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Frequency Analysis
Frequency Analysis

...  The orbital dynamics of NEAs is chaotic and in individual cases unpredictable on time scales >1000 years.  There are a number of useful tools that help us to deal with chaos such as Lyapunov exponents, surfaces of section, and frequency analysis.  Future evolution of a NEA can be described stati ...
August
August

... M13 At a distance of 25,100 light years, this globular cluster in the constellation Hercules (HER-cueleez) is about 145 light years in diameter. The age of M13 has been estimated at over 10 billion years. It contains over 300,000 stars. At the center, stars are about 500 times more concentrated than ...
Comets and the Solar System Practical Astronomy: 16 September
Comets and the Solar System Practical Astronomy: 16 September

... Near maximum evening elongation NOW Max on 22nd September About 15-18 degrees up at 7pm Phases like Venus Very small disk (6 arcsrc) but the phase is visible if the atmosphere is steady enough • Conjunction with Spica 20 & 21 Sept ...
Comets and the Solar System Practical Astronomy: 16 September
Comets and the Solar System Practical Astronomy: 16 September

... Near maximum evening elongation NOW Max on 22nd September About 15-18 degrees up at 7pm Phases like Venus Very small disk (6 arcsrc) but the phase is visible if the atmosphere is steady enough • Conjunction with Spica 20 & 21 Sept ...
Today`s Powerpoint
Today`s Powerpoint

... The proton and electron each have “spin”. A result from quantum mechanics: if both spinning the same way, atom's energy is slightly higher. Eventually will make transition to state of opposite spins. Energy difference is small -> radio photon emitted, wavelength 21-cm. ...
DEEP IMPACT and ROSETTA
DEEP IMPACT and ROSETTA

... • Ices of supervolatiles (CO, CO2, CH4)  comets were deeply frozen over their whole lifetime  formation region = outer planetary disk (Jupiter and beyond)  supervolatiles (& ortho-para ratio of H2O and others) are T tracers of evolution history of comets back to formation era • Small in size (m – ...
Toys Watch the Sky
Toys Watch the Sky

... The Sun appears to move from east to west due to the rotation of the Earth in the opposite direction (west to east). The time of day at which shadows are shortest is the time when the Sun is due north, so the shortest shadow points in a north-south direction. Some children may find it hard to believ ...
Voyage of Discovery - MESSENGER Education
Voyage of Discovery - MESSENGER Education

... of the planets, asteroids, comets, and small icy bodies beyond Neptune. The Solar System is truly the family of the Sun. The planets, asteroids, and comets orbit the Sun, while the moons orbit their parent planets. The Sun’s central role derives from its high mass; it has 99.8% of the mass in the So ...
KEPLER: Search for Earth-Size Planets in the Habitable Zone
KEPLER: Search for Earth-Size Planets in the Habitable Zone

... those locations where giant planets are commonly found: 0.05, 0.1, 0.2, 0.4, 0.6, 0.8. 1.0, 12., & 1.5 AU. When the position of the HZ is near any of the latter positions, the model assumes that the probability of a planet at that position is zero. To illustrate the capability of the instrument to r ...
The Association of Lunar and Planetary Observers Solar System
The Association of Lunar and Planetary Observers Solar System

... of individuals that study the sun, moon, planets, asteroids, meteors, and comets and other topics of study that relate to Solar System astronomy. ...
03_Testbank - Lick Observatory
03_Testbank - Lick Observatory

... 35) Kepler's third law, p2 = a3, means that A) a planet's period does not depend on the eccentricity of its orbit. B) all orbits with the same semimajor axis have the same period. C) the period of a planet does not depend on its mass. D) planets that are farther from the Sun move at slower average ...
Deep Space Mystery Note Form 2
Deep Space Mystery Note Form 2

... expanding gases to glow briefly and brightly. During this short interval, a supernova can radiate as much energy as our Sun could emit over its life span. The explosion expels much or all of the star’s material and causes a shock wave into the surrounding interstellar medium. The interstellar medium ...
Binary star formation
Binary star formation

