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10 New Constellations
10 New Constellations

... Also known as Alpha Persei, Mirfak is located around 500 light years from Earth and is the brightest star in the constellation, it's a white supergiant with a diameter around 30 times larger than the sun. Algol Also known as Beta Persei, Algol is actually a three star system located around 90 light ...
Venus1
Venus1

Full PDF - Royal Society Publishing
Full PDF - Royal Society Publishing

... The mass of the resulting atmosphere then depends on the composition of the planetesimals, and thus on their initial location as well as on the metallicity of the star. For a planet like the Earth formed at warm temperatures (where water ice is not stable), the available amount of volatites should b ...
Chapter 1 LONG-TERM VARIATIONS IN THE GALACTIC
Chapter 1 LONG-TERM VARIATIONS IN THE GALACTIC

... Bahcall, 1985), this stratification will result with a time variable ISM pressure. More variations arise from the spiral structure. The spiral density waves are generally O(10%) perturbations in the overall density, necessarily giving rise to similar variations in the pressure. However, cold compone ...
Star Map - Science Centre
Star Map - Science Centre

... The Big Dipper is one of the most famous asterisms (star patterns) throughout history. In some places of the Northern Hemisphere, its seven brightest stars can be seen all year round. Further South near the equator, it is only visible for a few months. Merak and Dubhe are known as The Pointers, poin ...
High precision astrometry as a tool for Fundamental
High precision astrometry as a tool for Fundamental

... Photon noise, near diffraction limited imaging ...
Moons of the Solar System
Moons of the Solar System

... overall composition • Formed in orbit around jovian planets • Circular orbits mostly in the same direction as planet rotation © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley ...
Astonomy-Space The Final Frontier
Astonomy-Space The Final Frontier

... Construct an explanation of the Big Bang theory based on astronomical evidence of light spectra, motion of distant galaxies, and composition of matter in the Universe. Communicate scientific ideas about the way stars, over their life cycle, produce elements. Use mathematical or computational represe ...
PowerPoint
PowerPoint

... • These are objects that are below 80 Jupiter masses. • The central density and temperature do not get large enough for nuclear fusion to occur. • These failed stars, gradually cool down and contract. • Recently, there have been a number of discovered brown dwarves. ...
Latitude and Longitude - Harvard University Laboratory for
Latitude and Longitude - Harvard University Laboratory for

... Hc = height (after corrections for refraction) d = declination of object L = latitude ...
1 A Re-appraisal of the Habitability of Planets Around M Dwarf Stars
1 A Re-appraisal of the Habitability of Planets Around M Dwarf Stars

... Hollingsworth,9 Manoj M. Joshi,13 Steven Kilston,14 Michael C. Liu,15 16 Eric Meikle,17 I. Neill Reid,18 Lynn J. Rothschild,9 John M. Scalo,19 Antigona Segura,20 Carol M. Tang,21 James M. Tiedje,22 Margaret C. Turnbull,4 Lucianne M. Walkowicz,23 Arthur L. Weber,1 and Richard E. Young9 Abstract Stabl ...
Sternentstehung - Star Formation
Sternentstehung - Star Formation

ASTR 330: The Solar System - University of Maryland
ASTR 330: The Solar System - University of Maryland

... • 1910 was a wonderful year for comet-viewing: as well as the anticipated return of Comet Halley, an even brighter new comet also appeared some months earlier (the “Great Daylight Comet of 1910” – why do you think it got this name?) • 1986 was a disappointment for Halley watching: the comet was on t ...
Cycles of the Sky
Cycles of the Sky

... – Standing in that umbral spot, you would be in total shadow, unable to see any part of the sun’s surface, and the eclipse would be total. – However, if you were located outside the umbra, in the penumbra, you would see part of the sun peeking around the edge of the moon and the eclipse would be par ...
Event Booklet - Exoplanets I Conference
Event Booklet - Exoplanets I Conference

... at Kitt Peak National Observatory (the latter which had time allocated through the NN-EXPLORE program). These observations aid the confirmation and characterization of these new exoplanets, many which are smaller than Neptune, orbit cool, nearby stars, and are amenable to detailed atmospheric charac ...
Chapter9- Asteroids, Comets, Dwarf Planets-pptx
Chapter9- Asteroids, Comets, Dwarf Planets-pptx

... Why are there very few asteroids beyond Jupiter's orbit? A. There was no rocky material beyond Jupiter's orbit. B. The heaviest rocks sank toward the center of the solar system. C. Ice could form in the outer solar system. D. A passing star probably stripped away all of those asteroids, even if they ...
April 2015 - Southern Astronomical Society
April 2015 - Southern Astronomical Society

... dark matter does not slow down when it collides with itself. This is significant as it shows the ghostly substance interacts with itself less than previously thought, narrowing down the options of what this invisible material might be. Dark matter does not reflect or absorb light. But its presence c ...
Lecture18
Lecture18

... Extrasolar planets Many hundreds now known! Very difficult to detect (star much much brighter)... indirect “wobble” methods used based on velocity (Doppler shift) or position (Astrometry) of the star, “transits” (planet blocks starlight). Which detection method can be used depends on orientation of ...
Artificial comets
Artificial comets

... Dirty snowballs Comets formed about 4.5 billion years ago, at the same time as our solar system. An estimated one hundred billion comets surround our solar system beyond the orbit of our outermost planet, Neptune. These comets make up the Kuiper belt and the Oort cloud. Some comets leave their “park ...
Year 7 Module 3 Practice Paper
Year 7 Module 3 Practice Paper

... Partridges feed mainly on insects and wild plants (weeds). Some farmers spray their crops with chemicals to kill insects and weeds. How would this affect the number of foxes? ...
fifth midterm -- review problems
fifth midterm -- review problems

... The Earth is 9.3 × 10 7 miles from the Sun. Calculate the gravitational force between the Earth and the Sun. The Earth-Sun distance is called 1.00 A.U. (astronomical unit). If Jupiter orbits the Sun in 11.9 years, what is the Jupiter-Sun distance in A.U. (Assume circular orbits.) If the mass of the ...
- Mastering Physics Answers
- Mastering Physics Answers

... A neutrino is a lightweight (almost massless) particle that is a by­product of nuclear reactions and radioactive decay. Neutrinos have the unusual property that they do not interact with light, and therefore they do not respond to the electromagnetic forces that affect protons and electrons. Neutrin ...
Origins: List of Evidences
Origins: List of Evidences

... true age limit. Higher age limits simply rule out hundreds of millions or billions of years needed for evolution due to the fact that any age above any maximum age limit violates that limit. Conversely, if an age is under all the maximum age limits, it is acceptable, even if it is far below the lowe ...
ppt
ppt

File
File

... Describe the methods scientists have used to help with this search in both our Solar System and the rest of the Universe. ...
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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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