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Our Solar System Scavenger Hunt Activity
Our Solar System Scavenger Hunt Activity

... Have a plan for students who finish early. You may want to have an assignment for them to complete when they're done, or you may have them help other students find fact cards. Super Teacher Worksheets - www.superteacherworksheets.com ...
Activity 06 - Total Solar Eclipse 2012
Activity 06 - Total Solar Eclipse 2012

... LUNAR ECLIPSE—The passage of the Moon into the shadow of the Earth, always occurring at a full moon. PATH OF TOTALITY—The path (up to about 270 km wide) that the Moon’s umbral shadow traces on the Earth during a total solar eclipse. TOTAL ECLIPSE—An eclipse during which the umbra touches the Earth ( ...
Geomagnetism and Aeronomy, 2016, Vol. 56, № 7, pp. 1
Geomagnetism and Aeronomy, 2016, Vol. 56, № 7, pp. 1

... Earth-Earth part of the flight (phases 1-2), when the spacecraft orbit lies almost in the ecliptic plane, is called the ecliptic phase. It is designed for formation of the heliocentric trajectory, which will allow to approach Venus, after the gravity assist maneuver with Earth, with the asymptotic s ...
Chapter 2 Universe and Planetary Geology
Chapter 2 Universe and Planetary Geology

... Union (IAU), at a meeting in August 2006, voted on their first "official" definition of a planet. Based on this new definition, Pluto is no longer a planet. According to the IAU's definition, our Solar System has eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. In th ...
Stellar Evolution and the fate of the Solar System
Stellar Evolution and the fate of the Solar System

... YUV420 codec decompressor are needed to see this picture. ...
Diapositiva 1 - Zanichelli online per la scuola
Diapositiva 1 - Zanichelli online per la scuola

... Atmosphere component ...
File
File

... moon like planets and some small asteroids covering around them. Also like planets, their orbits keep them about the same distance from the sun at all times, From the cosmic dust that formed the sun and the planets of our solar system. Along with comets, they’re sort of like the building blocks of t ...
CME - ASU
CME - ASU

... At 0.2 AU, the largest M can produce an acceptable magnetopause at 2* Earth's radius for weak CME, 1* for strong ...
What is our place in the universe?
What is our place in the universe?

... Earth orbits the Sun (revolves) once every year: • at an average distance of 1 AU ≈ 150 million km. • with Earth’s axis tilted by 23.5º (pointing to Polaris) • and rotating in the same direction it orbits, counterclockwise as viewed from above the North Pole. ...
challenger center simulators
challenger center simulators

... Scene 11 (Earth time lapse {old Scene 21}) The last time the sun was where it is now, Earth had but one continent … and dinosaurs roamed the land. Scene 12 (Solar birth {Old Scene 2 – first 43 seconds}) But using supercomputers and through studying other stars, we can travel, as if in a time machine ...
magnetospheres of the outer planets
magnetospheres of the outer planets

... tenuous ionized gas (a plasma), consisting mainly of ...
The Sun: Our Star Attraction
The Sun: Our Star Attraction

... thousands of miles of the sun's material surrounding it. Gravity pulls this material towards the core. The core is made of the lightest and simplest gas, hydrogen. Hydrogen, like all gases, will fit into whatever shape that surrounds them. Gravity of the sun puts pressure on these hydrogen atoms, ma ...
Scaling and the Solar System
Scaling and the Solar System

... room (so that you don't end up too far away with Pluto). If possible, two or more groups can do this part together. Take your time, and let yourself imagine that you are on a journey through an incredibly vast and empty solar system. Once you reach the "end" of your journey, turn around and look for ...
Coronal Mass Ejections and Angular Momentum Loss in Young Stars
Coronal Mass Ejections and Angular Momentum Loss in Young Stars

... space. In Fig. 1, we have also shown representative ranges of X-ray flare energy and prominence mass for two K dwarfs intermediate in age to the TTS sample and the Sun; with an eruptive prominence thought to be the core of a CME, these mass ranges likely represent lower limits on the range of CME ma ...
The edge of the solar system - Beck-Shop
The edge of the solar system - Beck-Shop

... though it was quite close, did not show a detectable disc when viewed through a telescope. This suggested that it was smaller than any of the other known planets. Three similar objects, Pallas, Juno and Vesta, were found in 1802, 1804 and 1807 respectively. All appearing as slowmoving points of ligh ...
IRIS observations of the solar transition region
IRIS observations of the solar transition region

