* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Volume 20 Number 10 September 2012
Lunar theory wikipedia , lookup
IAU definition of planet wikipedia , lookup
Geocentric model wikipedia , lookup
Hubble Deep Field wikipedia , lookup
Theoretical astronomy wikipedia , lookup
Cassiopeia (constellation) wikipedia , lookup
Chinese astronomy wikipedia , lookup
History of Solar System formation and evolution hypotheses wikipedia , lookup
Spitzer Space Telescope wikipedia , lookup
Definition of planet wikipedia , lookup
Space Interferometry Mission wikipedia , lookup
Formation and evolution of the Solar System wikipedia , lookup
Extraterrestrial skies wikipedia , lookup
Rare Earth hypothesis wikipedia , lookup
History of supernova observation wikipedia , lookup
Stellar evolution wikipedia , lookup
Comparative planetary science wikipedia , lookup
Cygnus (constellation) wikipedia , lookup
Dialogue Concerning the Two Chief World Systems wikipedia , lookup
Future of an expanding universe wikipedia , lookup
Aquarius (constellation) wikipedia , lookup
Astrobiology wikipedia , lookup
High-velocity cloud wikipedia , lookup
Perseus (constellation) wikipedia , lookup
International Ultraviolet Explorer wikipedia , lookup
Planetary habitability wikipedia , lookup
Stellar kinematics wikipedia , lookup
History of astronomy wikipedia , lookup
Astronomical naming conventions wikipedia , lookup
H II region wikipedia , lookup
Hebrew astronomy wikipedia , lookup
Observational astronomy wikipedia , lookup
Ancient Greek astronomy wikipedia , lookup
Corvus (constellation) wikipedia , lookup
Extraterrestrial life wikipedia , lookup
THE YOUNG ASTRONOMERS NEWSLETTER Volume 20 Number 10 STUDY + LEARN = POWER OWER FIRST 360-DEGREE PANORAMA FROM CURIOSITY – AND MORE September 2012 MORE RUSSIAN-STYLE MOTIVATION Russian Prime Minister Dmitry Medvedev said he will name officials responsible for a failed satellite launch: "I would like to hold a meeting on this …. it will be prepared by the appropriate deputy prime minister and structures. They are tasked with reporting who should be punished and what to do next," And “"I don't know what the cause of the failures is but this could not be tolerated anymore .… We are losing authority and billions of rubles.” Remarkable image sets from the Curiosity rover and Mars Reconnaissance Orbiter (MRO) are continuing to develop the story of Curiosity's landing and first days on Mars. The first images include the rover's first self-portrait and the first 360-degree view of its new home in Gale Crater. Curiosity, the centerpiece of the Mars Science Laboratory mission, touched down in Mars' Gale Crater PERSIEDS METEOR SHOWER on August 5th. It is expected to explore the chemical composition of this area and figure out how it was formed, Some comments from the Internet: with an eye out for signs that Mars once had conditions “It did not disappoint. Some were huge and slow, and some more typical streaks in the sky.” suitable for life. See: http://1.usa.gov/MfiyD0 “What an incredible treat, I saw enough to lose count. “ NEW KEPLER DISCOVERIES “Some were fast, some had long trails some were red The Kepler spacecraft has discovered 41 new and orange balls with long bright trails.” transiting planets in 20 star systems, increasing the “The second one I saw was the brightest one I ever saw. number of Kepler's confirmed planets to 116 in 67 It was so bright that it cast shadows and left an ionized tail systems, over half of which contain more than one planet. for about 20 to thirty seconds.” 19 of the 20 have two closely spaced planets and one “Spectacular! I was delighted with this rain of stars. system has three. The planets range up to seven times “Simply perfect!” the radius of Earth, but generally orbit so close to their “WOW! Simply Awesome!” parent stars that they are hot, inhospitable worlds. SPAIN’S MOON ROVER China will send a Spanish rover to the Moon in June 2014, according to the company which heads the "Barcelona Moon Team" that is competing in the Google Lunar X Prize contest. It is the only team based in Spain to take part in the Google Lunar X Prize, which challenges participants to create a robot that can move over the lunar surface and send live images back to Earth before December 2015. A LONELY GALAXY Many galaxies are comparatively isolated without close neighbors. One such example is the small galaxy known as DDO 190 ("DDO" stands for the David Dunlap Observatory, now managed by the Royal Astronomical Society