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Dynamical evolution of planetary systems
Dynamical evolution of planetary systems

... The apparent regularity of the motion of the giant planets of our solar system suggested for decades that said planets formed onto orbits similar to the current ones and that nothing dramatic ever happened during their lifetime. The discovery of extra-solar planets showed astonishingly that the orbi ...
The Oort Cloud
The Oort Cloud

... would not be much perturbed by typical passing stars nor by the gravity of the planets of the solar system, and the comets could reside in the inner cloud or belt for long periods of time without detection. It has been speculated, however, that a rare close passage by another star (possibly an undet ...
A new method to determine the mean density of massive Solar
A new method to determine the mean density of massive Solar

... determined the mean densities of Uranian satellites Miranda, Ariel, Umbriel, Titania, Oberon; Person et al. (2006) – Neptune’s satellite Triton. Thus and so, the present article analysis includes data on the known mean densities of 131 objects of the Solar System. The article treats a body’s mean de ...
ASTR 110 Lab Manual Sections M02 M03 M04
ASTR 110 Lab Manual Sections M02 M03 M04

... “2” above the three. 52 = 5 × 5 = 25. The exponent tells you how many times to multiply that number by itself: 84 = 8 × 8 × 8 × 8 = 4096. The square of a number simply means the exponent is 2 (three squared = 32 ), and the cube of a number means the exponent is three (four cubed = 43 ). Here are som ...
Asteroids - GEOCITIES.ws
Asteroids - GEOCITIES.ws

... crossers, change appreciably on a time scale of a few years or tens of years. For this reason about half the known Amors, including 1221 Amor, are part-time Earth crossers. Only asteroids that cross the orbits of planets, such as the Earth-approaching asteroids and objects like 944 Hidalgo and 2060 ...
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bode elert johann

... catalogue lists 3175 stars. They are arranged by constellation, starting with Cassiopeia (see Figure 3). The first column, headed “Fl. No”, gives the correct Flamsteed number. The positions (right ascension, declination) are calculated for 1800. Thus Bode’s star catalogue of 1776 is an extended and ...
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... space: H, O, C, and N. He assumed these atoms combined on a surface of some kind to form frozen saturated molecules. The surface was left as ‘to be determined’ (TBD). This is what later became known as the ‘dirty ice’ model and was the first application of surface physics to interstellar dust. The di ...
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... An attentive observer will soon notice that individual bright stars that are rather close together in the sky seem to form simple geometric shapes – squares, rhombuses, crosses, circles, arches. Giving a name to these shapes in the sky makes them more familiar to you and easier to locate again. That ...
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April 2016 - Central Arkansas Astronomical Society

... The gravita onal waves were detected on September 14, The existence of gravita onal waves was first demonstrated 2015 at 5:51 a.m. Eastern Daylight Time (09:51 UTC) by both in the 1970s and 80s by Joseph Taylor, Jr., and colleagues. of the twin Laser Interferometer Gravita onal‐wave Taylor and Russel ...
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ATTENTION: Epreuve non définitive!!!

... for observed irregularities and determined a position based on an orbit in the ecliptic plane and Bode’s Law that suggested a radius twice that of Uranus. In his third memoir, read on 31 August 1846, le Verrier gave more precise limits within which one should look for the new planet and even predict ...
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Stellarium User Guide - Skolekonsulenterne.dk

... As well as travelling through time, Stellarium lets to look around the sky freely, and zoom in and out. There are several ways to accomplish this listed in table 3.4. Let’s try it. Use the cursors to move around left, right, up and down. Zoom in a little using the Page Up key, and back out again usi ...
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... that pre-dated Solar System formation, along with material processed in the Solar Nebula.6 Aspects of such processing are illustrated in Figure 1.0. Detailed study of interstellar ices has advanced greatly in recent years7 with enhanced theoretical models and laboratory analogs, as well as with remo ...
Sidereus Nuncius (Print Translation)
Sidereus Nuncius (Print Translation)

... But what greatly exceeds all admiration, and what especially impelled us to give notice to all astronomers and philosophers, is this, that we have discovered four wandering stars, known or observed by no one before us. These, like Venus and Mercury around the Sun, 21 have their periods around a cert ...
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... eclipse, or a lunar occultation, Scientific Astronomer allows you to determine the location and details of the event. Similarly, you can use the package to re-create the circumstances of ancient eclipses, planetary alignments, and other events of historical significance. A very simple application is ...
r202 the new astronomy
r202 the new astronomy

