Underline your strong TEKS and circle your weak TEKS
... 6.11B Gravity & the Solar System Which of the following increases the gravitational attraction between two objects? Check all that apply. Increase the distance between the objects Increase the mass of the objects Decrease the distance between the objects Decrease the mass of the objects Change the c ...
... 6.11B Gravity & the Solar System Which of the following increases the gravitational attraction between two objects? Check all that apply. Increase the distance between the objects Increase the mass of the objects Decrease the distance between the objects Decrease the mass of the objects Change the c ...
TENTH GRADE SCOPE AND SEQUENCE DRAFT
... Night and day are caused by the rotation of the earth on its axis. The earth revolves around the sun once a year. The tilt of the earth results in seasonal changes. The sun gives us energy in the form of light and heat. The position of the sun in the sky appears to change over the course o ...
... Night and day are caused by the rotation of the earth on its axis. The earth revolves around the sun once a year. The tilt of the earth results in seasonal changes. The sun gives us energy in the form of light and heat. The position of the sun in the sky appears to change over the course o ...
Unit Name or Identification
... the center of the earth. Gravity plays a major role in the formation of the planets, stars, and solar system and in determining their motions. 1.9 Describe lunar and solar eclipses, the observed moon phases, and tides. Relate them to the relative positions of the earth, moon, and sun. 1.10 Compare a ...
... the center of the earth. Gravity plays a major role in the formation of the planets, stars, and solar system and in determining their motions. 1.9 Describe lunar and solar eclipses, the observed moon phases, and tides. Relate them to the relative positions of the earth, moon, and sun. 1.10 Compare a ...
Astronomy - Dallas ISD
... The diameter of the Earth is about 8,000 miles, and the diameter of the Moon is about 2,000 miles. The distance from the Earth to the Moon is about 240,000 miles. If a volley ball (diameter of about 8 inches) and a tennis ball (diameter of about 2 inches) are used to make a scale model of the Earth- ...
... The diameter of the Earth is about 8,000 miles, and the diameter of the Moon is about 2,000 miles. The distance from the Earth to the Moon is about 240,000 miles. If a volley ball (diameter of about 8 inches) and a tennis ball (diameter of about 2 inches) are used to make a scale model of the Earth- ...
Astronomy 8 - Dallas ISD
... The diameter of the Earth is about 8,000 miles, and the diameter of the Moon is about 2,000 miles. The distance from the Earth to the Moon is about 240,000 miles. If a volley ball (diameter of about 8 inches) and a tennis ball (diameter of about 2 inches) are used to make a scale model of the Earth- ...
... The diameter of the Earth is about 8,000 miles, and the diameter of the Moon is about 2,000 miles. The distance from the Earth to the Moon is about 240,000 miles. If a volley ball (diameter of about 8 inches) and a tennis ball (diameter of about 2 inches) are used to make a scale model of the Earth- ...
Document
... Radial Velocity Measurements of CoRoT-7b with HARPS. CoRoT-7b is a transiting planet discovered by CoRoT. The additional planets were found from the radial velocity follow up. ...
... Radial Velocity Measurements of CoRoT-7b with HARPS. CoRoT-7b is a transiting planet discovered by CoRoT. The additional planets were found from the radial velocity follow up. ...
cards for each vacation stop - Morehead Planetarium and Science
... CERES (representing the asteroid belt) — talk about a weight-loss diet 0.01 inches or 0.1 mm on our scale; too small to be included in the kit 1. Ceres is the largest object in the asteroid belt between Mars and Jupiter. Asteroids are “space rubble,” rocky remnants left over from the formation of o ...
... CERES (representing the asteroid belt) — talk about a weight-loss diet 0.01 inches or 0.1 mm on our scale; too small to be included in the kit 1. Ceres is the largest object in the asteroid belt between Mars and Jupiter. Asteroids are “space rubble,” rocky remnants left over from the formation of o ...
Earth Science Quarter 1 Credit Recovery
... How did planets form from smaller masses such as planetesimals and protoplanets? A protoplanet is created when many asteroids collide together and create a sphere with a molten core. Planetesimals are the many small pieces of asteroid that combine to make the protoplanet. ...
... How did planets form from smaller masses such as planetesimals and protoplanets? A protoplanet is created when many asteroids collide together and create a sphere with a molten core. Planetesimals are the many small pieces of asteroid that combine to make the protoplanet. ...
Better Than Earth
... these planetary systems long before our sun was born, flourishing and evolving for billions of years before even the first biomolecule emerged from the primordial soup on the young Earth. I am particularly fascinated by the possibility that a biosphere on these ancient worlds might be able to modify ...