of Canada, where the catalog was created). DDO 190 is classified as a dwarf irregular galaxy as it is relatively small and lacks clear structure. Older, reddish stars mostly populate the outskirts, while some younger, bluish stars gleam brightly in the more crowded interior. See: http://www.nasa.gov/ multimedia/imagegallery/Image_feature_2336.html THE VOYAGER SPACECRAFT Thirty-five years ago, NASA's Voyager 2 spacecraft, the first Voyager spacecraft to launch, departed on a journey that would make it the only spacecraft to visit Uranus and Neptune and the longest-operating NASA spacecraft ever. Voyager 2 and its twin, Voyager 1, that launched 16 days later on Sept. 5, 1977, are still going strong, hurtling away from the Sun. Mission managers are eagerly anticipating the day when they break on through to the other side - the space between stars. GLIESE 581D Based on new data, astronomers now believe exoplanet Gliese 581g is the best candidate as a potentially habitable exoplanet. Its star, Gliese 581 is well known for having four planets with the outermost planet, Gliese 581d, already suspected as habitable. FASTEST CME On July 23rd, a massive cloud of solar material erupted off the Sun’s right side and zoomed out into space. Scientists clocked this giant cloud (a coronal mass ejection) as traveling between 1,800 to 2,200 miles per second as it left the Sun. This was the fastest CME ever observed by the STEREO spacecraft. The mission consists of two spacecraft with orbits that give them views of the Sun that cannot be had from Earth. VICTIM OF A HUGE BLACK HOLE In 2011, astronomers watched a star at the center of a galaxy in Draco send out a distress flare when a giant black hole tore it to shreds. Now, some of the deceased star's glowing remains whirl around the black hole and emit x-rays and reveal the black hole’s mass. Satellites discovered that the x-rays fluctuate in strength every 200 seconds. Assuming this is the orbital period of hot gas revolving near the black hole, the astronomers calculated that the monster weighs 450,000 to 5 million times more than the Sun. This agrees with previous estimates and makes the black hole comparable to the one at the Milky Way's center. ================================================================================ SCIWORKS – for information and planetarium schedules call: 767-6730 The Sky Tonight? See - http://www.skymaps.com/downloads.html and also http://amazing-space.stsci.edu/tonights_sky/ Astronomy Picture of The Day - http://apod.nasa.gov/apod/astropix.html SLOAN SKY SURVEY – The new data is available to students, teachers, and the public. The SkyServer website includes lesson plans for teachers that use DR9 data to teach astronomy and other topics in science, technology, and math. DR9 data will also feature a new release of the Galaxy Zoo citizen science project, which allows online volunteers to contribute to cutting-edge astronomy research. See: http://www.sdss3.org/dr9 ============================================================================================================================================= PUZZLES S I G N S C N E T Y R N G Y R O T S H T FIND THE WORD E N A A I M A G E S V E T L K E I S S I O E L A P S E S E M R I E A H D T E S R M R T T R R R U S I B C R A E E R G A V H A C A H R T A P A E O T W N A O L S L BREAK CRATER DRACO EARTH GUESS IMAGE KEISS LAPSE MILLION MISTY PASSES PATCH PLANS RIVAL ROVER SIGNS SLOAN THESE TREAT WHERE SCRAMBLED ASTRONOMY IDENO MORE MOONS __ __ __ __ __ STALA __ __ __ __ __ ESIMOD __ __ __ __ __ __ BOSHOP __ __ __ __ __ __ SAJUN __ __ __ __ __ (Answers below) ****** INTERNET SITES ****** Time Lapse Video from the ISS - http://vimeo.com/44801709 NGC 4700’s new stars - http://www.nasa.gov/mission_pages/hubble/science/ngc4700.html . Pipe Nebula - http://www.eso.org/public/news/eso1233/ Can you count the stars? SITE OF THE MONTH Kids’ Astronomy - http://www.astronomy.com/en/News-Observing/Astronomy%20Kids.aspx ****** SEPTEMBER MOON ****** Last Quarter: 9/8 New Moon: 9/16 First Quarter: 9/22 Full Moon: 9/30 Apogee: 9/7 2:53 PM 251,217 mi. (404295 km) Perigee: 9/18 10:53 PM 227,265 mi. (365748 km) Best observing nights: 9/7 – 9/21 The Full Moon was called the Harvest Moon. 9/22 - 1st day of Autumn. ****** PLANETS IN SEPTEMBER ****** VENUS is rising in the east before sunrise. JUPITER rises in the east before midnight and is the brightest planet every night. MARS – its red glow is to the left of Saturn after sunset. MERCURY is near