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April 2011 - Skyscrapers, Inc.
April 2011 - Skyscrapers, Inc.

... himself. The light-colored bands and zones in Saturn’s cloud tops are much less prominent than those of Jupiter. (Very little cloud detail can be seen in small telescopes.) However, bright “spots” do develop from time to time. As I write this column at the end of February, a very large bright featur ...
September 2011 - Newbury Astronomical Society
September 2011 - Newbury Astronomical Society

... the beginner to astronomy. There will also be a monthly series of articles providing advice and help on the various instruments and equipment available to the modern amateur astronomer. This month we will be thinking about observing the Moon with basic equipment namely the Mk.1 eyeball and binocular ...
12_Testbank
12_Testbank

... 4) Explain how astronomers determine the size of an asteroid without resolving it. Answer: The brightness of an asteroid depends on its size, distance, and reflectivity. The brightness can be measured using a telescope, the distance is known from its orbit, and the reflectivity can be measured by c ...
Frantic Finish - Max-Planck
Frantic Finish - Max-Planck

... THE ASTRONOMERS GUESSING It could then also be possible to solve a mystery that has increasingly moved into the research spotlight in recent years: ultrabright supernovae, or superluminous supernovae, as astronomers call them. The scientists observed the first example of this type in 2010. Although ...
Paper - Astrophysics - University of Oxford
Paper - Astrophysics - University of Oxford

... 2.1. Formation of stars across the Universe When did stars form? To answer this basic question we can make use of the fact that every star must eventually die. Indeed the more massive stars die in spectacular supernova explosions that can outshine a whole galaxy. With an ELT these explosions can be ...
Desert Skies - Tucson Amateur Astronomy Association
Desert Skies - Tucson Amateur Astronomy Association

... but to locate them you should use a finder chart such as that found at http://tinyurl.com/qezbz (on the Sky Publishing website). Neither of these planets show much detail but Uranus will appear greenish and Neptune bluish. Uranus is unique in that its pole is tipped 98degrees to the ecliptic, so it ...
ph709-14
ph709-14

... Beta Pictoris may be due to the presence of large disk bodies (i.e., planets) that collide with icy Edgeworth-Kuiper Belt type objects (dormant comets) to replenish the dust. ...
No Slide Title
No Slide Title

... very stable pulsation modes. The presence of a planet will be revealed in anomalous timings, just as with pulsar planets ...
Quiz Reviews - Orion Observatory
Quiz Reviews - Orion Observatory

... Test 11. Searching for Extrasolar Planets 1. How did scientists first look for extrasolar planets? Why were their discoveries false? 2. How were their first extrasolar planets found? Why were scientists less interested in them? 3. How was the first extrasolar planet orbiting a main sequence star fou ...
Asteroids, Comets, and Dwarf Planets Their Nature, Orbits, and
Asteroids, Comets, and Dwarf Planets Their Nature, Orbits, and

... 4) Explain how astronomers determine the size of an asteroid without resolving it. Answer: The brightness of an asteroid depends on its size, distance, and reflectivity. The brightness can be measured using a telescope, the distance is known from its orbit, and the reflectivity can be measured by c ...
Oct 2011 - Bays Mountain Park
Oct 2011 - Bays Mountain Park

... wrote to Lassell, encouraging him to try to observe this new planet, with the intention of possibly being the first to spot its moons. Lassell first observed Neptune the night of October 2nd, which easily showed a disk. For the next week, Lassell continued to observe when weather permitted. Finally, ...
Chapter 15 The Formation of Planetary Systems
Chapter 15 The Formation of Planetary Systems

... of the sort that can now be detected. They are mostly gas giants like Jupiter, but closer to star. Why didn’t our Jupiter migrate? Nearly all of these have been discovered using the radial velocity method. This method (and most other methods) miss planets far from their stars, so can’t tell how comm ...
Jupiter returns as king of the night sky
Jupiter returns as king of the night sky