... these planetary systems long before our sun was born, flourishing and evolving for billions of years before even the first biomolecule emerged from the primordial soup on the young Earth. I am particularly fascinated by the possibility that a biosphere on these ancient worlds might be able to modify ...
Great Galaxies 5 - School Performance Tours
... These are huge numbers and each of the numbers in this list is larger than the one before it. Some of these mathematical terms you may not have heard before but these are the numbers that are needed when calculating the distances from earth to other objects in the universe. For instance there are hu ...
... These are huge numbers and each of the numbers in this list is larger than the one before it. Some of these mathematical terms you may not have heard before but these are the numbers that are needed when calculating the distances from earth to other objects in the universe. For instance there are hu ...
Feb 2017 - Astronomical Society of Northern New England
... 1609 and he discovered many things like rings of Saturn, phases of Venus, sunspots on the sun, moons of Jupiter, and many others. Feb. 17. Venus is illuminated to its greatest extent for the year tonight. Feb. 18. Last quarter moon is at 2:33 pm. Pluto was discovered in this day in 1930. Feb. 19. Ni ...
... 1609 and he discovered many things like rings of Saturn, phases of Venus, sunspots on the sun, moons of Jupiter, and many others. Feb. 17. Venus is illuminated to its greatest extent for the year tonight. Feb. 18. Last quarter moon is at 2:33 pm. Pluto was discovered in this day in 1930. Feb. 19. Ni ...
The Night Sky This Month - Usk Astronomical Society
... Jupiter is best observed early in the month, whilst there is much to see in a decent telescope. It can be found in the same position in the constellation of Leo throughout the night during this month. A waxing gibbous Moon accompanies Jupiter during the night of the 15/16th. The Galilean Moons with ...
... Jupiter is best observed early in the month, whilst there is much to see in a decent telescope. It can be found in the same position in the constellation of Leo throughout the night during this month. A waxing gibbous Moon accompanies Jupiter during the night of the 15/16th. The Galilean Moons with ...
EXOPLANETS The search for planets beyond our solar system
... The first exoplanets were discovered through the gravitational tug they exert on their parent stars, which causes the stars to wobble. This motion is revealed in the spectrum of a star’s emitted light. Elements present in the star absorb particular wavelengths of light to produce a characteristic se ...
... The first exoplanets were discovered through the gravitational tug they exert on their parent stars, which causes the stars to wobble. This motion is revealed in the spectrum of a star’s emitted light. Elements present in the star absorb particular wavelengths of light to produce a characteristic se ...
NIE10x301Sponsor Thank You (Page 1)
... Today it takes 29.5 days for the Moon to complete a cycle of phases around the Earth, and appears in the same position in the sky relative to the background stars upon completion of its orbit around the Earth. This period is known as the synodic month or lunar month. The difference between the sider ...
... Today it takes 29.5 days for the Moon to complete a cycle of phases around the Earth, and appears in the same position in the sky relative to the background stars upon completion of its orbit around the Earth. This period is known as the synodic month or lunar month. The difference between the sider ...
ORBITAL MOTION
... dust & rocks), outflow has stopped, the star is visible. Theory: Gas disperses, “planetesimals” form (100 km diameter rocks), collide & stick together due to gravity forming protoplanets). Protoplanets interact with dust disks: tidal torques cause planets to migrate inward toward their host stars. E ...
... dust & rocks), outflow has stopped, the star is visible. Theory: Gas disperses, “planetesimals” form (100 km diameter rocks), collide & stick together due to gravity forming protoplanets). Protoplanets interact with dust disks: tidal torques cause planets to migrate inward toward their host stars. E ...
Publication - Centre for Star and Planet Formation
... respectively. The binary star consists of a Sun-like star and a companion roughly one-third its size, orbiting each other every 7.45 days. With an orbital period of 49.5 days, 18 transits of the inner planet have been observed, allowing a detailed characterization of its orbit and those of the stars ...
... respectively. The binary star consists of a Sun-like star and a companion roughly one-third its size, orbiting each other every 7.45 days. With an orbital period of 49.5 days, 18 transits of the inner planet have been observed, allowing a detailed characterization of its orbit and those of the stars ...
8L Earth and Space SoW
... Describe the Earth’s magnetic field and explain why a magnetic compass needle points north Describe the shape of the magnetic field between two bar magnets in different arrangements Recall the factors that affect the strength of gravity Stat the meaning of gravitational field strength Explain why th ...
