Summer Constellation Worksheet
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Exploring Exoplanet Populations with NASA's Kepler Mission
SPECIAL FEATURE: PERSPECTIVE PERSPECTIVE SPECIAL FEATURE: Exploring exoplanet populations with NASA’s Kepler Mission Natalie M. Batalha1 National Aeronautics and Space Administration Ames Research Center, Moffett Field, 94035 CA Edited by Adam S. Burrows, Princeton University, Princeton, NJ, and accepted by the Editorial Board June 3, 2014 (received for review January 15, 2014) The Kepler Mission is exploring the diversity of planets and planetary systems. Its legacy will be a catalog of discoveries sufficient for computing planet occurrence rates as a function of size, orbital period, star type, and insolation flux.The mission has made significant progress toward achieving that goal. Over 3,500 transiting exoplanets have been identified from the analysis of the first 3 y of data, 100 planets of which are in the habitable zone. The catalog has a high reliability rate (85–90% averaged over the period/radius plane), which is improving as follow-up observations continue. Dynamical (e.g., velocimetry and transit timing) and statistical methods have confirmed and characterized hundreds of planets over a large range of sizes and compositions for both single- and multiple-star systems. Population studies suggest that planets abound in our galaxy and that small planets are particularly frequent. Here, I report on the progress Kepler has made measuring the prevalence of exoplanets orbiting within one astronomical unit of their host stars in support of the National Aeronautics and Space Admin- istration’s long-term goal of finding habitable environments beyond the solar system. planet detection | transit photometry Searching for evidence of life beyond Earth is the Sun would produce an 84-ppm signal Translating Kepler’s discovery catalog into one of the primary goals of science agencies lasting ∼13 h. -
Get Outside What to Look for in the Summer Sky Your Hosts of the Summer Sky Are Three Bright Stars — Vega, Altair and Deneb
Get Outside What to Look for in the Summer Sky Your hosts of the summer sky are three bright stars — Vega, Altair and Deneb. Together they make up the Summer Triangle. Look for the triangle in the east on a June evening, moving NORTH to overhead as the season progresses. Polaris The Big Dipper Deneb Cygnus Vega Lyra Hercules Arcturus EaST West Summer Triangle Altair Aquila Sagittarius Antares Turn the map so Scorpius the direction you are facing is at the Teapot the bottom. south facebook.com/KidsCanBooks @KidsCanPress GET OUTSIDE Text © 2013 Jane Drake & Ann Love Illustrations © 2013 Heather Collins www.kidscanpress.com Get Outside Vega The Keystone The brightest star in the Between Vega and Arcturus, Summer Triangle, Vega is look for four stars in a wedge or The summer bluish white. It is in the keystone shape. This is the body solstice constellation Lyra, the Harp. of Hercules, the Strongman. His feet are to the north and Every day from late Altair his arms to the south, making December to June, the The second-brightest star in his figure kneel Sun rises and sets a little the triangle, Altair is white. upside down farther north along the Altair is in the constellation in the sky. horizon. But about June Aquila, the Eagle. 21, the Sun seems to stop Keystone moving north. It rises in Deneb the northeast and sets in The dimmest star of the the northwest, seemingly Summer Triangle, Deneb would in the same spots for be the brightest if it were not so Hercules several days. -
Survey of Britain's Most Powerful Radial Engine : an Example Of
JULY 5TH, 1945 FLIGHT Survey of Britain's Most Powerful Radial Engine : An Example of . r l^OgiCal Layout to Achieve Compactness with Power T has been eommbn knowledge far some time past that •power figure of 3,500, the b.h.p. /litre of both Hercules the Bristol Aeroplane Co., Ltd., have been engaged with Centaurus is 46.5, although we know that the latter engine the production of a larger and improved model in the is somewhat better than this, as may be rough!y indicated age of radial, air-cooled, sleeve-valve engines with which by the figures for b.h.p./sq. in. of piston area, these ey have for so long enhanced their reputation. This being respectively:. Hercules 4.93. and Centaurus better mmon knowledge—the result of unofficial "leaks"— than 5.34. • f ibraced the facts that the new engine was an 18-cylinder : Cooling Arrangements lit of over 2,000 h.p. and was called the Centaurug.. ther than this nothing much was generally known until As an indication of refinement in the design of the cowl- nctioned reference, to the engine was made with the ing, if. we take as a datum the frontal area of the Hercules lease of the Short Shetland flying boat (Flight, May 17th, at 2,122 sq. in. and give it the value of unity, then the 145), when it was revealed that the Centaurus was of Centaurus frontal area of 2,402 sq. in. gives a comparative 'er 2,500 h.p. ratio of 1.13:1, which is well below the relative h.p..ratio Even now we are not permitted to give any indication of 1.385 :1, itself a conservative figure. -
A Spectroscopic Atlas of Deneb (A2 Iae) $\Lambda\Lambda$3826–5212
