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The Solar System
The Solar System

Solar system
Solar system

Collapse of the Solar Nebula - Indiana University Astronomy
Collapse of the Solar Nebula - Indiana University Astronomy

The Sun: Our Extraordinary Ordinary Star
The Sun: Our Extraordinary Ordinary Star

... • When this material overwhelms the protective Van Allen Belt layer of our atmosphere all electromagnetic activities can be interrupted. – Electronic communication – Electrical Distribution – Satellites ...
Nogami, D. - Subaru Telescope
Nogami, D. - Subaru Telescope

Ch. 4 review
Ch. 4 review

... as they “burned” the hydrogen and helium into carbon, oxygen, neon, calcium, magnesium, silicon, and iron These were then expelled into space by - stellar winds (happening with our sun now) - planetary nebulae (not planets, but similar appearance to early astronomers) - see slides - nova and superno ...
Light: The Cosmic Messenger
Light: The Cosmic Messenger

... our solar system? – Solar nebula spun faster as it contracted because of conservation of angular momentum – Collisions between gas particles then caused the nebula to flatten into a disk – We have observed such disks around newly forming stars ...
Our Star, the Sun
Our Star, the Sun

Powerpoint Presentation (large file)
Powerpoint Presentation (large file)

Last signal sent from RTG
Last signal sent from RTG

... solar system, studying energetic particles from the Sun (solar wind), and cosmic rays entering our portion of the Milky Way. The spacecraft continued to make valuable scientific investigations in the outer regions of the solar system until its science mission ended on March 31, 1997. Since that time ...
Can you write numbers in scientific notation
Can you write numbers in scientific notation

... should be noted that some items from lecture may not be included on this review sheet, but will still be referenced on the exam. As such, use these questions as a reminder of the material that was covered in the lectures while studying from the textbook and the notes you took during lectures. Questi ...
Cosmochemistry from Nanometers to Light- Years A Written by
Cosmochemistry from Nanometers to Light- Years A Written by

... other primitive materials that formed in the solar nebula before the planets formed. We have known for a long time that the CAIs were the oldest solids to form in the solar nebula, but it was not clear if chondrules formed at the same time, or later, and if later, how much later? Age-dating wizards ...
The way things work
The way things work

... Finally, the accumulated stack of 8 GeV antiprotons, plus a new batch of 8 GeV protons from the Booster, are accelerated to 900 GeV by the Main Ring and the superconducting Tevatron working in tandem. ...
Cosmic Rays 3 - zainab
Cosmic Rays 3 - zainab

Lecture10 - Indiana University Astronomy
Lecture10 - Indiana University Astronomy

Origin of the Solar System
Origin of the Solar System

...  The terrestrial planets are relatively small and rocky. In ...
A Planet to Discover - Scholastic New Zealand
A Planet to Discover - Scholastic New Zealand

Exam 3 Solution Set - Indiana University Astronomy
Exam 3 Solution Set - Indiana University Astronomy

... and assume ρ = 1.3 gm cm-3 The value of the mean molecular weight depends on whether the hydrogen is ionized. If not, µ = 1; if so µ = 0.5. Calculate Tc assuming one or the other, and then decide. Or, you could remember that Jupiter might have a metallic hydrogen core, which would not be ionized…. T ...
East Valley Astronomy Club
East Valley Astronomy Club

... If true, the planets formed closer to the Sun, which speeds up their formation, but still not < 10 Myr. However, if the planets formed closer together, the Minimum Mass Solar Nebula must be wrong! The planets were spread out from 5-15 AU, not 5-30 AU. One quarter the area = 4 x denser!! ...
The Sun and Its Solar System Topic 1
The Sun and Its Solar System Topic 1

The Big yellow missing variable in the climate
The Big yellow missing variable in the climate

... Ptolemy’s Tetrabiblos: “It is based also upon their aspects to the planets, when they are at each of the positions of this kind, or likewise others, such as trine and sextile.” ...
Slide 1
Slide 1

From eclipse drawings to the coronagraph and spectroscopy
From eclipse drawings to the coronagraph and spectroscopy

... Continuous corpuscular radiation: solar wind ...
Composition of the Sun
Composition of the Sun

... Some of the particles from a solar flare escape into space, increasing the strength of the solar wind. Particles also escape as coronal mass ejections. The particles in the ejection can cause disturbances to Earth’s magnetic field. These disturbances have been known to interfere with radio commun ...
Chapter 8 Welcome to the Solar System
Chapter 8 Welcome to the Solar System

... • What caused the orderly patterns of motion in our solar system? – Solar nebula spun faster as it contracted because of conservation of angular momentum – Collisions between gas particles then caused the nebula to flatten into a disk – We have observed such disks around newly forming stars ...
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Advanced Composition Explorer



Advanced Composition Explorer (ACE) is a NASA Explorers program Solar and space exploration mission to study matter comprising energetic particles from the solar wind, the interplanetary medium, and other sources. Real-time data from ACE is used by the NOAA Space Weather Prediction Center to improve forecasts and warnings of solar storms. The ACE robotic spacecraft was launched August 25, 1997 and entered a Lissajous orbit close to the L1 Lagrangian point (which lies between the Sun and the Earth at a distance of some 1.5 million km from the latter) on December 12, 1997. The spacecraft is currently operating at that orbit. Because ACE is in a non-Keplerian orbit, and has regular station-keeping maneuvers, the orbital parameters at right are only approximate. The spacecraft is still in generally good condition in 2015, and is projected to have enough fuel to maintain its orbit until 2024. NASA Goddard Space Flight Center managed the development and integration of the ACE spacecraft.
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