Wonders Of The Sky 2009 Eclipses
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There are two types of eclipses: solar eclipses which occur when the moon passes between the earth and sun, and lunar eclipses which occur when the earth passes between the sun and moon. During a solar eclipse, the moon can block all, some, or none of the sun, resulting in total, partial, or annular eclipses. A total solar eclipse occurs when the moon completely covers the sun, briefly turning day to night, while partial eclipses only block part of the sun. Lunar eclipses occur during a full moon when the earth blocks the sun's light from reaching the moon, causing it to take on a red color from the sunlight bending through the earth's atmosphere.
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Eclipse presentation[1]
A lunar eclipse occurs when the Moon passes through the Earth's shadow. There are three types of lunar eclipses - total, partial, and penumbral - depending on how much of the Moon passes through the Earth's umbra or penumbra. During a total lunar eclipse, the Moon takes on a red color due to refraction of sunlight through the Earth's atmosphere. A solar eclipse occurs when the Moon passes between the Earth and the Sun, casting its shadow on parts of Earth. There are also three types of solar eclipses - total, partial, and annular - depending on the Moon's position and alignment with the Earth and Sun.
phases_eclipses.ppt
The document discusses lunar phases and eclipses. It explains that the moon orbits the Earth at an angle and its phases (new, waxing crescent, first quarter, etc.) are caused by the changing portion of its surface that is illuminated by the sun. It describes three types of lunar eclipses that occur when the Earth passes between the sun and moon, casting its shadow on the moon. Solar eclipses happen when the moon passes between the Earth and sun, casting its shadow on parts of the Earth. The document also briefly discusses how tides are caused by the gravitational pull of the moon and sun on the Earth's oceans and atmosphere.
Ch. 17 l.s. 2
The document discusses patterns that can be seen in the night sky and provides details about the moon phases and eclipses. It explains that the moon revolves around the Earth and rotates on its axis, causing the shapes and illumination that we see over the course of a month. The phases include the new moon, waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, third quarter, and waning crescent. Eclipses occur when the moon or Earth pass through each other's shadows. There are lunar and solar eclipses. The document also briefly discusses stars and constellations visible in the night sky.
D. the moon
There were several theories proposed to explain the origin of the Moon throughout history. The first was the fission theory from the 19th century, which suggested that the Moon formed when a chunk of Earth was pulled away by the Sun's gravity as Earth rapidly spun. Later theories included the capture theory, where the Moon was a wandering planet captured by Earth, and the coaccretion theory where the Moon and Earth formed together from the same material. Currently, the giant impact theory is favored, where a Mars-sized body collided with Earth, ejecting debris that coalesced to form the Moon. This theory best explains the compositional similarities and differences between Earth and the Moon.
Solar and Lunar eclipse
This document discusses eclipses, including lunar and solar eclipses. It explains that eclipses occur when the sun, earth, and moon are aligned so that one celestial body casts a shadow on the other. A lunar eclipse can only happen during a full moon, while a solar eclipse can only happen during a new moon. The document outlines the different types of solar eclipses and provides safety precautions for viewing a solar eclipse directly.
Shadows and Solar-Lunar Eclipses
This document discusses shadows, solar eclipses, and lunar eclipses. There are four types of solar eclipses: total, annular, hybrid, and partial. During a total solar eclipse, the moon completely obscures the sun, allowing the solar corona to be seen. An annular solar eclipse occurs when the moon is not large enough to completely cover the sun, leaving a ring of sunlight visible. A hybrid eclipse shifts between total and annular. A partial solar eclipse occurs when the moon only partially obscures the sun. There are also three types of lunar eclipses: total, partial, and penumbral.
Phases of the_moon
The document discusses the phases of the moon. It explains that as the moon orbits the Earth over 28 days, the angle of illumination changes from our perspective, causing it to appear to go through eight phases from new moon to full moon and back again. These phases include the waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, last quarter, and waning crescent. Diagrams and a modeling activity are provided to illustrate how the changing positions of the Earth, moon, and sun cause the moon to appear to change shape over the course of its orbit.
Think Science: What Are Eclipses, by Craig Bobchin
Craig Bobchin, of Astronomy4You, prepared this presentation for Texas Public Radio's Think Science event on April 8, 2024.
Eclipses - Solar and Lunar Eclipses
The document discusses lunar and solar eclipses. It explains that lunar eclipses occur when the Earth passes between the Sun and Moon, casting its shadow on the Moon. Solar eclipses occur when the Moon passes between the Earth and Sun, casting its shadow on parts of Earth. For an eclipse to occur, the Sun, Moon and Earth must be aligned on the same plane. The document provides details on the conditions required to view lunar and solar eclipses and why the Moon appears red during a lunar eclipse.
