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Astronomy Daystarter Questions
Astronomy Daystarter Questions

... 4. Yesterday is but a memory, tomorrow is but a dream. This implies that time does NOT exist at all, because it precludes what? a. Order c. Simultaneity b. Duration d. Continuity 5. You look up at the sky. You see a star that has a size and mass indicating that it will exist on the main sequence for ...
Astronomy Unit BM study guide
Astronomy Unit BM study guide

... light from the nearest large galaxy, Andromeda, was emitted 2.5 million years ago. Therefore, the images we see of these objects are how they looked at the time in the past when their light left them. The further away an object is, the older the light is that we are receiving from it. The shapes of ...
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Directions: your answers to the questions below. Check your answers... and then go ...

... 5. According to the Law of Universal Gravitation, two objects are attracted to each other. The greater the total mass of the two objects, the stronger the attraction, or gravitational force. The greater the distance between the objects, the weaker the gravitational force. The orbital speed of a plan ...
THE SCIENTIFIC METHOD
THE SCIENTIFIC METHOD

... This chapter introduces the scientific method, the process scientists use to interpret the physical universe. Science is a living body of knowledge whose laws and theories are subject to constant test and change. Although science can never arrive at an "ultimate truth," it has nevertheless successfu ...
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... Earth. This means that the Earth, Sun, and Moon are nearly in a straight line, with the Earth in the middle. The Moon that we see is very bright from the sunlight reflecting off it. ...
Phys133 SAMPLE questions for MidTerm#1
Phys133 SAMPLE questions for MidTerm#1

... B) It is the star straight overhead. C) It appears very near the north celestial pole. D) It can be used to determine your longitude on Earth. E) It is the star directly on your northern horizon. ...
Starry Monday at Otterbein
Starry Monday at Otterbein

... • Is the Earth or the Sun the center of the solar system? • How do we decide between these two theories? • Invoke the scientific methods: – both theories make (different) predictions – Compare to observations – Decide which theory explains data ...
The Celestial Sphere - University of North Texas
The Celestial Sphere - University of North Texas

... – The Sun, Moon, planets, and stars appear to rise in the east, cross the meridian due south, and set toward the west. – Celestial objects are said to transit when the cross the celestial meridian in the southern sky. • This is when they are highest in the sky. ...
relative size and distance
relative size and distance

... • Based on the Earth's orbit around the Sun. • Ecliptic is the plane of the Earth's orbit projected on to the celestial sphere. – The 12 zodiac constellations are located in a band following the ecliptic. – The Sun, Moon, and planets are found on or near the ecliptic. – The ecliptic is tilted 23.5o ...
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Circular Motion and Gravitation Jeopardy Review Game

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... modern astronomy but modern science in general. ...
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... The moon actually falls, but because it is not stationary (it has an initial radial speed), it follows a curved path around the Earth. Newton theorized that the Moon did not get attracted with the same force as the apple nor did it fall with the same gravitational acceleration. Why not? 1. The moon ...
Astronomy Merit program @ Huntley Meadows Park
Astronomy Merit program @ Huntley Meadows Park

... B. Sketch the phase and the daily position of the Moon at the same hour and place, for four days in a row. Include landmarks on the horizon such as hills, trees, and buildings. Explain the changes you observe. C. List the factors that keep the Moon in orbit around Earth. D. With the aid of diagrams, ...
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... Orbits are ellipses: this one would have been the same. All that’s necessary for this is a “Keplerian” system, where all (or at least the vast majority) of the mass in the system is concentrated towards the center (inside the orbit of the innermost planet you’re considering). Equal areas in equal ti ...
Circular Motion and Gravity Jeopardy
Circular Motion and Gravity Jeopardy

... What are Newton-meters or Foot-pounds? ...
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Part 1) Steve Quayle is Right! A Dwarf Star, Capturing

... magnitude of the force of attraction between two masses is directly proportional to the mass of body A multiplied by the mass of body B. Now, we know that passing meteors are sucked into Earth every single day of our lives. Why is this so? It's simple, yet some folks need to be taught that when a sm ...
NEXT MEETING 7:30 p.m., Monday, November 3, 2014
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... Visual vs. radio measurements When astronomers estimate stellar distances for objects that are relatively close to Earth, they use a method called parallax. Simply speaking, measurements of a star’s position relative to other stars are taken when Earth is at either side of its yearlong orbit. By mea ...
Study Notes Lesson 13 Gravitational Interactions
Study Notes Lesson 13 Gravitational Interactions

... Cancellation of gravitational force: If Earth were of uniform density, half way to the center gravitational force would be exactly half that at the surface. Cancellation is of the entire surrounding shell of inner radius equal to your radial distance from the center. Half way down, for example, all ...
Astronomy and the Universe - Department of Physics and Astronomy
Astronomy and the Universe - Department of Physics and Astronomy

... – A set of related hypotheses can be pieced together into a self consistent description of natural observations ...
Ancient Astronomy
Ancient Astronomy

... • Having measured the position of a new star (now known as Tycho’s supernova), and observed no parallax, he concluded that it was farther away than the Moon. • This led him to question the Ptolemaic theory, according to which objects farther away than the Moon were celestial (therefore perfect) and ...
TENTH GRADE SCOPE AND SEQUENCE DRAFT
TENTH GRADE SCOPE AND SEQUENCE DRAFT

... Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal principles of gravitation allow predictions regarding the motions of objects within the Galaxy and beyond. Earth’s motion, position, and posture account for a variety of cyclic events ob ...
The Prague Astronomical Clock
The Prague Astronomical Clock

... the sun as it spins on its axis and must turn a little bit more than 360 deg to again reach the Sun’s meridian transit starting point. Stars are so far away compared to the Sun that the Earth’s orbital motion has no effect on the time of a star’s meridian transit. Declination of the Sun The Earth’s ...
Age and Origin of the Earth
Age and Origin of the Earth

... • Expanding universe hypothesis- Edvin Hubble1920, validated in 1972. • Everything originated from a point-singularity • Gigantic explosion- 15 billion years ago, energy converted into matter, first atoms began to form • Matter expanded to form billions of galaxies, in time with their stars with the ...
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Lunar theory

Lunar theory attempts to account for the motions of the Moon. There are many irregularities (or perturbations) in the Moon's motion, and many attempts have been made to account for them. After centuries of being problematic, lunar motion is now modeled to a very high degree of accuracy (see section Modern developments).Lunar theory includes: the background of general theory; including mathematical techniques used to analyze the Moon's motion and to generate formulae and algorithms for predicting its movements; and also quantitative formulae, algorithms, and geometrical diagrams that may be used to compute the Moon's position for a given time; often by the help of tables based on the algorithms.Lunar theory has a history of over 2000 years of investigation. Its more modern developments have been used over the last three centuries for fundamental scientific and technological purposes, and are still being used in that way.
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