the western horizon in late September. SATURN is low in the west-southwest after sunset and sinking lower each evening. URANUS rises low in the east after sunset, below the Great Square of Pegasus, and visible all night. It is opposite the Sun on the 29th (opposition). Uranus is a blue dot in telescopes and binoculars but can even be seen from a dark site. The Moon passes within 5° of Uranus at 1 AM on the 30th. ****** METEOR SHOWERS ****** NAME DATES BEST NIGHT PER HOUR WHERE TO LOOK ALPHA AURIGIDS 8/25 – 9/8 9/1 7 Low in the north. Alpha Aurigids is a “maybe” with an erratic history. It is believed to be occasional debris from Comet Keiss 2 and has produced up to 30 meteors per hour. The meteors are bright with some leaving trails. SEPTEMBER PERSEIDS 9/5 - 10/10 9/8 6 Northeast. This shower is not the same as the spectacular Perseids shower which peaks in mid-August and is one of the year's highlights. They both appear to radiate from the same constellation but are not related - they were formed by different comets. September has five minor showers with three or less per hour. ----------------------------------------------------------------------------------------------------------------------------- ---------------------------LOOK FOR: >>>>> The Andromeda Galaxy. The Andromeda constellation is twice the size of the Milky Way and looks like a narrow “V” as it spreads to the northeast. It is to the northeast from the Great Square of Pegasus. The Galaxy is a misty patch and the most distant object visible without a telescope or binoculars. >>>>> The Beehive Cluster (M44) to the upper left of Venus in mid-September. >>>>> The Moon passes only .6° south of Jupiter on the 6th. >>>>> Antares – a big, red bloated super-giant low in the southwest – the “Rival of Mars“. MISSING PLANET PHOENIX CLUSTER An international team of astronomers has discovered the first evidence of a planet's destruction by its aging star. The missing planet was devoured as the star began expanding into a "red giant" - the stellar equivalent of advanced age. The astronomers also discovered a massive planet in a surprisingly elliptical orbit around the same lithium-polluted red-giant star. New observations of the Phoenix Cluster may force astronomers to rethink how these colossal structures and the galaxies that inhabit them evolve. Clusters are some of the largest objects in the universe. (The largest is the Sloan Great Wall.) Stars are forming in the Phoenix Cluster at the highest rate ever observed for the middle of a galaxy cluster. It is also the most powerful producer of X-rays of any known cluster and among the most massive. The data also suggest the rate of hot gas cooling in the central regions of the cluster is the largest ever observed. While galaxies at the center of most clusters may have been dormant for billions of years, the central galaxy in this cluster seems to have come back to life with a new burst of star formation. See: http://www.nasa.gov/chandra and http://chandra.si.edu SPRITES High above the clouds during thunderstorms, some 50 miles above Earth, a different kind of lightning dances. Bursts of red and blue light, known as "sprites," flash for a scant one thousandth of a second. They are often only visible to those in flight above a storm, and happen so quickly you might not even see it unless you chance to be looking directly at it. Astronauts on the ISS recently captured the signature red flash of a sprite, offering the world and researchers a rare opportunity to observe one. See: http://www.nasa.gov/mission_pages/ sunearth/news/seeing-sprites.html MERGING CLUSTERS Astronomers observed two clusters full of massive stars that may be in the early stages of merging. They are in the Large Magellanic Cloud, a small satellite galaxy to our Milky Way. The two clusters in the core of the Tarantula Nebula differ in age by about one million years. The nebula, also known as the 30 Doradus complex, has been an active star-forming region for 25 million years. Smaller systems that merge into larger ones could help to explain the origin of some of the largest known star clusters. See: http://www.30doradus.org/ and also http://www.nasa.gov/multimedia/ imagegallery/image_feature_2337.html and http://www.nasa.gov/mission_pages/hubble/ science/tarantula.html NEW PHOBOS IMAGE An image taken by ESA's Mars Express spacecraft as it passed just 60 miles above Mars' largest moon Phobos is seen in fantastic detail - and in 3D. This view is much different