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05-Circular motion.pptx
05-Circular motion.pptx

... → Something must provide the force – Centripetal force Centripetal force is NOT a force of nature. Any of the forces we discussed in Chapter 4 can play a role of centripetal force when object’s moving along a circle. To solve problems in uniform circular mo+on → apply the same set of rules prov ...
Astrobiological Stoichiometry
Astrobiological Stoichiometry

... of that element (by number) in the Sun. Elements heavier than He are termed ‘‘metals.’’ Because the Sun is considered to sample the average interstellar medium, it is presumed that all stars will share the Sun’s relative proportions of metals. The relative sizes of the boxes for C, O, etc., are pres ...
1 kg coal - Lick Observatory
1 kg coal - Lick Observatory

... force to overcome the electromagnetic force holding the electrons to the nucleus. Gas in the sun is ionized: the electrons and nuclei are no longer bound by the electromagnetic force - like a rocket accelerating to the escape speed and no longer being bound to the gravitational pull of the earth A p ...
PDF only - at www.arxiv.org.
PDF only - at www.arxiv.org.

... Thanks to Bethe and his followers we know today in great detail that the Sun is a huge fusion reactor. Although the solution of the riddle may be safely dated to 1939, more than a decade earlier Arthur Eddington had anticipated that thermonuclear reactions power the Sun [Hufbauer 2006]. Our present ...
Asteroids, Comets, and Dwarf Planets Their Nature, Orbits, and
Asteroids, Comets, and Dwarf Planets Their Nature, Orbits, and

... darker asteroid. It will therefore shine less brightly at infrared wavelengths, relative to its visible brightness, than the dark asteroid. Once the reflectivity and size are known, the size can be determined from the asteroid brightness: for a given reflectivity and distance, the brightness depends ...
3. Chapter 12
3. Chapter 12

... been told that things in “outer space” never change. This conclusion was reached by astronomers who made observations using the best instruments available to them at the time. Scientific theories develop and change as we learn more. New evidence can cause scientists to rethink existing theories. Bet ...
Astr 102 Lec 6: Basic Properties of Stars
Astr 102 Lec 6: Basic Properties of Stars

... • Measure distance • Measure brightness ...
NAME ..........................................................................CLASS.............ADM
NAME ..........................................................................CLASS.............ADM

... b) The earth surface is made up of land __________ % and water _________. It is about ___________ million km from the sun and it as old as______________ million years. It receives energy in form of radiation from a start known as the sun. The sun is made up of two main gases name ___________________ ...
CH02.AST1001.F16.EDS
CH02.AST1001.F16.EDS

... rejected the correct explanation (1) because they did not think the stars could be that far away. Thus the stage was set for the long, historical showdown between Earth-centered and Sun-centered systems. ...
Chapter 2: Discovering the Universe for Yourself 2.1 Patterns in the
Chapter 2: Discovering the Universe for Yourself 2.1 Patterns in the

... •  Earth's axis points in the same direction (to Polaris) all year round, so its orientation relative to the Sun changes as Earth orbits the Sun. •  Summer occurs in your hemisphere when sunlight hits it more directly; winter occurs when the sunlight is less direct. •  AXIS TILT is the key to the se ...
doc - Eu-Hou
doc - Eu-Hou

... The telescope is fully steerable, i.e. it can be directed to any position in the sky and can be kept on a specific position. This is accomplished by a computer control system, which calculates every 10th of a second the exact position. In this way, the rotation of the Earth (and other more complex m ...
Measuring the Properties of Stars - Sierra College Astronomy Home
Measuring the Properties of Stars - Sierra College Astronomy Home

... stars) is equal to a brightness change of 100 times (so as to closely match Hipparchus’s original ...
Eighth Grade Science
Eighth Grade Science

... State how wind and the rotation of the Earth influence surface currents; Discuss how ocean currents affect weather and climate; Describe the causes and effects of density currents; Explain how an upwelling occurs Describe how wind can form ocean waves; Explain the movement of particles in a wave; De ...
IFAS Novice Handbook - Indiana Astronomical Society
IFAS Novice Handbook - Indiana Astronomical Society

