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SDO | solar dynamics observatory
SDO | solar dynamics observatory

... • Optional: “East” and “West” popsicle sticks • Optional: Zodiac constellation signs • Optional: NASA Solar Pizza Background Information: Earth revolves around the Sun once per year. The seasons on Earth are caused by the tilt of Earth on its rotation axis, which is approximately 23.5 degrees with r ...
1 Marsbugs: The Electronic Astrobiology Newsletter, Volume 12
1 Marsbugs: The Electronic Astrobiology Newsletter, Volume 12

... In the new CU-Boulder scenario, it is a hydrogen and CO2-dominated atmosphere that leads to the production of organic molecules, not the methane and ammonia atmosphere used in Miller's experiment, Toon said. Tian and other team members said the research effort will continue. The duration of the hydr ...
Version A - Otterbein University
Version A - Otterbein University

... example, say we are seeing Taurus in the south at midnight on December 1. At what other combination of date and time do we see Taurus in the south? a. January 1 at 2 am b. November 1 at 10pm c. February 1 at 6pm d. December 15 at 11pm e. None of the above 31. The sidereal day (a full rotation of the ...
Version B - Otterbein University
Version B - Otterbein University

... a. You would have the same view since the Earth barely moves around the Sun in two hours. b. Aries would be in the South because the stars shift by one constellation. c. Pisces would be in the South because the stars shift a constellation per hour. d. Gemini would be highest in the South because the ...
Lecture 10
Lecture 10

... objects, which are defined by reference to the celestial equator and celestial poles, must also be constantly changing. • Because of this change in the direction of the Earth's pole with time, the coordinate systems of RA and DEC that we adopt for one epoch are actually different for other epochs. • ...
Document
Document

... What Causes the Seasons? • Because of the tilt of the Earth’s axis, the altitude the Sun reaches changes during the year: It gets higher above the horizon during the summer than it does during the winter. • Also, the length of the daytime hours changes during the year: the daylight hours are longer ...
Astronomy Final review key - Hicksville Public Schools
Astronomy Final review key - Hicksville Public Schools

... The differences shown in the student’s drawings are mostly due to the changing (1) distance between Earth and the Moon (2) speed of the Moon in its orbit (3) position of the Moon in its orbit (4) position of the observer on Earth 9. The length of a year is equivalent to the time it takes for one (1) ...
Standard and Essential Question
Standard and Essential Question

... Less direct, meaning the area receives less Energy from the sun ...
Chapter 2 User`s Guide to the Sky
Chapter 2 User`s Guide to the Sky

... The Sun’s gravity is doing the same to Earth. The resulting “wobbling” of Earth’s axis of rotation around the vertical w.r.t. the Ecliptic takes about 26,000 years and is ...
The Milky Way - Computer Science Technology
The Milky Way - Computer Science Technology

... The Sun’s gravity is doing the same to Earth. The resulting “wobbling” of Earth’s axis of rotation around the vertical w.r.t. the Ecliptic takes about 26,000 years and is ...
IS Chapter 14 Notes
IS Chapter 14 Notes

... - is large enough to be made round by its own gravity - has cleared the area of its orbit - 8 in our solar system - Venus is the brightest planet in our night sky at dawn and dusk, second brightest object in the night sky after the moon -planets closest to the sun are seen at sunrise and sunset, pla ...
Sun - Blackboard
Sun - Blackboard

... The Sun’s gravity is doing the same to Earth. The resulting “wobbling” of Earth’s axis of rotation around the vertical w.r.t. the Ecliptic takes about 26,000 years and is ...
Astro 4 Practice Test 1
Astro 4 Practice Test 1

... a. That’s not likely, because the Sun will be in a different place in the sky in about a month. b. Probably not, because it takes the Moon much more than a month to go around the Earth. c. That’s correct, because it takes the Moon about one month to orbit the Earth. d. Probably not, because the Moon ...
Celestial Sphere 2015
Celestial Sphere 2015

... annual path of Sun on the CS ...
E8A1_CRT_CR_MSTIPS_Final
E8A1_CRT_CR_MSTIPS_Final

... for the Northern Hemisphere and away when it is winter. At each of the equinoxes the Earth should not be tilted toward or way from the sun. B. The sun’s rays would be least direct in the winter for the northern hemisphere, and most direct in the southern hemisphere at this same time (The southern he ...
Celestial Sphere 9-23-12
Celestial Sphere 9-23-12

... annual path of Sun on the CS ...
Earth in Space
Earth in Space

... Tides- the rise and fall of ocean water that occurs every 12.5 hours. The water rises for about 6 hours, then falls for about 6 hours. Tides are caused mainly by differences in how much the moon’s gravity pulls on different parts of the Earth. At any one time there are two high tides and two places ...
The cosmological distance ladder
The cosmological distance ladder

... The Cosmological Distance Ladder ...
ASK 8 Science
ASK 8 Science

... The hemisphere that is tilted away from the sun experiences winter. The hemisphere that is tilted toward the sun experiences summer. COMMON MISCONCEPTION: The earth experiences the seasons because it is farther away from the sun in the winter and nearer to the sun in the summer. WHY THIS MUST BE WRO ...
Celestial Equator
Celestial Equator

... While the Sun’s distance from the Earth varies slightly throughout the year, becoming closest on about January 3, it has no noticeable effect on the climate. The effect of the Sun being closer in the northern winter is reduced by the fact that the southern hemisphere has a higher percentage of ocean ...
Solstice vs Equinox
Solstice vs Equinox

... northerly point on the horizon each day. When the sun reaches its extreme northerly point, it rises above the line of latitude known as the Tropic of Cancer (about 23.5° north of the equator). In the northern hemisphere, that day marks the summer solstice, the longest day of the year and the beginni ...
Space Systems: Patterns and Cycles
Space Systems: Patterns and Cycles

... The amount of daylight changes throughout the year. The sun and moon appear to rise in one part of the sky, move across the sky, and set. Stars other than our sun are visible at night but not during the day Comparisons of the amount of daylight in the winter to the amount in the spring or fall. Illu ...
Earth-Mars Interplanetary Transport System Brian Dodson The issue
Earth-Mars Interplanetary Transport System Brian Dodson The issue

... approach is to place the waystation for Earth at the Sun-Earth Lagrange point 1 or 2 (SEL 1 or SEL2), and the Mars waystation at the Sun-Mars Lagrange point 1 or 2 (AML1 or SML2). The Lagrange points in the restricted three-body problem (2 massive bodies, one weightless body) are critical points of ...
HO-04 5a Astro Unit Content
HO-04 5a Astro Unit Content

... Note that except for our sun, the other stars we see at night are all very far outside our solar system. Generally stars other than our sun are visible in the sky only at nighttime. (There are stars in the sky during the daytime as well, but they are not visible because the sun’s light is so much br ...
1) Suppose that a planet was discovered that has twice the mass
1) Suppose that a planet was discovered that has twice the mass

... is the closest planet to the sun. Jupiter is the fifth planet from the sun. Imagine the much more massive Jupiter were to switch places with the less massive Mercury, so that Jupiter became the closest planet to the sun. Which of the following would accurately describe the outcome? A) Jupiter would ...
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Astronomy on Mars



In many cases astronomical phenomena viewed from the planet Mars are the same or similar to those seen from Earth but sometimes (as with the view of Earth as an evening/morning star) they can be quite different. For example, because the atmosphere of Mars does not contain an ozone layer, it is also possible to make UV observations from the surface of Mars.
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