Similar to Wonders Of The Sky 2009 Eclipses (20)
An astronomical event that occurs when one celestial object (Earth or moon) m...
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Think Science: What Are Eclipses, by Craig Bobchin
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Wonders of the sky test slides alphabetic order 2010
This document lists various natural phenomena that can be observed in the sky, including different types of clouds, celestial events like eclipses and meteor showers, atmospheric optics phenomena like rainbows and halos, and luminous phenomena like the aurora and zodiacal light.
Jovian Planets (2010)
1. The document provides information about the planet Jupiter and its moons. Jupiter is the largest planet in the solar system and has many moons, including the four largest Galilean moons - Io, Europa, Ganymede, and Callisto.
2. The Cassini spacecraft obtained images of Saturn and its rings and moons. Saturn has a vast ring system made of small particles of ice and rock. It has several large moons such as Titan, which has a thick atmosphere.
3. The document discusses the gas giant planets Jupiter and Saturn, their compositions, atmospheric features, rotations, magnetic fields, rings and moons as observed by spacecraft such as Galileo, Cassini, and Voyager.
Topic Pioneers In Astronomy (2008)
The document discusses key figures in the development of astronomy and our understanding of planetary motion, including:
1) Ptolemy first proposed the geocentric model, placing Earth at the center. Copernicus later developed the heliocentric model with the Sun at the center.
2) Tycho Brahe made very accurate observations of planetary positions, which Kepler used to formulate his three laws of planetary motion.
3) Newton later published his law of universal gravitation and laws of motion, unifying Kepler's laws and gravity to explain orbital motions.
4) Edmond Halley used Newton's theories to predict the periodic return of Halley's Comet.
Intro To The Solar System 2010
The document discusses the formation and current state of the solar system. It describes how the solar system formed from a large cloud of gas and dust via the nebular hypothesis. The inner planets formed from solid debris while the outer planets retained gases. Today the planets orbit counterclockwise in nearly the same plane, with Pluto having a more tilted orbit. The document also provides comparisons of planetary properties like size, mass, temperature, and classification as terrestrial or Jovian planets.
Ch.20 Notes Mc Neely 2010
This document provides an overview of weather patterns and severe storms, including:
1) It describes different air masses and how they are classified based on their source regions and temperatures. This includes polar, tropical, continental, and maritime air masses.
2) It discusses specific weather phenomena driven by air masses, such as lake effect snow, monsoons, and Indian summers.
3) It outlines different types of fronts that form when air masses meet, including warm, cold, stationary, and occluded fronts.
4) It provides an overview of mid-latitude cyclones, thunderstorms, tornadoes, hurricanes, and highlights some significant storms like the Tri-State Tornado and Hurricane
Cloud Diary
The document provides instructions for creating a cloud diary to record daily observations of cloud types and other atmospheric phenomena. Students are directed to go outside each day and sketch the visible clouds in their diary, noting the date, time, and Latin names of observed clouds or "clear" if no clouds. The goal is to make observations at the same time each day to track changes in cloud types and phenomena like halos, sundogs, and coronas.
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Ch.19 Notes Mc Neely 2009
1. Air pressure is caused by the weight of air above exerting pressure in all directions, and differences in air pressure cause wind as air moves from high to low pressure areas.
2. Global wind patterns are caused by uneven heating of the Earth's surface by the sun, which causes large scale rising and sinking of air and the formation of circulation cells.
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Wonders Of The Sky 2009 Darkening Sky
The document discusses several natural phenomena visible in the night sky, including twilight, earthshine, crescent moons, planets like Mercury and Venus, conjunctions between celestial bodies, satellites, and noctilucent clouds. Twilight is caused by the Earth's atmosphere, while earthshine allows the dark side of the moon to glow from reflected light from Earth. Morning and evening crescents have different names. Inferior planets like Mercury and Venus can only be seen either after sunset or before sunrise. Satellites resemble moving stars in the sky. Noctilucent clouds are only visible from high latitudes in the summer.
Wonders Of The Sky 2009 Sunset Sky
The document discusses various optical phenomena that can be observed in sunrises and sunsets. It explains how the setting or rising sun may appear oval-shaped or broken into layers due to atmospheric effects. Other topics covered include green flashes, crepuscular rays, volcanic sunsets, the earth's shadow, moonrises, harvest moons, and rocket contrails visible at sunset.
Wonders Of The Sky 2009 Day Sky
The document discusses various optical phenomena that can be seen in the sky, such as rainbows, halos, sun pillars, and iridescent clouds. It describes the factors that influence the color of the sky and some rare atmospheric optical effects like glories, moonbows, and circumzenithal arcs. The document includes pictures demonstrating many of the atmospheric optical phenomena it describes.