... something to improve your observing power. If you are new to astronomy as a hobby, you will probably have been told by now that a good pair of binoculars are well worth spending your money on. They are cheap, robust, and are easy to maintain and store. A good size to start from would be 10X50's. Wha ...
Earth Science ® Curriculum Guide - Mount Vernon City School District
Earth Science ® Curriculum Guide - Mount Vernon City School District

... benchmarks for student achievement. Standards work best when they are well defined and clearly communicated to students, teachers, administrators, and parents. The focus of a standards-based education system is to provide common goals and a shared vision of what it means to be educated. The purposes ...
Modified True/False - Indicate whether the statement is true or false
Modified True/False - Indicate whether the statement is true or false

... ____ 17. HS-ESS1-2 The apparent shift in a star’s position caused by the motion of the observer is called ____. a. Luminosity c. Apparent magnitude b. Absolute magnitude d. Parallax ____ 18. HS-ESS1-1 Small, massive, dense object that has gravity so immense that nothing—not even light— can escape it ...
The Dynamics of the Galaxies in the Local Group
The Dynamics of the Galaxies in the Local Group

... Milky Way Future • The Milky Way will merge with the Andromeda galaxy to become an elliptical galaxy – Their collision does not need to be as direct a hit as shown in the movie – They do always approach each other close enough to make a merger inevitable ...
Celestial Globes Armillary Spheres
Celestial Globes Armillary Spheres

... 7 - Ptolemy: Used a horizon ring in order to make the celestial globe more universal (fig 2), as opposed to the previous globes that only considered the sky from Rhodes. The above list is brief, but it gives an indication of the type of knowledge that was all potentially passed over to the Islamic w ...
Seasons and the Appearance of the Sky
Seasons and the Appearance of the Sky

... • Earth’s axis points in the same direction (to Polaris) all year round, so its orientation relative to the Sun changes as Earth orbits the Sun. • Summer occurs in your hemisphere when sunlight hits it more directly; winter occurs when the sunlight is less direct. • AXIS TILT is the key to the seaso ...
ASBA Yearlongplan Science 8
ASBA Yearlongplan Science 8

...  Describe the largest moons of each of the outer planets.  Describe how comets change when they approach the Sun.  Distinguish among comets, meteoroids, and asteroids.  Explain that objects from space sometimes impact Earth. Chapter 13: Stars and Galaxies Content:  For many years, people have b ...
Highlights in astronomical polarimetry
Highlights in astronomical polarimetry

... First spectropolarimetric observations I At the middle of the XIX century, the phenomenon of polarization is fairly well understood, but it is necessary to wait for more than 50 years before the first astronomical application combining polarimetry with spectroscopy. In 1908 Hale succeeds in observi ...
File - metc instructors collab site
File - metc instructors collab site

... Defines and evaluates the co-latitude, polar distance and zenith distance and uses them as the sides of the PZX triangle Solves the PZX triangle to find the calculated zenith distance of the body when it is out of the meridian Applies this calculated zeníth distance to the true zenith distance of th ...
J Gravity and space
J Gravity and space

... Framework yearly teaching objectives – Forces • Recognise that gravity is a force of attraction between objects, that this force is greater for large objects like the Earth but gets less the further an object moves away from the Earth’s surface; use these ideas to explain: – how weight is different ...
Perseid Watch at Weiser State Forest August 12
Perseid Watch at Weiser State Forest August 12

... made a motion to accept the minutes. Chip Templin seconded the motion. Minutes were approved. Financial report. Charles Oldland stressed that two people counted all currency collected at the star party. Two speakers at the star party returned their honorarium checks. We had a few refunds approved fo ...
Stars
Stars

... Basic Properties of Stars Magnitude • The classification of stars by absolute magnitude allows comparisons that are based on how bright the stars would appear at equal distances from an observer. The disadvantage of absolute magnitude is that it can be difficult to determine unless the actual distan ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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