... is also a tendency for the UFS loops to appear to rise with time, as can be seen in ROI 2 (Fig. 1). We find that the UFS loops have a full length of 4 to 12 Mm (106 meters), a maximum height of 1 to 4.5 Mm with an average of 2.5 Mm, and a median intensity in data numbers per second of 40 to 50 DN/s ...
The Moon - DTFizzix
The Moon - DTFizzix

...  The Moon’s orbit is tilted about 5° with respect to the ecliptic plane  It is also tilted with respect to the Earth’s equator – very unlike most of the moons in the solar system which lie almost exactly in their respective central planet’s equatorial plane  The Moon is also very large relative t ...
PLANETARY MAGNETIC FIELDS: SALIENT CHARACTERISTICS
PLANETARY MAGNETIC FIELDS: SALIENT CHARACTERISTICS

... develops in the aft–body portion of solar wind interaction region with the planet. Within this magnetic tail is a field reversal region, the neutral sheet, containing an embedded plasma. The strength of the magnetic field in the magnetic tail of the planets varies, depending upon the condition and d ...
ASR201017 - UCLA IGPP
ASR201017 - UCLA IGPP

... global MHD simulation of the magnetosphere [Walker and Ogino, 1996]. We chose a snapshot 720 min. after the beginning of the run when the IMF was oriented 30 ° dawnward of pure southward (Case 2 in Walker and Ogino, 1996) and a large flux rope contained a combination of closed, open and solar wind f ...
neptune - Robertson County School
neptune - Robertson County School

... than Earth's Moon and has active volcanoes which erupt like geysers and eject nitrogen frost over the surface. Some of the other moons of Neptune are Nereid, Proteus, Larissa, Despina, Galatea, Thalassa, and Naiad. These moons are much smaller than Triton and, except for Nereid, were not discovered ...
SOLAR SYSTEM BRACELET/ANKLET
SOLAR SYSTEM BRACELET/ANKLET

... Comment 1) from Shirley (AESP- Montana) You can use this with any beads (Size E’s are good) and black seed beads. I let the kids choose the beads they want for each planet, but discuss the planet as we are stringing them. This gives the kids ownership in their bracelets, and often as they hear about ...
Solar System: Small Bodies
Solar System: Small Bodies

... Many asteroids, once called minor planets, are chunks of rock with odd shapes. They are too small to have been rounded into spheres by __________. Other asteroids are nickel steel. At least a few other asteroids are cores of dead comets. Main belt asteroids are made of primitive material from the ea ...
The Aurora
The Aurora

... (ISIS-2)” (inizio anni ‘70) ...
The role of the sun in climate forcing
The role of the sun in climate forcing

... amplitude is about 0.1%. This is too small to a!ect signi"cantly the climate. However, there are indications that, on longer time scales, solar variability coluld be much larger. The analysis of cosmogenic nuclides stored in natural archives provides a means to extend our knowledge of solar variabil ...
The Sunspots - Scientific Research Publishing
The Sunspots - Scientific Research Publishing

... Sunspots. A large amount of observational data has been accumulated of the subject [1]; in particular, it is well known that the presence of Sunspots on the solar disk is related to a substantial increase in sun’s activity. The most important expression of that activity is the emission of large quan ...
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Heliosphere



The heliosphere is the bubble-like region of space dominated by the Sun, which extends far beyond the orbit of Pluto. Plasma ""blown"" out from the Sun, known as the solar wind, creates and maintains this bubble against the outside pressure of the interstellar medium, the hydrogen and helium gas that permeates the Milky Way Galaxy. The solar wind flows outward from the Sun until encountering the termination shock, where motion slows abruptly. The Voyager spacecraft have actively explored the outer reaches of the heliosphere, passing through the shock and entering the heliosheath, a transitional region which is in turn bounded by the outermost edge of the heliosphere, called the heliopause. The overall shape of the heliosphere is controlled by the interstellar medium, through which it is traveling, as well as the Sun, and does not appear to be perfectly spherical. The limited data available and unexplored nature of these structures have resulted in many theories.On September 12, 2013, NASA announced that Voyager 1 had exited the heliosphere on August 25, 2012, when it measured a sudden increase in plasma density of about forty times. Because the heliopause marks one boundary between the Sun's solar wind and the rest of the galaxy, a spacecraft such as Voyager 1 which has departed the heliosphere can be said to have reached interstellar space.
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