... Leo, the lion. You might even be able to see the lion's mane – beginning with Regulus, look for a pattern of stars that traces out an upside-down question-mark. Jupiter revealed This July, we will begin to learn more about Jupiter than ever before. NASA's spacecraft Juno has been travelling towards ...
March 15 Newsletter
March 15 Newsletter

... against it. It would be enough to shred a planet. It may even be that long ago a system of worlds did swing about the pulsar in steady orbits, but if so they would have been on fire, violently boiling under the impact of the terrible radiation. From each a vast plume of vaporised rock would have str ...
The Sky This Month Mar Apr 2015
The Sky This Month Mar Apr 2015

... approx. 13.78 km per second (49,600 kph), then head out into the Kuiper Belt. The Pluto-and-moons system will be approximately face-on, so close attention will be payed up to the last days of approach in order to “thread the needle”. Radio signal travel times are more than 4 hours one-way. The space ...
- EPJ Web of Conferences
- EPJ Web of Conferences

... example Latham et al. 2009). These false positives typically involve multiple star systems which produce light curves derived from wide-field survey images that are consistent with a planet transiting a single star. While most of the false positives are easily identified and rejected based on a few ...
February 2013 - astronomy for beginners
February 2013 - astronomy for beginners

... brightest stars are called Pollux (β) and Castor (α) and are known as the Gemini Twins. The twins originated in a Greek myth which told that they had one mother but two fathers. Castor was the mortal son of King Tyndareus but Pollux was the immortal son of the God Zeus who had disguised himself as C ...
April - Bristol Astronomical Society
April - Bristol Astronomical Society

... Like Corvus, Crater is an ancient constellation, it is linked to the story of Corvus and Apollo. It was put into the sky just out of reach of the Corvus as a punishment for the bird failing to fetch water for Apollo, the cup is normally represented as a large double-handed chalice of the type known ...
Uranus - Rackspace
Uranus - Rackspace

... in the solar system. ...
The Search for Extrasolar Planets
The Search for Extrasolar Planets

... and results obtained in the decade after the discovery of the planet 51 Peg b. The existence of planets orbiting other stars was speculated upon even in the 4th century BC, when Epicurus and Aristotle debated it using their early notions about our world. Epicurus claimed that the infinity of the Uni ...
Second Semester Study Guide
Second Semester Study Guide

... 25. What conclusion can be drawn from the fact that some planets with solid surfaces and satellites have impact craters? A. Collisions between Solar System bodies and planetesimals were common at one time. B. The young planets had softer surfaces. C. Volcanoes were very active in the early stages of ...
The most common habitable planets – atmospheric characterization
The most common habitable planets – atmospheric characterization

... planets (Gonzalez 1998; Fisher & Valenti 2005). On the other hand, the extensive debris disc discovered (Greaves et al. 2004) indicates that it had the necessary material for rocky planet formation, and the lower metallicity may indicate that PP01 was formed closer to the star than was the case for ...
Lesson Plan - ScienceA2Z.com
Lesson Plan - ScienceA2Z.com

... Some well-known constellations contain striking and familiar patterns of bright stars. Examples are Orion (containing a figure of a hunter), Leo (containing bright stars outlining the form of a lion), Scorpius (a scorpion), and Crux (a cross). The International Astronomical Union (IAU) divides the s ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

... This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed Seth B. Nicholson and Nicholas U. Mayall of from multiple Hubble Space Telescope photographs taken from 2002 to 2003. the Mount Wilson Observatory published a note on the mass of Pluto, based on th ...
Chapter 15 The Formation of Planetary Systems
Chapter 15 The Formation of Planetary Systems

... of the sort that can now be detected. They are mostly gas giants like Jupiter, but closer to star. Why didn’t our Jupiter migrate? Nearly all of these have been discovered using the radial velocity method. This method (and most other methods) miss planets far from their stars, so can’t tell how comm ...
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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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