A&A 400, 1043–1049 (2003) Astronomy DOI: 10.1051/0004-6361:20030014 & c ESO 2003 Astrophysics A spectroscopic atlas of Deneb (A2 Iae) λλ3826–5212? B. Albayrak1,A.F.Gulliver2,??,S.J.Adelman3,??, C. Aydın1,andD.Ko¸cer4 1 Ankara University, Science Faculty, Department of Astronomy and Space Sciences, 06100, Tando˘gan, Ankara, Turkey e-mail: [email protected]; [email protected] 2 Department of Physics and Astronomy, Brandon University, Brandon, MB, R7A 6A9, Canada e-mail: [email protected] 3 Department of Physics, The Citadel, 171 Moultrie Street, Charleston, SC 29409, USA e-mail: [email protected] 4 Istanbul˙ K¨ult¨ur University, Science & Art Faculty, Department of Mathematics, E5 Karayolu Uzeri,¨ 34510, S¸irinevler, Istanbul,˙ Turkey e-mail: [email protected] Received 2 December 2002 / Accepted 6 January 2003 Abstract. We present a spectroscopic atlas of Deneb (A2 Iae) obtained with the long camera of the 1.22-m telescope of the 1 Dominion Astrophysical Observatory using Reticon and CCD detectors. For λλ3826–5212 the inverse dispersion is 2.4 Å mm− with a resolution of 0.072 Å. At the continuum the mean signal-to-noise ratio is 1030. The wavelengths in the laboratory frame, the equivalent widths, and the identifications of the various spectral features are given. This atlas should provide useful guidance for studies of other stars with similar spectral types. The stellar and synthetic spectra with their corresponding line identifications can be examined at http://www.brandonu.ca/physics/gulliver/atlases.html Key words. atlases – stars: early type – stars: individual: Deneb – stars: supergiants 1. -
Newpointe-Catalog
NewPointe® Constellation Collections More value from Batesville Constellation Collections 18 Gauge Steel Caskets Leo Collection Leo Brushed Black Silver velvet interior Leo Brushed Black shown with Praying Hands decorative kit. 257178 - half couch Choose from 11 designs. 262411 - full couch See page 15 for your options. • Includes decorative kit option for lid Leo Painted Silver Silver velvet interior 257172 - half couch 262415 - full couch • Includes decorative kit option for lid Leo Brushed Ruby Leo Brushed Blue Leo Painted Sand Leo Painted White Moss Pink velvet interior Light Blue velvet interior Champagne velvet interior Moss Pink velvet interior 257177 - half couch 257179 - half couch 257173 - half couch 257166 - half couch 262410 - full couch 262412 - full couch 262416 - full couch 262414 - full couch • Includes decorative kit option • Includes decorative kit option • Includes decorative kit option • Includes decorative kit option for lid for lid for lid for lid 2 All caskets not available in all locations. Please check to ensure availability in your area. 18 Gauge Steel Caskets Virgo Collection Virgo White/Pink Moss Pink crepe interior| $845 250673 - half couch Virgo White/Pink shown with Roses 254258 - full couch decorative kit and corner decals. Choose from 11 designs. • Includes decorative kit option See page 15 for your options. for lid and corner decals Virgo Blue Light Blue crepe interior 250658 - half couch 254255 - full couch • Includes decorative kit option for lid and corner decals Virgo Silver Virgo White Virgo Copper -
Summer Constellations
Night Sky 101: Summer Constellations The Summer Triangle Photo Credit: Smoky Mountain Astronomical Society The Summer Triangle is made up of three bright stars—Altair, in the constellation Aquila (the eagle), Deneb in Cygnus (the swan), and Vega Lyra (the lyre, or harp). Also called “The Northern Cross” or “The Backbone of the Milky Way,” Cygnus is a horizontal cross of five bright stars. In very dark skies, Cygnus helps viewers find the Milky Way. Albireo, the last star in Cygnus’s tail, is actually made up of two stars (a binary star). The separate stars can be seen with a 30 power telescope. The Ring Nebula, part of the constellation Lyra, can also be seen with this magnification. In Japanese mythology, Vega, the celestial princess and goddess, fell in love Altair. Her father did not approve of Altair, since he was a mortal. They were forbidden from seeing each other. The two lovers were placed in the sky, where they were separated by the Celestial River, repre- sented by the Milky Way. According to the legend, once a year, a bridge of magpies form, rep- resented by Cygnus, to reunite the lovers. Photo credit: Unknown Scorpius Also called Scorpio, Scorpius is one of the 12 Zodiac constellations, which are used in reading horoscopes. Scorpius represents those born during October 23 to November 21. Scorpio is easy to spot in the summer sky. It is made up of a long string bright stars, which are visible in most lights, especially Antares, because of its distinctly red color. Antares is about 850 times bigger than our sun and is a red giant. -
CONSTELLATION VULPECULA, the (LITTLE) FOX Vulpecula Is a Faint Constellation in the Northern Sky
