10: Introduction to General Astronomy Instructor: Tony
Astronomy 10: Introduction to General Astronomy Instructor: Tony

... The Roche limit tells us how far a moon can be from a planet before it is completely torn apart by the planet’s tidal forces. Saturn’s rings are within this Roche limit. This makes sense, because moons could not survive at such a close distance. Also, it may indicate that the rings were formed by a ...
The Milky Way
The Milky Way

... too large) – better than any previous radius estimate ...
Planetarium Field Guide 2015-2016 Third Grade
Planetarium Field Guide 2015-2016 Third Grade

... The program takes students on a tour to explore the many objects that populate our solar system. The students will be able to examine each individual planet and move outside to see where the Earth fits in the larger picture. The Solar System a. What are the two things the Sun provides our planet tha ...
Scale Model of the Solar System
Scale Model of the Solar System

...  Yellow or orange card to make a 2D model of the sun (A spherical model will be quite big!)  A map of your locality. (The solar system is a very big place and you will not get all the models placed properly in the school grounds!) Now that you have set out the model Solar System, you might like to ...
50 FACTS about SPACE
50 FACTS about SPACE

... 3. What is the study of the universe called? __________________________. 4. A person who studies astronomy is called an ______________________________. 5. The sun along with the planets is known as the ___________________ ____________________. 6. A hot ball of plasma is known as a __________________ ...
ppt - The Eclecticon of Dr French
ppt - The Eclecticon of Dr French

... The ancient Hindu Rig Veda text postulates the Universe has a lifetime of 8 million years. There are an infinite number of Universes in ‘existence’. Existence itself renews after a cycle of 311 trillion years! The Ancient Egyptians believed the flat Earth god Geb was overarched by the air god Shu an ...
Homework 2 (Due Sept 18, 2014)
Homework 2 (Due Sept 18, 2014)

... this chamber, a feather would fall at the same rate as a rock.! c. When an astronaut goes on a space walk outside the Space Station, she will quickly ! float away from the station unless she has a tether holding her to the station.! d. If the Sun were magically replaced with a giant rock that had pr ...
The Milky Way
The Milky Way

... stadia (probably ~ 14 % too large) – better than any previous radius estimate ...
Observation & Inference - East Hanover Schools Online
Observation & Inference - East Hanover Schools Online

... between the orbits of Mars and Jupiter. Asteroids are also known as planetoids. ...
TEST1-WHITE Modern scientific theories are NOT: Testable
TEST1-WHITE Modern scientific theories are NOT: Testable

... a. It had the authority of Aristotle behind it b. It was consistent with Church doctrines c. It used perfect circles, which appealed to many d. It accounted well for Galileo’s observations of the phases of Venus e. It explained why stellar parallaxes were not observed by the Greeks 10. Which was a c ...
Lecture6
Lecture6

... wandering object (sun, moon, + 5 planets), in addition to the “fixed stars”. Problem: couldn’t explain retrograde motion. Solution (Ptolemy): small circles upon large (offset) circles. ...
Planets around Other Stars
Planets around Other Stars

... Reproduced below is a plot of observations of the radial velocity of the star 51 Pegasi, the first star discovered to have a planet. The observed velocity (in meters per second) is plotted vs. the time (in days) when the observation was made. The velocity of the star varies with time because the sta ...
Sun, Moon, and Earth Review Sheet
Sun, Moon, and Earth Review Sheet

... Revolution/revolves- the movement of an object around another object. The sun, Earth, and other planets are part of the solar system. Our solar system is part of the Milky Way Galaxy. ...
ITS3
ITS3

... Our Sun is an average size star Sirius B is a dwarf star, whilst Antaris is a red giant, about 300 times larger than the Sun. if it were possible to drive a car around the equator of the Sun at 88 kph it would take 5.5 years to complete the journey non-stop! The Sun is shrinking at a rate of 1 metre ...
Astronomical history
Astronomical history

... the people about how in religion “god” had made the earth perfect everything revolving around them. (b) Where did Ptolemy place the stars in his model? In this model Ptolemy places the stars outside of the revolving planets. The sun is an example being the first star in our solar system and being th ...
The Nine Planets
The Nine Planets

... • Another giant & cold planet made mostly of hydrogen & helium • Rotates backwards -its axis is tilted 98˚ • 1 day is about 18 Earth hours, but 1 year is about 84 Earth years • Has at least 27 moons, all small • Through a telescope - looks like a small blue-green disk • Named from the Greek word whi ...
Astronomy 100 Homework #2 Solutions 1, Problem 3‐27 (2 pts
Astronomy 100 Homework #2 Solutions 1, Problem 3‐27 (2 pts

... 1,
Problem
3‐27
(2
pts).
According
to
Kepler’s
third
law,
(b)
Jupiter
orbits
the
Sun
 more
quickly
than
Saturn.

