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Asteroids and Meteorites
Asteroids and Meteorites

... 3: corresponds to the distance of Ceres, discovered in 1801 by Piazzi. 6: corresponds to Uranus 7: a=40 AU, Neptune is at 30 AU ...
The mass of the Moon is 1/81 of the mass of the Earth. Compared to
The mass of the Moon is 1/81 of the mass of the Earth. Compared to

... A planet (P) is moving around the Sun (S) in an elliptical orbit. As the planet moves from aphelion to perihelion, the Sun’s gravitational force A. does positive work on the planet. B. does negative work on the planet. C. does positive work on the planet during part of the motion and negative work d ...
Jupiter`s Galilean Moons
Jupiter`s Galilean Moons

... Again, with the exception of Callisto, all the cores are surrounded by rock (shown in brown) shells. Io’s rock or silicate shell extends to the surface, while the rock layers of Ganymede and Europa (drawn to correct relative scale) are in turn surrounded by shells of water in ice or liquid form (sho ...
speed
speed

... Compared to the Earth, Planet X has twice the mass and twice the radius. This means that compared to the amount of energy required to move an object from the Earth’s surface to infinity, the amount of energy required to move that same object from Planet X’s surface to infinity is A. 4 times as much. ...
space tech - Project Jugaad
space tech - Project Jugaad

Existence of collisional trajectories of Mercury, Mars and Venus with
Existence of collisional trajectories of Mercury, Mars and Venus with

... enough to allow collision with Venus within 5 Gyr (refs 1–3). This conclusion, however, was established either with averaged equations1,2 that are not appropriate near the collisions or with nonrelativistic models in which the resonance effect is greatly enhanced by a decrease of the perihelion velo ...
The mass of the Moon is 1/81 of the mass of the Earth. Compared to
The mass of the Moon is 1/81 of the mass of the Earth. Compared to

... Compared to the Earth, Planet X has twice the mass and twice the radius. This means that compared to the amount of energy required to move an object from the Earth’s surface to infinity, the amount of energy required to move that same object from Planet X’s surface to infinity is A. 4 times as much. ...
Tidal forces in the Solar System
Tidal forces in the Solar System

Document
Document

...  ratio of Type I & II migration may be less than previously thought (Winn et al. 2010)  one cannot distinguish between p-p scattering and Kozai migration by spin-orbit misalignments or eccentricities alone  Need to search for counterparts of migration processes  very long term radial velocity me ...
Formation of Stars
Formation of Stars

... density of each clump rises. Eventually the cloud core becomes opaque to UV and optical radiation. At the end of stage 2, the fragments are ~100 times the size of the solar system.  Stage 3: The cloud fragment develops a hot core - from 100 K to 104 K. The gas density increases much faster in the c ...
Astrology
Astrology

... couples marrying or 500 divorcing. • Choice of profession: No correlation with Sun sign for 6000 politicians or 17,000 scientists • Horoscope of mass murderer sent to 150 people. 94% said it described them well. • 3000 specific predictions about celebrities: – 10% correct, 90% incorrect ...
Astrology
Astrology

... •  Sun sign compatibility? No correlation with 3000 couples marrying or 500 divorcing. •  Choice of profession: No correlation with Sun sign for 6000 politicians or 17,000 scientists •  Horoscope of mass murderer sent to 150 people. 94% said it described them well. •  3000 specific predictions about ...
Astrology
Astrology

... • Sun sign compatibility? No correlation with 3000 couples marrying or 500 divorcing. • Choice of profession: No correlation with Sun sign for 6000 politicians or 17,000 scientists • Horoscope of mass murderer sent to 150 people. 94% said it described them well. • 3000 specific predictions about cel ...
The Jovian Planets
The Jovian Planets

... did not know how large Jupiter was when they first named it.  Jupiter is 10 times the size of Earth and 300 times in mass ...
Lunar Eclipse
Lunar Eclipse

... Tides Basics: Tides: -The moon pulls on everything on Earth. -since water is fluid, the Earth cannot hold onto it and the moon is able to pull on it. -This creates two tides per day. ...
Lecture 13: The stars are suns
Lecture 13: The stars are suns

... Stars are fusion reactors like our sun, with similar physical properties. Spectroscopes, atomic theory, and especially measurements of stellar distances (1838) made it possible for astronomers to derive properties of stars and establish the Sun-stellar connection. • Physical properties of stars we w ...
The Jovian Planets
The Jovian Planets

... did not know how large Jupiter was when they first named it.  Jupiter is 10 times the size of Earth and 300 times in mass ...
Powerpoint slides - Earth & Planetary Sciences
Powerpoint slides - Earth & Planetary Sciences

... ultimate source – Kuiper Belt • Pluto’s current orbit is probably due to perturbations by Neptune as N moved outwards (recall the 3:2 resonance) • Charon is most likely the result of a collision. Clues: – Its orbital inclination (and Pluto’s rotation) strongly suggest an impact (c.f. Neptune) – The ...
Last time: looked at proton-proton chain to convert Hydrogen into
Last time: looked at proton-proton chain to convert Hydrogen into

... Young stars which are still accreting material are called T-Tauri Stars. Because mass is piling on, they sometimes have explosive outbursts. ...
life
life

... Number of communicating civilisations = rate of formation of suitable stars  x fraction of these stars with planets  x number of Earth-like planets per system  x fraction of such planets which develop life  x fraction of life-bearing planets evolving intelligence x fraction of intelligent specie ...
99942 Apophis Asteroid - Lawrencehallofscience
99942 Apophis Asteroid - Lawrencehallofscience

... How close will the asteroid get to Earth? To calculate this, we need two of the orbital elements: a, the semi-major axis of the ellipse, which measures how far away the asteroid is from the Sun on average (for a perfect circle, the semi-major axis is equal to the radius), and e, the eccentricity, wh ...
1 Sun Stars Planets. Problem Sheet I
1 Sun Stars Planets. Problem Sheet I

... (b) The measured speeds of convection in granular cells at the surface of the sun are about 2 km/s and the photospheric density is of order 10-3 kg m-3 . A magnetic field of strength B will be able to alter the motion of a plasma in which it is embedded when the magnetic energy density B2 /2 µo is g ...
ppt
ppt

... resembles each other in mass and size more than any other planet-satellite pair in the solar system. • The distance is also the smallest, 19,640 km • Charon’s orbit period is the same as its rotational period, and also the same as the Pluto’s rotation period (6.3 days) – Both keep the same face towa ...
Five Planets
Five Planets

... named Cassini is traveling to Saturn now. It will arrive in July. There are no people onboard Cassini; the spaceship is a robot. Cassini is going to explore Saturn's rings, study Saturn's weather, and drop a probe into the thick orange atmosphere of Titan. What's hiding beneath Titan's clouds? No on ...
6 Minute English
6 Minute English

... In terms of its current lifestyle it’s here for as long again, so we’re about half way through. And then it becomes a different sort of star – it becomes a giant star and that’s probably curtains for us, actually. It’ll get a bit warm, a bit toasty, and we’ll get enveloped in the sun, and it won’t b ...
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Formation and evolution of the Solar System



The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.
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