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Astronomy
Astronomy

... these spots moving, so he realized that the Sun must be rotating. He thought that if the Sun was moving, we probably were rotating on an axis. • Galileo observed 4 points of light that changed their positions with time around the planet Jupiter. He concluded that these were objects in orbit around J ...
SKYTRACK Glossary of Terms
SKYTRACK Glossary of Terms

... Solstice – (a) The two points at which the Sun is at its greatest distance from the celestial equator. It happens twice each year, when the tilt of the Earth's axis is most inclined toward or away from the Sun, causing the Sun's apparent position in the sky to reach its northernmost or southernmost ...
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... possible because of – Quantum Mechanics: the laws of QM are inherently stochastic; QM predicts the probability of what might happen, not what will actually happen – Possibility of chaotic behavior: very small differences in the initial conditions can have vastly different effects (a butterfly’s wing ...
Exploring the Universe
Exploring the Universe

... • When the moon is new, the side that is facing you is dark, so you can’t see it. ...
Why do things move?
Why do things move?

... • Good news: no more need for complex epicycles to explain retrograde motion! Mars orbit ...
Astronomy - Fort Thomas Independent Schools
Astronomy - Fort Thomas Independent Schools

... set forth the heliocentric model, indicating that Mercury and Venus are inside the Earth’s orbit of the Sun and that Mars, Jupiter and Saturn are outside the Earth’s orbit. Brahe: Amassed a huge collection of data regarding the position and motion of planets at his observatory Uranaborg. Galileo: Fi ...
Revolutions of Earth
Revolutions of Earth

... Certainly no one today doubts that Earth orbits a star, the Sun. Photos taken from space, observations made by astronauts, and the fact that there has been so much successful space exploration that depends on understanding the structure of the solar system all confirm it. But in the early 17th centu ...
Chap. 4: Gravitation and the Waltz of the Planets
Chap. 4: Gravitation and the Waltz of the Planets

... Heliocentric Model by Copernicus • Heliocentric (Suncentered) model: all the planets, including the Earth, revolve about the Sun • A heliocentric model simplifies the explanation of the retrograde motion of planets • Occam’s razor: simple explanations of phenomena are most likely to be correct ...
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... (iii) We all know/expect that many current and next-generation astronomical instruments are/will be equipped with polarimetric capabilities. But it is more surprising to learn that even smartphones may turn into spectropolarimeters that can be used by anyone to perform measurements of aerosols in th ...
CST Prep- 8th Grade Astronomy 19. Sketch a planet
CST Prep- 8th Grade Astronomy 19. Sketch a planet

... 9. Combining four hydrogen atoms to create helium is how the sun produces its energy. This process is called ...
PPT - osmaston.org.uk
PPT - osmaston.org.uk

... 4. Planetary spins are almost exclusively prograde, but vorticity in a Keplerian disc is retrograde. Where did they nucleate and get their spins? 5. Solar System satellites are almost exclusively prograde w.r.t. spin of their planet. Why? ...
Space Station One, Grades 4-8 Program Description: Have you ever
Space Station One, Grades 4-8 Program Description: Have you ever

... 4. The structure and composition of the universe can be learned from the study of stars and galaxies, and their evolution. As a basis for understanding this concept, students know: a. galaxies are clusters of billions of stars, and may have different shapes. b. the sun is one of many stars in our ow ...
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Friday, August 29

... – Moon 0.5, Sun 0.5, Jupiter 20”, Betelgeuse (α Ori) 0.05” ...
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astr221lect2x

13.14 The Eight Planets
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... relate to the process of scientific discovery? Scientists observed that Uranus was a plant; then they discovered that its motion was not smooth. They made a hypothesis that another object was tugging on Uranus. They predicted where the other object was; then they tested their hypothesis and discover ...
Celestial Sphere - Otterbein University
Celestial Sphere - Otterbein University

... itself in the same time •  always shows us the same side! •  “dark side of the moon” (not dark at all!) ...
PowerPoint Presentation - ASTR498E High energy
PowerPoint Presentation - ASTR498E High energy

... The area under consideration must be oriented face-on to lineof-sight to the star In principle, this definition works for any kind of energy emitted by the star… most commonly, we mean e/m radiation Sometimes, it is useful to consider the observed flux in a restricted range of e/m wavelengths (e.g., ...
The Ever Expanding Universe
The Ever Expanding Universe

... Herculean task that involved over 2000 years of work! The Greeks knew how to do it using their mathematical invention trigonometry (the mathematics of right triangles), but a telescope precise enough to measure extremely tiny angles was not available until the 19th century when Friedrich Bessel succ ...
In the Spring of 2007 two of us began planning a new course in
In the Spring of 2007 two of us began planning a new course in

... a. It will have moved toward the North. b. It will have moved to a position higher in the sky. c. It will stay in the same position. d. It will have moved to a position closer to the horizon. e. It will have moved toward the west. 5. Which sentence best describes why the Moon goes through phases? a. ...
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Friday Feb 25th, 2000

... period = against the stars) ~ month – Similar to a woman’s cycle – Luna always a female association in all cultures ...
BIO 10 Lecture 2
BIO 10 Lecture 2

... • The Moon formed as a result of an early catastrophic collision between Earth and another planetoid, which also created the tilt in Earth’s axis • The heat of early bombardments and impacts kept Earth hot and enabled heavier elements (principally iron) to flow to the core, where they remained molt ...
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384 kb

... The lecture will feature spectacular videos of the Sun’s surface taken from Hinode. The observation satellite has made discoveries that elucidate how and why solar activity fluctuates periodically, registering a minimum every eleven years or so. The Sun is currently into Solar Cycle 24 – a numbering ...
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... Recognize that one half of the Moon is always facing the Sun and, therefore, one half of the Moon is always lit Relate the apparent change in the moon’s position in the sky as it appears to move east-to-west over the course of a day to Earth’s counterclockwise rotation about its axis Describe how th ...
lecture3
lecture3

... Galileo arrogantly published his findings supporting the Copernican view and belittling the Catholic church. His book “Dialogues” featured a character Simplicio (a simpleton) who tries to defend the church’s geocentric doctrine. Galileo spent the rest of his life in house arrest.  Check out “Galile ...
TOP 78 ASTRONOMY FACTS 1. The solar system consists of the
TOP 78 ASTRONOMY FACTS 1. The solar system consists of the

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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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