... • Wide range of scales involved in different binaries Possible mechanisms that have been suggested: • Fission - one star splits into two • Capture - one star captures another initially unbound star into a bound orbit • Cloud fragmentation - collapsing cloud breaks up into several pieces during colla ...
d Kepler Telescope Lies from NASA The Claims "NASA`s Kepler
d Kepler Telescope Lies from NASA The Claims "NASA`s Kepler

... "Kepler, a space telescope, looks for planet signatures [How?] by measuring tiny decreases in the brightness of stars caused by planets crossing in front of them [the stars]. They see nothing... This is known as a transit." It's "…like looking at a headlight at a great distance and trying to sense t ...
Lecture 8 - Kepler and Brahe
Lecture 8 - Kepler and Brahe

... that this is a voluntary choice based on his attitude. He refused to add epicycles. But now, of course, he had no model of the motions of the planets. Kepler realized that to get the most out of Tycho’s data, he first needed to determine the Earth’s orbit, since all planetary observations are made f ...
Exploring_Gravity_ LessonPlan
Exploring_Gravity_ LessonPlan

... Our Solar System began to form about 4.6 billion years ago from a swirling cloud of gas and dust. It is made up of the Sun, the planets, their moons, asteroids and comets. Gravity is a force that attracts objects to each other. All things exert some gravitational force but the more mass an object ha ...
Worcester Public Schools
Worcester Public Schools

... 1. After looking at your solar system line graphs, what patterns can you identify in each? 1) Mass of a planet increases with distance from the sun. 2) Radius of a planet increases with distance from the sun. 3) Density generally decreases with distance from the sun. 2. What planets can be grouped i ...
Slide 1
Slide 1

... there differences? Report out two Tier 2 words that are most likely to cause student confusion or misunderstanding ...
Comins Chapter 8 - The Outer Planets
Comins Chapter 8 - The Outer Planets

... surrounded by a thick layer of liquid metallic hydrogen and an outer layer of ordinary liquid hydrogen. Both planets have an overall chemical composition very similar to that of the Sun. The visible features of Jupiter exist in the outermost 100 km of its atmosphere. Saturn has similar features, but ...
Outline2a
Outline2a

... As the gas cloud collapses, the protostar gets smaller and smaller (and, due to the increased central pressure), hotter and hotter. Accretion will cause the mass of the protostar to increase more than 100 times. The star will move towards its place on the ...
Star in a Box
Star in a Box

... The luminosity of a star is powered by nuclear fusion taking place in the centre of the star converting hydrogen into helium. – The temperature and density must be high enough to allow nuclear fusion to occur. – Stars are primarily composed of hydrogen, with small amounts of helium. ...
DTU 8e Lecture PPT Chap 1 Discovering the Night Sky v2
DTU 8e Lecture PPT Chap 1 Discovering the Night Sky v2

... north polar region (ignoring Earth’s orbit around Earth-Moon barycenter). For the Moon to keep the same side facing Earth as it orbits our planet, the Moon must rotate on its axis at precisely the same rate that it revolves around Earth. ...
Exam 2
Exam 2

... structures. This diversity holds clues about stellar evolution and about numerous ways in which stars interact with their environments. For example, some of the heavy elements (such as carbon, nitrogen and oxygen) that form in a star’s core move into its outer layers. The abundance of these elements ...
April 10th
April 10th

... • Hot core ionizes the escaping atmosphere • Colors come from a mix of emission lines such as oxygen (green), nitrogen (red), and hydrogen ...
1. The planetary winds in Earth`s Northern Hemisphere generally
1. The planetary winds in Earth`s Northern Hemisphere generally

... Northern Hemisphere’s winter. During which season in the Northern Hemisphere is Earth’s orbital velocity greatest? (1) winter (3) summer (2) spring (4) fall 10. Terrestrial planets move more rapidly in their orbits than the Jovian planets because terrestrial planets are (1) rotating on a tilted axis ...
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History of Solar System formation and evolution hypotheses



Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a ""Solar System"", simply because almost no one knew or believed that the Solar System, in the sense we now understand it, existed. The first step towards a theory of Solar System formation was the general acceptance of heliocentrism, the model which placed the Sun at the centre of the system and the Earth in orbit around it. This conception had been gestating for thousands of years, but was only widely accepted by the end of the 17th century. The first recorded use of the term ""Solar System"" dates from 1704.
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