to the faint object that astronomer Asaph Hall would have just been able to make out as he observed the Red Planet through the United States Naval Observatory's 66 cm telescope in 1877. Through this telescope he discovered Mars' smaller, outermost moon Deimos and the larger, innermost moon Phobos. A bite-sized chunk appears to be missing from the right edge of the irregular shaped moon - this is a side-on view of the rim of large impact crater Stickney, so-called after the maiden name of the discoverer's wife. Families of grooves appear to emanate from Stickney, carving channels across the approximately 27 km length of the moon. Initially thought to be associated with the Stickney impact crater, one recent theory suggests that they were instead formed when Phobos passed through debris clouds thrown up from the surface of Mars by asteroid impacts onto the planet's surface. See: http://www.esa.int/esaSC/ SEMDAB1YZ5H_index_1.html NOCTILUCENT CLOUDS Noctilucent clouds are a mystery dating back to 1885 when northern sky watchers first noticed them about two years after the eruption of Krakatoa. Ash from the Indonesian volcano caused such splendid sunsets that evening sky watching became a worldwide pastime. One observer, German T.W. Backhouse, noticed something odd. He stayed outside long enough for the twilight to fully darken, and on some nights he saw wispy filaments glowing electric blue against the black sky. Scientists thought they were some manifestation of volcanic dust until Krakatoa's ash settled and the sunsets faded. Strangely the noctilucent clouds did not go away. They're still present today, stronger than ever. But the dust behind the clouds we see now is meteor dust. SUPERNOVA WITH THREE STARS A research group from Japan used the Subaru Telescope to conduct observations of supernovae (plural of supernova) with clumpy 3-D structures. This finding supports a new scenario of supernova explosions instead of the widely accepted bipolar explosions. Five of six showed the signature of the clumpy 3-D geometry. NEW CHEMICALS? A new study concludes that white dwarfs - aged stars with the mass of the Sun or greater that have collapsed to the size of a planet, could generate unusual types of chemical bonds. Because the magnetic field around a white dwarf can be hundreds of thousands of times the strength of Earth's magnetic field, it can actually distort the shape of the electron clouds around atoms. Simulations suggest the intense fields may actually stimulate chemical reactions that typically don't take place on Earth. FAST GALACTIC WINDS Fierce galactic winds powered by an intense burst of star formation may blow gas right out of massive galaxies, shutting down their ability to make new stars. Astronomers found 29 objects with out-flowing winds measuring up to 1,600 miles per second, twice as fast as most observed galactic winds. Young, bright, and compact, these massive galaxies are in the midst of or just completing a period of star formation as intense as anyone has ever observed. IMPACT CRATERS NGC 1187 Researchers in Canada's western Arctic have found evidence of a crater that formed when a huge meteorite slammed into Earth millions of years ago. Measuring about 15 miles across, the formation was named the Prince Albert impact crater after the peninsula where it was discovered. Researchers don't know exactly when it was created, but evidence suggests the crater is between 130 million and 350 million years old. Earlier this summer, researchers in Greenland documented possibly the oldest and largest meteorite crater ever found on Earth. The crater, estimated to be 3 billion years old, currently measures about 62 miles across. But the researchers believe its width before erosion was likely more than 310 miles — much bigger than the largest visible crater, the 2-billion-year-old Vredefort crater in South Africa which measures 186 miles across. Spiral galaxy NGC 1187 in the constellation of Eridanus (The River) has six prominent arms, each containing large amounts of gas, dust, and young stars born out of the clouds of interstellar gas. It looks tranquil and unchanging, but it has hosted two supernovae explosions since 1982. In this image, the bulge of the galaxy is glowing yellow and is mostly made up of old stars. Around the outside of the galaxy many much fainter and more distant galaxies can also be seen. A supernova is near the bottom of the image. See: http://www.eso.org/public/news/eso1231/ MOST MASSIVE STARS In 