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Earth, Sun, Moon System
Earth, Sun, Moon System

... Something Special: Is there anything special about your planet? This can often be the best part of the report, taking you off on interesting topics. For example, are there 100-year-long storms on your planet? Are there giant volcanoes? Does your planet have a very tilted axis (giving it extreme seas ...
Earth in Space - Learning Outcomes
Earth in Space - Learning Outcomes

... When the Apollo 11 satellite took the first men to the Moon in 1969 its trajectory was very closely monitored. The satellite had a velocity of 5374 m s-1 when 26306 km from the centre of the Earth and this had dropped to 3560 m s-1 when it was 54368 km from the centre of the Earth. The rocket motors ...
1 Marsbugs: The Electronic Astrobiology Newsletter, Volume 12
1 Marsbugs: The Electronic Astrobiology Newsletter, Volume 12

... is between 2 and 4 percent methane—going from the middle, coldest part of the atmosphere, the tropopause, down to the surface. And that means there is abundant organic chemistry going on, powered primarily in the upper atmosphere by ultraviolet light from the sun. There may be additional chemistry o ...
Note Packet
Note Packet

... slightly bigger than the polar circumference. (bulges at the equator) This difference is small and can not be seen with the naked eye. Proof that the earth is round: -Ships appear to sink GRADUALLY below the horizon as they travel away from observer -Polaris (North Star) changes altitude (angle meas ...
The Universe - HMXEarthScience
The Universe - HMXEarthScience

... C) longer than normal (a red shift) D) longer than normal (a blue shift) 16. In a Doppler red shift, the observed wavelengths of light from distant celestial objects appear closer to the red end of the spectrum than light from similar nearby celestial objects. The explanation for the red shift is th ...
005 Astrophysics problems
005 Astrophysics problems

... When the Apollo 11 satellite took the first men to the Moon in 1969 its trajectory was very closely monitored. The satellite had a velocity of 5374 m s-1 when 26306 km from the centre of the Earth and this had dropped to 3560 m s-1 when it was 54368 km from the centre of the Earth. The rocket motors ...
Document
Document

... making in the 16th century, a north-south line through Greenwich became the world standard for measurements of longitude. Today, the Greenwich meridian, also known as the prime meridian, has become the reference line from which longitude is measured, as you can see in Figure 2-7. Lines of equal long ...
Atmospheric biomarkers on terrestrial exoplanets Abstract Introduction
Atmospheric biomarkers on terrestrial exoplanets Abstract Introduction

... by ancient Greek philosophers, has been proved only very recently, first around pulsars (Wolszczan & Frail 1992), then around solar type stars (Mayor & Queloz 1995). In the latter case, the planets discovered are giant planets (of the order of Jupiter’s mass) and likely to be gaseous, which proved t ...
Planets, Moons, and Stars
Planets, Moons, and Stars

... of its lighted side. The Sun shines on and lights half of the Moon’s surface. The other half faces away from the Sun. It is in darkness. As the Moon revolves around Earth, different amounts of the Moon’s lighted half face Earth. The lighted parts are the phases you see. When the Moon is between Eart ...
The Color of Plants on Other Worlds
The Color of Plants on Other Worlds

... advanced civilizations, but we can look for the physical and chemical signs of fundamental life processes: “biosignatures.” Beyond the solar system, astronomers have discovered more than 200 worlds orbiting other stars, socalled extrasolar planets. Although we have not been able to tell whether thes ...
Astronews - Hawaiian Astronomical Society
Astronews - Hawaiian Astronomical Society

... so far have matched the greatest expectations for what we would see. Pluto and Charon are dynamic worlds with varied landscapes and some relatively recent, perhaps even ongoing, geologic activity. There are mountain ranges several thousand feet high and large expanses of terrain with no visible crat ...
Circumstellar Disks: the Formation and Evolution of
Circumstellar Disks: the Formation and Evolution of

... • Sub-blow out sized dust grains will be subject to radiation pressure (infrared imaging) • Largest grains may be trapped in resonances (submm/mm imaging) • Intermediate-sized grains may be at similar distances as larger grains but not physically trapped in resonances (far-infrared imaging) ...
eratoshenes_earth_measurement
eratoshenes_earth_measurement