... enormous work, begun by Prof. Helmut Werner shortly after the Second World War. This project of H. Werner, who was astronomer and member of the staff of the Carl Zeiss firm was continued after his death in 1973 by F. Schmeiller, who edited this survey of the fixed stars visible to the naked eye in 1 ...
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Cassiopeia Kelly Pearce

... (Stars.Astro.Illinois.edu, Segin, 2010). It forms the outer most left point of the W and is the fifth brightest of all 5 stars. It is noticeably dimmer than the remaining stars but definitively forms the one of the outermost points of the shape. The next star to the right is Delta Cassiopeiae and is ...
Advances in exoplanet science from Kepler (Lissauer et al. 2014)
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... Most of the planet candidates were found by the automated Kepler dataanalysis pipeline, but many of the larger candidates were first identified by eye, including several dozen using data from the public Kepler archive by citizen scientists through the Planet Hunters project29. Other groups have foun ...
PLUTO - Department of Earth and Planetary Sciences, Northwestern
PLUTO - Department of Earth and Planetary Sciences, Northwestern

... location of a ninth planet, beyond Neptune, and then find it, it would surely improve his status (Tombaugh, 1986). At the faintness this planet was predicted to be, there are millions of points of light in the sky and the task is to find one that shifts its position relative to the background stars… ...
Eight billion asteroids in the Oort cloud
Eight billion asteroids in the Oort cloud

... the region interior to 2.5 au could represent a significant fraction of bodies in the present-day Oort cloud. To address the question of how common asteroids should be in the Oort cloud, we perform simulations of the Oort cloud’s formation, considering small bodies starting with dynamically cold orb ...
Eight billion asteroids in the Oort cloud
Eight billion asteroids in the Oort cloud

... than 1% of objects ever become Oort cloud objects, rising to ∼ 10% for objects beginning beyond the orbit of Uranus. Qualitatively, this outcome is unsurprising, since Fernandez & Ip (1981) found that Neptune and Uranus produce Oort cloud objects much more effectively than do Jupiter or Saturn, and ...
a changing cosmos - Whittier Union High School District
a changing cosmos - Whittier Union High School District

... Walter Alvarez from the University of California at Berkeley. He was studying a thin layer of clay between rock layers of the Cretaceous Period (Age of Reptiles) and the Tertiary Period (containing no dinosaurs fossils). The clay layer contained very large amounts of the rare element iridium, which ...
Advances in exoplanet science from Kepler
Advances in exoplanet science from Kepler

... positives plague ground-based searches for exoplanets, but the Kepler light curves (starlight received as a function of time) are of such high quality that they can usually be used to discriminate between grazing or blended stellar eclipses and planetary transits. Moreover, Kepler is an imaging inst ...
oC - geogreenapps
oC - geogreenapps

... lending it forth to the world. ID ita preparation for the Prell, the aGthor has availed himaelf of all the hel.. within his reach. He h. OOD8Ulted all the boob UPOD the wbject that were available in th. COIIDtry t U well .. many practical teacheJ'll, and gentlemen of acknowledged ecientific abilitie ...
Starwalk Manual En
Starwalk Manual En

... The Search feature allows you to switch between the following categories: • Stars and constellations • Solar system - includes planets, the Moon, the Sun, meteor showers, dwarf planets, asteroids, comets • Deep space – includes clusters, nebulas, galaxies, clouds • Satellites Each category has a lis ...
Irregular Satellites of the Giant Planets
Irregular Satellites of the Giant Planets

... in brightness of satellites with increasing heliocentric distance means that current surveys at Uranus and Neptune are almost certainly much less complete than those at Jupiter and Saturn, raising the distinct possibility that we are seeing only the largest member or two of each orbital group. It is ...
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Astronomical naming conventions

In ancient times, only the Sun and Moon, a few hundred stars and the most easily visible planets had names. Over the last few hundred years, the number of identified astronomical objects has risen from hundreds to over a billion, and more are discovered every year. Astronomers need to be able to assign systematic designations to unambiguously identify all of these objects, and at the same time give names to the most interesting objects and, where relevant, features of those objects.The International Astronomical Union (IAU) is the officially recognized authority in astronomy for assigning designations to celestial bodies such as stars, planets, and minor planets, including any surface features on them. In response to the need for unambiguous names for astronomical objects, it has created a number of systematic naming systems for objects of various sorts.
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