... Describe the Earth’s magnetic field and explain why a magnetic compass needle points north Describe the shape of the magnetic field between two bar magnets in different arrangements Recall the factors that affect the strength of gravity Stat the meaning of gravitational field strength Explain why th ...
Third Grade Science
... • Describe our solar system as a collection of nine planets, moons, and numerous other objects (such as asteroids and comets) with the sun at its center • State that the force of gravity keeps the planets in orbit around the sun • Name the planets in our solar system in order starting with the pl ...
... • Describe our solar system as a collection of nine planets, moons, and numerous other objects (such as asteroids and comets) with the sun at its center • State that the force of gravity keeps the planets in orbit around the sun • Name the planets in our solar system in order starting with the pl ...
MS Word version
... Question 13: If the sweep segments were measured from the empty focus and not from the sun, would Kepler's 2nd Law still be valid? Explain your reasoning. ...
... Question 13: If the sweep segments were measured from the empty focus and not from the sun, would Kepler's 2nd Law still be valid? Explain your reasoning. ...
NEXT MEETING 7:30 p.m., Monday, November 3, 2014
... Along the way, researchers made a discovery: Two of those stars are a binary system, something that was suspected but had not been verified. Measurements made at the Keck Observatory in Hawaii confirmed the binary, Melis said. Resolving a controversy? Melis said his team’s work resolves a decades-lo ...
... Along the way, researchers made a discovery: Two of those stars are a binary system, something that was suspected but had not been verified. Measurements made at the Keck Observatory in Hawaii confirmed the binary, Melis said. Resolving a controversy? Melis said his team’s work resolves a decades-lo ...
Sun, Earth, and Moon
... How many stars are in our solar system? How many days does it take for the Earth to revolve around the sun? • How many low and high tides on Earth every 24 hours? ...
... How many stars are in our solar system? How many days does it take for the Earth to revolve around the sun? • How many low and high tides on Earth every 24 hours? ...
May - Fort Worth Astronomical Society
... Cloudy skies have kept the young observers at Rosemont 6th from viewing the alignment of the five visible planets. However, Yolanda Navarette did manage to "sneak a peak" between clouds of Venus and Saturn and the moon by Jupiter and do an observation report. Yolanda has been diligent all year in he ...
... Cloudy skies have kept the young observers at Rosemont 6th from viewing the alignment of the five visible planets. However, Yolanda Navarette did manage to "sneak a peak" between clouds of Venus and Saturn and the moon by Jupiter and do an observation report. Yolanda has been diligent all year in he ...
WORD - hrsbstaff.ednet.ns.ca
... (d) Neptune, Uranus, Sol, Jupiter 35. What are the four Jovian Planets? (a) Saturn, Neptune, Jupiter, Uranus (b) Mars, Ceres, Mercury, Saturn (c) Uranus, Mercury, Mars, Neptune (d) Charon, Neptune, Uranus, Mars 36. What is another name for an interstellar gas cloud? (a) Nebula (b) Coma (c) Corona (d ...
... (d) Neptune, Uranus, Sol, Jupiter 35. What are the four Jovian Planets? (a) Saturn, Neptune, Jupiter, Uranus (b) Mars, Ceres, Mercury, Saturn (c) Uranus, Mercury, Mars, Neptune (d) Charon, Neptune, Uranus, Mars 36. What is another name for an interstellar gas cloud? (a) Nebula (b) Coma (c) Corona (d ...
1 - Astronomy
... 11. Any model for the planets must explain the various motions of all celestial objects, such as the Sun, Moon, and planets. A Model of Planetary Motion: Epicycles 1. Ptolemy’s geocentric model was able to explain the planetary motions using epicycles. An epicycle is the circular orbit of a planet, ...
... 11. Any model for the planets must explain the various motions of all celestial objects, such as the Sun, Moon, and planets. A Model of Planetary Motion: Epicycles 1. Ptolemy’s geocentric model was able to explain the planetary motions using epicycles. An epicycle is the circular orbit of a planet, ...
Properties of the Asteroids
... pulverising the outside layers – the impacts that an asteroid experiences in its history are largely responsible for shaping their appearance today. The pieces chipped away from an asteroid by the impacts create asteroid moons if they are not expelled with sufficient velocity to escape gravitational ...
... pulverising the outside layers – the impacts that an asteroid experiences in its history are largely responsible for shaping their appearance today. The pieces chipped away from an asteroid by the impacts create asteroid moons if they are not expelled with sufficient velocity to escape gravitational ...
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.