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Stellar Evolution Notes
Stellar Evolution Notes

... A protostar is the birth of a star. They are starting out in their life as a star. Eventually, a protostar’s center becomes so hot that a fusion reaction begins. When fusion begins, a star is born ...
MOVEMENT OF THE SUN ON THE SKY
MOVEMENT OF THE SUN ON THE SKY

... 300 million metres each second Year: ...
Stellar Evolution Notes
Stellar Evolution Notes

... A protostar is the birth of a star. They are starting out in their life as a star. Eventually, a protostar’s center becomes so hot that a fusion reaction begins. When fusion begins, a star is born ...
Habitability of planets around Red Dwarf Stars
Habitability of planets around Red Dwarf Stars

– 1 – 1.
– 1 – 1.

... after the Fe core is formed is believed to carry away approximately the binding energy of the neutron star core formed at that time, ∼ 2.5 × 1053 ergs. This leaks out on a timescale of N 2 l/c, where N is the number of mean free paths to the surface (random walk), so this timescale τ ≈ R(core)2 /(lc ...
S T A R S
S T A R S

... These constitute a whole band of objects that have been detected. Most are in the size range of 100-500km. About 90% are in a roughly circular orbit beyond Neptune. Another scattered band exists in an inclined elliptical orbit and extends out to about 200AU. These are more than another asteroid belt ...
Habitable Planets Webquest
Habitable Planets Webquest

Stars - HMXEarthScience
Stars - HMXEarthScience

... Sequence” star during which size, the star grows in size as it uses up its fuel 5. Eventually when the hydrogen fuel becomes exhausted, the star expands greatly becoming a giant or a supergiant ...
Physivd Preliminary Module 8.5 The Cosmic Engine
Physivd Preliminary Module 8.5 The Cosmic Engine

The Ceres Connection - MIT Lincoln Laboratory
The Ceres Connection - MIT Lincoln Laboratory

... formation of the solar system, most likely material that never coalesced into a planet because of Jupiter’s gravitational influence. The estimated total mass of all the minor planets is much less than that of Earth’s Moon. Only two dozen minor planets in the main asteroid belt have diameters greater ...
steady flow
steady flow

... • 1920 Aston measures mass defect of helium (!= 4p’s) • 1920 Nuclear Astrophysics is born with Sir Arthur Eddington remarks in his presidential address to the British Association for the Advancement of Science: “Certain physical investigations in the past year make it probable to my mind that some p ...
PPT 5 - Uranus, Neptune and Pluto
PPT 5 - Uranus, Neptune and Pluto

... Cloud-belt structure with high-velocity winds; origin not well understood. Darker cyclonic disturbances, similar to Great Red Spot on Jupiter, but not long-lived. White cloud features of methane ice crystals ...
Geology/Physics 360
Geology/Physics 360

... We will briefly discuss the orbit of the moon in class. We will return to the moon later in the semester (it has its own chapter) The moon goes through its cycle of phases in 29.5 days however the sidereal month is the time the moon takes to complete an orbit relative to the distant stars of one co ...
ph709-10
ph709-10

... axis < 0.07 AU have low e. This is similar to binary stars, and is likely due to tidal circularization. Earth's eccentricity is 0.017, while Jupiter's is 0.094. In our solar system, the planet with the largest eccentricity is Pluto at 0.244, and Mercury with 0.205. The planet with the lowest eccentr ...
Kerboodle Gravity Questions673 KB
Kerboodle Gravity Questions673 KB

... Surprising observations of a star swiftly orbiting the cloudy heart of the Milky Way Galaxy have verified with near certainty the existence of a central black hole, a theoretical object that still eludes direct detection. Astronomers watched the star for a decade, tracking two-thirds of its path aro ...
Rachel and the TreeSchoolers Theme Song
Rachel and the TreeSchoolers Theme Song

... favorite. Oh, Bongo, that’s actually an airplane! Airplane, airplane, flying ‘round Sometimes I hear zooming sounds I can see your flashing lights Moving slowly through the night Now I know just what you are You’re my favorite “not a star” ...
Chapter 10 Center of Gravity
Chapter 10 Center of Gravity

... piece of clay or putty, and is distorted into different shapes, then its CG may change as its shape is changed. Even then, it has one CG for any given shape. ...
16. Gravity and Space - Mr. Brick's Web Page
16. Gravity and Space - Mr. Brick's Web Page

... The effect of a large asteroid hitting our planet would be catastrophic, it could destroy many species, including the human race. The damage that an asteroid might cause can be estimated by examining crater sites created by earlier asteroid impacts, both on Earth and other planets. ...
The human race has made great strides in the last few centuries
The human race has made great strides in the last few centuries

... pop out of the surface, leaving a sunspot as a footprint. The Sun has an eleven year sunspot frequency cycle. Where the magnetic fields interact with the bulk motion of plasma at the surface, high energy phenomena are generated. Giant loops of confined, hot gas lift off the surface. Some material st ...
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... As Earth revolves around the Sun, the northern and southern hemispheres experience the seasons – spring, summer, autumn, and winter. The Earth’s tilt is what is primarily responsible for creating our seasons, not the distance that Earth is from the Sun. When Earth is farthest from the Sun, the north ...
The difference between asteroids and meteorites
The difference between asteroids and meteorites

... coming closer to the Sun, and therefore closer to Earth. In addition to the asteroid belt, however, there have been recent discussions among astronomers about the potential existence of large number asteroids in the Kuiper Belt and Oort Cloud. Asteroids are sometimes referred to as minor planets or ...
Herschel
Herschel

... The data suggest that the dominant grain size is larger than ~100 µm and that the small grains are strongly underabundant. This clashes with what is observed in the debris discs studied so far, where the models point to grains in the range of ~µm. A possible explanation for the scarcity of small gr ...
Solar system formation by accretion has no observational evidence
Solar system formation by accretion has no observational evidence

... seems to be undergoing dissolution rather than evolving. This is why theorists have been unable to explain how the solar nebula—even if it had existed—could collapse into celestial bodies. At the end of a long review of nebula collapse theories (also known as cloud formation theories), one theorist ...
January 14 - Astronomy
January 14 - Astronomy

... with time. Also, the axis of rotation of any spinning object remains in a fixed direction in ...
Gravitational Field
Gravitational Field

...  Understand the term weightlessness of objects in free fall and orbit  Describe gravitational fields  Contrast Einstein's concept of gravity to that of Newton’s ...
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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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