... Eratosthenes to go to Alexandria as the tutor of his son Philopator. On the death of Callimachus in about 240 BC, Eratosthenes became the third librarian at Alexandria, in the library in a temple of the Muses called the Mouseion. The library is said to have contained hundreds of thousands of papyrus ...
Earth Chakras - Astrogeographia
Earth Chakras - Astrogeographia

... Rudolf Steiner considered Southeast Asia separately from the rest of Asia, bringing the number back to seven. Southeast Asia he correlated with Venus, and the rest of Asia—at least, that part of Asia comprising the natural habitat of the “Mongolian peoples”—he brought into connection with Mars. Thu ...
The Sun: A Model Star
The Sun: A Model Star

... electrons) which flow outwards from the coronal holes. The wind speed is high (800 km/s) over coronal holes and low (300 km/s) over streamers. These high and low speed streams interact with each other and alternately pass by the Earth as the Sun rotates. ...
ph507-16-6sun
ph507-16-6sun

... electrons) which flow outwards from the coronal holes. The wind speed is high (800 km/s) over coronal holes and low (300 km/s) over streamers. These high and low speed streams interact with each other and alternately pass by the Earth as the Sun rotates. ...
newsletter - Thanet Astronomy Group
newsletter - Thanet Astronomy Group

... About the Cover Picture From time to time, and not very often, various groups of planets will, of course, group together or 'align' around one particular direction from the Sun. When this happens if the alignment is in a direction visible from the side of the Earth that faces away from the Sun, the ...
A-level Physics A Question paper Unit 05 - Section 2A
A-level Physics A Question paper Unit 05 - Section 2A

... Analysis of the spectrum of one of the stars shows a periodic variation in wavelength. Figure 2 shows the results for one of the spectral lines in the Hydrogen Balmer series. The wavelength for this line as measured for a source in a laboratory on the Earth is 656.28 nm. Figure 2 ...
ES 104 Midterm Exam Study Guide 1
ES 104 Midterm Exam Study Guide 1

... Know how the craters and the maria on Earth’s moon were formed. Jovian planets versus the Terrestrial planets – be familiar with the physical and compositional differences between these 2 categories of planets – look over the table that you completed for the first homework activity. Also know why th ...
Physivd Preliminary Module 8.5 The Cosmic Engine
Physivd Preliminary Module 8.5 The Cosmic Engine

...  Describe how the ozone layer forms.  Explain how the ozone layer protects the surface of the Earth from UV  Describe how some chemicals such as CFCs destroy ozone, forming ozone “holes” in the ozone layer.  Explain how some gases such as water, carbon dioxide and methane trap/reflect heat escap ...
TLW design a model that describes the position and relationship of
TLW design a model that describes the position and relationship of

... dwarf planets, plutoids, comets and asteroids orbit the Sun. Moons orbit the planets. There are currently eight planets and three or four (depending on the source) identified plutoids and dwarf planets in our solar system. Dwarf planets and plutoids are smaller, orbit the Sun, have enough mass and g ...
Earth Science pacing guide
Earth Science pacing guide

...  shape and size of Planet Earth  gravity, inertia, and orbits  characteristics of electromagnetic radiation  axial tilt of Earth’s rotation Students will understand…  the positions of the Earth, Moon, and Sun and how they move through space  the effects of the movement of Earth, Moon and Sun; ...
September 2016
September 2016

... side has almost no Maria (seas) but does have an enormous multi ringed crater that looks like an eye. It is interesting to wonder what our ancestors would have made of this ‘eye’ like feature looking down from the sky if it had been on the near side. Observing the phases of the Moon does not need an ...
File
File

... each asteroid in the asteroid belt D) calculations of the temperature and luminosity of stars ...
Measuring the Size of the Astronomical Unit (AU)
Measuring the Size of the Astronomical Unit (AU)

... Measuring the Size of the Astronomical Unit (AU) SYNOPSIS: In this lab, you will estimate the size of the orbits of Venus and Mercury, and measure the distance that the Earth is from the Sun. You will also be able to derive the size of the Sun, and the size of Venus as part of the exercise. EQUIPMEN ...
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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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