Because
the
semimajor
axis
is
smaller,
the
orbital
period
 P
=
a3/2
will
be
smaller.
 2.
Problem
3‐40
(2
pts).
The
recently
discovered
object
Sedna
orbits
our
sun
 beyond
Pluto,
at
an
ave ...
Astronomy - cloudfront.net
Astronomy - cloudfront.net

... The Sun's heat drove the remaining dust and gas out of the part of the solar system with planets, and gravitational interactions ejected most of the larger debris. ...
Bad Astronomy
Bad Astronomy

... Tides are the vertical rising and lowering of sea level, and are greatly controlled by the gravitational pull of the sun and moon. Although the sun has a stronger gravitational attraction than the moon, the moon's relative nearness to the earth makes its gravitational pull more than twice as effecti ...
Dwarf Planets
Dwarf Planets

... the sun. This forms a thin atmosphere. ...
where it is, how big it
where it is, how big it

... completely unexpected and only discovered when two of the Voyager 1 scientists insisted that they should at least check to see if any rings might be present. Unlike Saturn's, Jupiter's rings are dark. ...
solution
solution

... 3.24 How did Aristarchus try to estimate the diameters of the Sun and Moon? He used geometry and proportions to estimate the relative distances between the Sun, Earth and Moon. Once he had these, he used the eclipses to state that the Sun and Moon had the same angular size, so their relative sizes c ...
Chapter 19 I. The Sun, Earth and Moon A. Sun is our closest star B
Chapter 19 I. The Sun, Earth and Moon A. Sun is our closest star B

... b. tides are caused by the moon’s gravitational pull on the Water on the Earth b. everything in solar system orbits around Sun F. The Moon 1. Moon doesn’t orbit the Sun directly a. orbits the Earth i. due to this the moon has phases 2. How was the moon formed? a. Earth collided by large body & part ...
Today`s Powerpoint
Today`s Powerpoint

... - Occam’s Razor: Simpler Theories are better -You can prove a theory WRONG but not RIGHT Prediction ...
previous mid-term () - Department of Physics and Astronomy
previous mid-term () - Department of Physics and Astronomy

... 56. The planets formed into two main groups: the inner terrestrial planets and the outer Jovian planets. Which of the following is NOT characteristic of the formation sequence of the terrestrial planets? a. Heavy elements condense to form grains and then planetesimals. b. Planetesimals coalesce and ...
< 1 ... 104 105 106 107 108 109 110 111 112 ... 133 >

Satellite system (astronomy)



A satellite system is a set of gravitationally bound objects in orbit around a planetary mass object or minor planet. Generally speaking, it is a set of natural satellites (moons), although such systems may also consist of bodies such as circumplanetary disks, ring systems, moonlets, minor-planet moons and artificial satellites any of which may themselves have satellite systems of their own. Some satellite systems have complex interactions with both their parent and other moons, including magnetic, tidal, atmospheric and orbital interactions such as orbital resonances and libration. Individually major satellite objects are designated in Roman numerals. Satellite systems are referred to either by the possessive adjectives of their primary (e.g. ""Jovian system""), or less commonly by the name of their primary (e.g. ""Jupiter system""). Where only one satellite is known, or it is a binary orbiting a common centre of gravity, it may be referred to using the hyphenated names of the primary and major satellite (e.g. the ""Earth-Moon system"").Many Solar System objects are known to possess satellite systems, though their origin is still unclear. Notable examples include the largest satellite system, the Jovian system, with 67 known moons (including the large Galilean moons) and the Saturnian System with 62 known moons (and the most visible ring system in the Solar System). Both satellite systems are large and diverse. In fact all of the giant planets of the Solar System possess large satellite systems as well as planetary rings, and it is inferred that this is a general pattern. Several objects farther from the Sun also have satellite systems consisting of multiple moons, including the complex Plutonian system where multiple objects orbit a common center of mass, as well as many asteroids and plutinos. Apart from the Earth-Moon system and Mars' system of two tiny natural satellites, the other terrestrial planets are generally not considered satellite systems, although some have been orbited by artificial satellites originating from Earth.Little is known of satellite systems beyond the Solar System, although it is inferred that natural satellites are common. J1407b is an example of an extrasolar satellite system. It is also theorised that Rogue planets ejected from their planetary system could retain a system of satellites.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report