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society journal - Auckland Astronomical Society
society journal - Auckland Astronomical Society

... The Summer Star Party is our seasonal observing event at the Stardome Observatory. The session will start in the planetarium with a tour of the summer night sky and as it gets dark outside we will move to telescope viewing. The EWB Zeiss Telescope will be available for viewing as well as portable te ...
So, our cosmic address is
So, our cosmic address is

... Where in the Universe is the Milky Way Galaxy? ...
The basics - Front Page Science
The basics - Front Page Science

... not always at the same distance from the Sun and the Moon is not always the same distance from Earth. The Earth-Sun distance varies by 3 percent and the MoonEarth distance by 12 percent. The result is that the Moon’s apparent diameter can range from 7 percent larger to 10 percent smaller than the Su ...
SWFAS August 16 Newsletter - Southwest Florida Astronomical
SWFAS August 16 Newsletter - Southwest Florida Astronomical

... Juno will plunge closer to the Jovian cloud tops than any mission before, passing just 4,200 km (2,600 miles) away over the course of 36 orbits. Its instruments will also examine Jupiter's polar regions close up on each successive close pass, another first. ...
Chapter 16 - Follow “Ironmtn.wordpress.com”
Chapter 16 - Follow “Ironmtn.wordpress.com”

... including Pathfinder (1990s) and Odyssey (2002). A Martian atmosphere was also possible in the past. These are the two prerequisites for formation of life. Link To: Exploring the Solar System Difficulty Level: Hard ...
Astronomer Notes PowerPoint
Astronomer Notes PowerPoint

... how much would he weigh on the moon if the surface gravity is 17% of that on Earth? Weight=mass x gravitational acceleration Or weight = weight on earth x specific gravity Now see if you can figure it out W= 100 lbs x .17=17 lbs. ...
Chapter 13 - KFUPM Faculty List
Chapter 13 - KFUPM Faculty List

... Q19 Four equal masses, 2.0 kg each, are placed at the four corners of a square of side 10 cm as shown in Fig 7. What is the magnitude of the gravitational force on one of the masses due to the other three? A1 5.1 * 10**-8 N Q20 The escape speed from a certain planet for an empty spaceship of mass M ...
Ch#13 - KFUPM Faculty List
Ch#13 - KFUPM Faculty List

... Q19 Four equal masses, 2.0 kg each, are placed at the four corners of a square of side 10 cm as shown in Fig 7. What is the magnitude of the gravitational force on one of the masses due to the other three? A1 5.1 * 10**-8 N Q20 The escape speed from a certain planet for an empty spaceship of mass M ...
General - Friends of APOD
General - Friends of APOD

... Explanation: What would it be like to see a sunset on Mars? To help find out, the robotic rover Spirit was deployed in 2005 to park and watch the Sun dip serenely below the distant lip of Gusev crater. Colors in the above image have been slightly exaggerated but would likely be apparent to a human e ...
MySci Unit 23
MySci Unit 23

... A. The Earth, Sun, and Moon are part of a larger system that includes other planets and smaller celestial bodies a. Observe and identify the Earth is one of several planets within a solar system that orbits the Sun b. Observe and identify the Moon orbits the Earth in about a month Identify that plan ...
Exploring the Solar System Jeopardy!
Exploring the Solar System Jeopardy!

... Planets & Pluto: 500 Name the eight planets in order by increasing distance from the sun (closest to furthest). ...
So What All Is Out There, Anyway?
So What All Is Out There, Anyway?

... Eventually you become big enough that you can look down and see all the planets of the solar system—Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto—orbiting the Sun. Pluto is about 3.5 billion miles away from the Sun. Light from our Sun takes over 5 hours to reach Pluto. Tha ...
Index to issues
Index to issues

... 12 - A Proposal for a daytime Astronomy Course for the US (solar and non-visible-spectrum based course) 11 - A Way To Know Just What Introductory Astronomy Students Are Interested In ((Using APOD), in Astronomical Teachniques) 11 - Would You Like a Homemade Dome With That Toy Planetarium? (in Astron ...
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... elevator (a) accelerates downward, (b) accelerates upward, (c) is in free fall, (d) moves upward at constant speed? In which case would your weight be the least? When would it be the same as when you are on the ground? ...
teacher resource - Michigan Science Center
teacher resource - Michigan Science Center

... There are six areas: the core, the radiative zone, the convective zone, the photosphere, the chromosphere, and the corona. The photosphere or surface of the sun is a 500 kilometer thick region from which most of the Sun’s radiation escapes outward and is detected as the sunlight we see. Eventually o ...
Supplemental Educational Support Materials
Supplemental Educational Support Materials

... You might think that astronomers still would have discovered Xena because it is slightly larger than Pluto. This answer is incorrect. Xena is small and far away from Earth. Astronomers spotted Xena because it reflects lots of light. Xena is so far away that, if it did not reflect as much light as it ...
The astronauts in the upper left of this photo are working on the
The astronauts in the upper left of this photo are working on the

... the elevator (a) accelerates downward, (b) accelerates upward, (c) is in free fall, (d) moves upward at constant speed? In which case would your weight be the least? When would it be the same as when you are on the ground? ...
Lecture 25: The Outer Planets
Lecture 25: The Outer Planets

... the core of each planet, and are probably produced in the metallic hydrogen layers •The magnetic fields on Neptune and Uranus are quite offset from the core of each planet, and display very large tilt angles ...
4. The Solar System
4. The Solar System

... – Earth and Mars rotate at about the same rate; Venus and Mercury are much slower, and Venus rotates in the opposite direction. – Earth and Mars have moons; Mercury and Venus don’t. – Earth and Mercury have magnetic fields; Venus and Mars don’t. © 2017 Pearson Education, Inc. ...
Habitable Planets Webquest
Habitable Planets Webquest

... Step 7: Search “Bad Universe Goldilocks Zone” (should be the first video) or open this link: http://science.howstuffworks.com/44484-bad-universe-goldilocks-zone-video.htm and answer this question: 1. What happens to the “planet” as it’s moved around the solar system? Step 8 : Search “What Makes a Pl ...
ptolemy day 21 - Arts of Liberty
ptolemy day 21 - Arts of Liberty

... Jupiter, Saturn, can be any angular distance from the sun. This is the big distinction between inner and outer planets. (The cause of this, in truth, is clear. Our own orbit encompasses those of Venus and Mercury, while it is encompassed by those of Mars, Jupiter, and Saturn. This is another sneak p ...
Sky Diary - Society for Popular Astronomy
Sky Diary - Society for Popular Astronomy

... Sun means that they too are lost to detailed night time observation but, Saturn in particular, may be found and observed in daylight as long as sensible precautions are taken to ensure the Sun can never enter the field of view of either the telescope or the finder-scope. Jupiter is just too close to ...
Page 1 of 13 View Edit Map 12/4/2007 http://mapster.gstboces.org
Page 1 of 13 View Edit Map 12/4/2007 http://mapster.gstboces.org

... lithospheric plate, mid-ocean ridge, ocean trench, plastic, plate tectonics, polarity, subduction, transform boundary, tsunami, volcano ...
C - ScienceWilmeth5
C - ScienceWilmeth5

... Third Quarter ...
Saturn
Saturn

... 9. Ring material may come from ripped up moons. The point where the gravitational pull of Saturn equals the structural integrity of the moon itself is the _______________ _________________. This is also called the tidal stability limit. Page 310 10. The largest gap in the rings is called the _______ ...
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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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