2010, observers reported the most massive stars ever seen, - it exceeded what many astronomers thought was a maximum about 150 times the mass of the Sun. The heavyweight champs resided 160,000 light-years from Earth in Radcliffe 136, a dense star cluster within the Large Magellanic Cloud, the brightest galaxy that revolves around our Milky Way. They have simulated the evolution of this star cluster and found that a stellar heavyweight can result when two massive stars born orbiting each other merge into a single giant due to the frequent juggling of other stars in such a dense environment. Though the idea is plausible because massive stars usually have partners, observers need to test the claim by measuring how fast the record-breaking stars spin. SLOAN SKY SURVEY Researchers have released the largest threedimensional map of black holes and massive galaxies, it pinpoints the locations and distances to more than 1 million galaxies, each of which contains more than 100 billion stars, This will enable scientists to retrace the history of the universe for the last 6 billion years, and also, develop better estimates of how much is "dark matter" that can’t be directly seen, and "dark energy," the mysterious force that’s driving the expansion of the universe. The survey has so far covered about 8% of the sky. When completed, researchers will have mapped all massive galaxies outside the plane of the Milky Way that are visible from the Northern Hemisphere - about onefourth of the sky visible from Earth. (See page 2.) ORIGIN OF THE MOON About 4.53 billion years ago, a Mars-sized impactor slammed into Earth, forming a young, molten moon and astronomers now think that the impactor scored a direct hit, crashing into Earth at a steep angle and at a very high speed. The resulting smashup would have ejected far more Earth debris into space than some models have indicated, and with much hotter temperatures. This would mean the Moon formed from more Earthlike material than previously thought. The origin of the impactor itself is an open question. A new model suggests an origin from far-away in the solar system. SOLAR SYSTEM For decades it has been thought that a shock wave from a supernova explosion triggered the formation of our Solar System - the shock wave also injected material from an exploding star into a cloud of dust and gas, and the newly polluted cloud collapsed to form the Sun and its surrounding planets. A new Carnegie study has provided the first fully three-dimensional models for how this process could have happened. SN1006 Astronomers say that the brightest supernova in recorded history left no star after the explosion. In 1006, observers watched a star explode in the constellation Lupus shining about a dozen times more brilliantly than Venus. The explosion was a Type Ia supernova, the most luminous variety, which occurred when a small, dense star known as a white dwarf blew up. Such a supernova is supposed to result when a larger companion star dumps material onto the white dwarf, triggering a runaway nuclear reaction that annihilates the small star. But a thorough search for the larger companion, has turned up nothing. This finding suggests the explosion arose when two white dwarfs that were in orbit around each other merged and blew up - more Type Ia supernovae may stem from double white dwarfs than astronomers had thought. See: http://chandra.harvard.edu/photo/2005/sn1006/ KEPLER-30 Earlier this year, scientists discovered three planets circling a star (Kepler-30) which is about the size and mass of the Sun it has ahuge, dark spot similar to the sunspots on the face of the Sun. By tracking the spot, they determined that the star rotates once every 16 days suggesting that Kepler-30 is a young, very active star. SUPER-SPEEDY PULSAR Scientists say that a newly discovered pulsar fleeing from the scene of a violent supernova explosion may be the fastest traveling pulsar yet discovered. The small but powerful neutron star is almost 25 times faster than most similar objects move. The explosion sent it flying away between 5.4 and 6.5 million miles per hour. When the dust clears from a supernova, the outer layers of the dying star blow into space leaving behind a neutron star - a city-sized object with a mass comparable to the Sun. ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ The YOUNG ASTRONOMERS NEWSLETTER is distributed by the Forsyth Astronomical Society. :SREWSNA YMONORTSA DELBMARCS SUNAJ ,SOBOHP ,SOMIED ,SALTA ,ENOID