Day And Night Sky Phenomena Study Guides 2008
The document is a study guide covering various natural phenomena that can be observed in the day and night sky, including rainbows, halos, sun dogs, lunar phases, planets, meteors, the Milky Way, auroras, and eclipses. It provides questions about the factors that affect sky color, celestial events visible at sunrise and sunset, optical effects of the moon, characteristics of meteor showers, and details of solar and lunar eclipses.
Ch.18 Notes Mc Neely 2009
The document summarizes key concepts about the water cycle and atmospheric moisture. It describes the three states of water, processes like evaporation and condensation, cloud formation mechanisms including convection and orographic lifting, different cloud types classified by height and shape, and various forms of precipitation including rain, snow, hail and acid rain. Diagrams illustrate concepts like the water cycle, adiabatic processes, cloud classification and hailstone formation.
Ch. 18 Study Guide 2009
The document is a study guide covering topics about water in the atmosphere including the water cycle, humidity, cloud formation, and cloud types. It discusses processes like evaporation, condensation, and adiabatic cooling that cause water vapor to condense into clouds. Students are asked questions about changes of state, cloud formation mechanisms, cloud classification, and types of precipitation to test their understanding of these atmospheric water concepts.
Time And The Sun
The document describes how to create an analemma graph showing the changing position of the sun at solar noon throughout the year based on the observer's latitude. It provides information on altitude, zenith, and the equation of time. The observer completes a table with data on the sun's position at different dates and uses this to graph an analemma figure-8 pattern. Questions ask about maximum/minimum altitudes, the dates closest to the equator, seasons when solar time is ahead/behind, and how the first analemma photo was taken. It also discusses the analemma pattern on Mars based on its axial tilt and elliptical orbit.
Time & Calendars Study Guide 2010
The document is a study guide for a time and calendars class containing questions about various calendars and timekeeping systems used throughout history. It includes questions about the Gregorian calendar, Roman calendar, Julian calendar, lunar calendars, the equation of time, analemma, sundials, precession, dog days, French Revolutionary calendar, Maya calendar systems, and the World Calendar.
Moon, Sun, And Seasons
The document discusses how the height of the sun and moon in the sky changes with the seasons. It provides data on the noon altitude of the sun and maximum altitude of the moon every few days for one year. The data is to be graphed to show the seasonal patterns, with the full moon's behavior mirroring the sun's. Analysis questions examine when the sun and moon appear at the same altitude, how new moons relate to the sun, and what seasons are best for seeing low, orange "honeymoon" full moons.
Cycles Study Guide 2009
This document contains a study guide with questions about cycles of the day, month, and year. It asks about the movement of shadows, constellations, phases of the moon, seasons, equinoxes, solstices, and how celestial objects like the sun, moon, and stars appear to move through the sky over different periods of time. The questions cover topics like how sundials inspired clocks, using the Big Dipper to tell time, the cause of moon phases, the difference between summer and winter sun positions, and seasonal star patterns.
Seasons Interactive
The document describes an interactive simulation that models the relationship between Earth's position relative to the sun throughout the year and the resulting seasonal changes in temperature and daylight hours in four cities located in different hemispheres. Students are asked to use the simulation to collect monthly temperature and daylight data for each city, create line graphs to visualize the patterns, and then answer questions about the seasonal changes and how they relate to each city's location and proximity to the equator or tropics.
Ch.17 Notes Mc Neely 2009
The document discusses key topics about Earth's atmosphere including its composition, structure, and factors that influence climate. It describes the four main layers of the atmosphere - troposphere, stratosphere, mesosphere, and thermosphere - and explains how temperature varies within each layer. Additionally, it covers how Earth's orientation and motions affect seasonal changes in temperature and daylight hours at different latitudes. Climate is influenced by proximity to oceans and seas, elevation, cloud cover, and other geographic factors.
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Wonders Of The Sky 2009 Eclipses
- 1. Wonders of the Sky
- 2. Eclipses
- 7. Moon’s Shadow from Mir, 1999
- 11. Eclipse Shadows Above: View of eclipse through a telescope, note the corresponding shadows (right)
- 14. Diamond Ring Effect Last remaining bit of sun’s visible surface before totality
- 19. Chromosphere & Inner Corona
- 21. 360-Degree “Sunset” An all-sky image during totality Note, “sunset” colors surround entire horizon
- 25. Shadow Band Still Image
- 27. Safe-totality NOT safe- partial eclipses
- 30. Again, Jones’s sneaky colleagues aimed the telescope at the sun…
- 34. Eclipse ‘94
- 35. Annular Geometry
- 37. Lunar Eclipse
- 39. Lunar Eclipse Partial Stages
- 42. Eclipse ’04: Red Moon
- 43. Earth’s Shadow
- 49. Full Moon Night