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The Seasons Interactive - Home
The Seasons Interactive - Home

... explains why eclipses of the sun and moon do not happen every month. With this tilt of the moon’s orbit, five out of six times (on average) the moon’s shadow passes above or below the plane of the earth’s orbit. Likewise, the moon, on the anti-solar end of its orbit, passes below the earth’s shadow ...
(the largest solar system planet) represents at
(the largest solar system planet) represents at

... The Solar System The solar system consists of a main sequence star (the sun), four terrestrial planets (Mercury, Venus, Earth, Mars), four outer planets (Jupiter, Saturn, Uranus, Neptune), approximately three “dwarf planets,” more than 130 satellites (orbiting moons), an asteroid belt, and entering ...
Time - Academic Computer Center
Time - Academic Computer Center

... • In reality because the Earth rotates on its axis from West to East the Sun, Moon and stars all appear to move from East to West. • The Sun appears to rise in the East and set in the West because the Earth spins. • The Moon however also orbits the Earth traveling from West to East but it takes much ...
MCSD Grade 4 Science Quarterly Assessment
MCSD Grade 4 Science Quarterly Assessment

... d. many new stars, but no dust or gas ____ 11. Which of these describes a sphere of hot gases that gives off its own light and heat? a. star b. planet c. galaxy d. asteroid ____ 12. During a trip to a planetarium, Greg learned that the outer planets are Jupiter, Saturn, Uranus, and Neptune. ...
Lec4_2D
Lec4_2D

... on the composition of a body, just its mass and distance. The Moon exerts a force on the Earth, but since the Earth has a finite size, this force is different from one side of the Earth to the other. The side of the Earth near the Moon gets pulled most, the center of the Earth less, and the backside ...
space tech - Project Jugaad
space tech - Project Jugaad

... your two eyes are separated by a few inches, each views your thumb from a different position. The amount that your thumb appears to move is its parallax. When astronomers measure the parallax of an object and know the separation between the two positions from which it is observed, they can calculate ...
AST111, Lecture 1b
AST111, Lecture 1b

... • Actual sizes can be estimated from angular sizes once the distance to an object has been estimated from its orbit. Remember that Kepler’s third law relates the orbit period to it semi-major axis. However, angular resolution from most earth ground based observations is limited by atmospheric seeing ...
Lecture 2 - Lines in the Sky
Lecture 2 - Lines in the Sky

... • In order to use the sky to measure time you need to measure the location of objects in the sky. We will look at two methods of measuring locations in the sky. • Both methods require measuring angles. • These methods have long been used not only for timekeeping but for navigation as well. • But fir ...
Voyage: A Journey Through Our Solar System Grades K
Voyage: A Journey Through Our Solar System Grades K

... The total area of Mars’s surface is about the same as all the dry land on Earth. Why does Mars appear red? Mars’ surface contains iron oxide, also known as rust, which gives it its red color. Between which planets is the asteroid belt? Mars and Jupiter. If you wanted to tie a ribbon around Ceres, th ...
Astronomy 111 Overview of the Solar system
Astronomy 111 Overview of the Solar system

... on meteorites, nearly all of which originate in the asteroid belt. We will study this in great detail: ❑ When rocks melt, the contents homogenize pretty thoroughly. ❑ When they cool off, they usually recrystallize into a mixture of several minerals. Each different mineral will incorporate a certain ...
new mercury - stmarysroom52010
new mercury - stmarysroom52010

... 2010 and 2012; the mission will consist of two identical orbiters and for the first time possibly a launcher. ...
Lecture 1: Our Place in Space
Lecture 1: Our Place in Space

... Lecture Series 1: Earth’s Movement & Lunar • The Moon has phases or changes in appearance during the night sky because of how the light from the Sun reflects off the Moon as it rotates around the Earth. • New Moon, Full Moon, etc. ...
the copernican revolution - University of Florida Astronomy
the copernican revolution - University of Florida Astronomy

... Sun.that revolve about the Sun. 4.  The stars are very much farther away than the •!HSun. e placed the planets in the correct order: Mercury, Venus, Earth, Mars, Jupiter, and Saturn. 5.  The apparent movement of the stars around the •!The nearer a planet is to the Sun, the greater its orbital speed. ...
Document
Document

... piece of matter in space that is visible when it falls into Earth’s atmosphere. Background source: 1Wyrmshadow1 website ...
Physics-Y11-LP2 - All Saints` Catholic High School
Physics-Y11-LP2 - All Saints` Catholic High School

... Earth round the Sun H: explain why a sidereal day, a rotation of 360° of the Earth, is different from a solar day due to the orbital movement of the Earth and that a sidereal day is 4 minutes less than a solar day LP2/2 explain that the positions of astronomical objects are measured in terms of two ...
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 ...
`It`s Raining, It`s Pouring`
`It`s Raining, It`s Pouring`

... they are named very similarly, there are very few similarities between the super-Earths and the Earth that we know. There are stark contrasts between the two, with the super-Earth having a considerably denser atmosphere and icy surface, although both surfaces are of a solid consistency. It is also s ...
Precession of the Earth`s Axis
Precession of the Earth`s Axis

... around 130 BC, adding his own observation to those of Babylonian and Chaldean astronomers in the preceding centuries. In particular they measured the distance of the stars like Spica to the Moon and Sun at the time of lunar eclipses, and because he could compute the distance of the Moon and Sun from ...
Universe Notes - Solon City Schools
Universe Notes - Solon City Schools

... diagram are known as supergiants i. Very large (100 to 1000 times the diameter of the sun) b. Just below the supergiants are the giants c. Below the main sequence are the white dwarfs, which are the small, dense remains of a low- or mediummass star ...
The Celestial Sphere
The Celestial Sphere

... Partial Solar Eclipse ...
Document
Document

... 9. Why did the model of the universe proposed by Copernicus gain support soon after its publication? a. It more accurately predicted the position of planets. b. It gave a better explanation for the phases of the Moon. c. It was a more elegant explanation of retrograde motion. d. The old system of Pt ...
time astro 2014 - Fort Thomas Independent Schools
time astro 2014 - Fort Thomas Independent Schools

...  What if everyone kept the same time…then 12 midnight for some would be dark and for others it would be light.  What led to the development of time zones?  Synchronization of human activities over long distances led to the standardization of local times.  How were the time zones determined?  It ...
Lecture11 - UCSB Physics
Lecture11 - UCSB Physics

... This highly magnified image shows a microscopic dust grain that came from interplanetary space. It entered Earth’s upper atmosphere and was collected by a high-flying aircraft. Dust grains of this sort are abundant in star-forming regions like the Orion nebula. These tiny grains were also abundant i ...
Astrophysics - Student Reference Packet
Astrophysics - Student Reference Packet

... passage, more than 300 scientists signed a petition stating that they did not agree with the IAU's definition of a planet and that a better definition was needed. As of 2006, the debate is not over. The definition put in place by the members of the IAU who voted (only about 5 percent of the world's ...
T 4
T 4

... • The outer edge of the HZ is the distance from the Sun at which even a strong greenhouse effect would not allow liquid water on the planetary surface. • Carbonate-silicate cycle can help to extend the outer edge of the HZ by accumulating more CO2 and partially offsetting low solar luminosity. ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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