CONSTELLATION VULPECULA, THE (LITTLE) FOX Vulpecula is a faint constellation in the northern sky. Its name is Latin for "little fox", although it is commonly known simply as the fox. It was identified in the seventeenth century, and is located in the middle of the northern Summer Triangle (an asterism consisting of the bright stars Deneb in Cygnus (the Swan), Vega in Lyra (the Lyre) and Altair in Aquila (the Eagle). Vulpecula was introduced by the Polish astronomer Johannes Hevelius in the late 17th century. It is not associated with any figure in mythology. Hevelius originally named the constellation Vulpecula cum ansere, or Vulpecula et Anser, which means the little fox with the goose. The constellation was depicted as a fox holding a goose in its jaws. The stars were later separated to form two constellations, Anser and Vulpecula, and then merged back together into the present-day Vulpecula constellation. The goose was left out of the constellation’s name, but instead the brightest star, Alpha Vulpeculae, carries the name Anser. It is one of the seven constellations created by Hevelius. The fox and the goose shown as ‘Vulpec. & Anser’ on the Atlas Coelestis of John Flamsteed (1729). The Fox and Goose is a traditional pub name in Britain. STARS There are no stars brighter than 4th magnitude in this constellation. The brightest star is: Alpha Vulpeculae, a magnitude 4.44m red giant at a distance of 297 light-years. The star is an optical binary (separation of 413.7") that can be split using binoculars. The star also carries the traditional name Anser, which refers to the goose the little fox holds in its jaws. -
Spring Constellations Leo
Night Sky 101: Spring Constellations Leo Leo, the lion, is very recognizable by the head of the lion, which looks like a backwards question mark, and is commonly known as “the sickle.” Regulus, Leo’s brightest star, is also easy to pick out in most lights. The constellation is best seen in April and May, but rises after the Spring Equinox in March. Within the constellation, there are several spiral galaxies: M65, M66, M95, and M96. It is possible to fit M65 and M66 into the same view on a low powered telescope. In Greek mythology, Leo was the Nemean lion, who was completely impervious to bronze, steel and any kind of metal. As part of his 12 labors, Hercules was charged to fight the lion and killed him Photo Credit: Starry Night by strangling him. Hercules took the lion’s pelt as a prize and Leo, the lion, was placed in the stars to commemorate their fight. Virgo Virgo is best seen in the late spring and early summer, usually May to June. The bright star Arcturus, in the constellation Boötes, lines up with the Virgo’s brightest star Spica, which makes it easy to find. Within the constellation is the Virgo Galaxy Cluster, which is a conglomerate of thousands of unnamed galaxies. These galaxies are about 65 million light years away, and usually only appear as smudges in a telescope. Virgo, the maiden, is also known as Persephone, or the daughter of the Demeter. Hades, god of the Un- derworld, fell in love with Virgo and took her to the Underworld. -
SEPTEMBER 2014 OT H E D Ebn V E R S E R V ESEPTEMBERR 2014
THE DENVER OBSERVER SEPTEMBER 2014 OT h e D eBn v e r S E R V ESEPTEMBERR 2014 FROM THE INSIDE LOOKING OUT Calendar Taken on July 25th in San Luis State Park near the Great Sand Dunes in Colorado, Jeff made this image of the Milky Way during an overnight camping stop on the way to Santa Fe, NM. It was taken with a Canon 2............................. First quarter moon 60D camera, an EFS 15-85 lens, using an iOptron SkyTracker. It is a single frame, with no stacking or dark/ 8.......................................... Full moon bias frames, at ISO 1600 for two minutes. Visible in this south-facing photograph is Sagittarius, and the 14............ Aldebaran 1.4˚ south of moon Dark Horse Nebula inside of the Milky Way. He processed the image in Adobe Lightroom. Image © Jeff Tropeano 15............................ Last quarter moon 22........................... Autumnal Equinox 24........................................ New moon Inside the Observer SEPTEMBER SKIES by Dennis Cochran ygnus the Swan dives onto center stage this other famous deep-sky object is the Veil Nebula, President’s Message....................... 2 C month, almost overhead. Leading the descent also known as the Cygnus Loop, a supernova rem- is the nose of the swan, the star known as nant so large that its separate arcs were known Society Directory.......................... 2 Albireo, a beautiful multi-colored double. One and named before it was found to be one wide Schedule of Events......................... 2 wonders if Albireo has any planets from which to wisp that came out of a single star. The Veil is see the pair up-close. -
Constellation at Your Fingertips: Cygnus
The National Optical Astronomy Observatory’s Dark Skies and Energy Education Program Constellation at Your Fingertips: Cygnus (Cygnus version adapted from Constellation at Your Fingertips: Orion at www.globeatnight.org) Grades: 3rd - 8th grade Overview: Constellation at Your Fingertips introduces the novice constellation hunter to a method for spotting the main stars in the constellation, Cygnus, the swan. Students will make an outline of the constellation used to locate the stars in Cygnus and visualize its shape. This lesson will engage children and first-time night sky viewers in observations of the night sky. The lesson links history, Greek mythology, literature, and astronomy. Once the constellation is identified, it may be easy to find the summer triangle. The simplicity of Cygnus makes locating and observing it exciting for young learners. More on Cygnus is at the Great World Wide Star Count at http://www.starcount.org. Materials for another citizen-science star hunt, Globe at Night, are available at http://www.globeatnight.org. Purpose: Students will use the this activity to visualize the constellation of Cygnus. This will help them more easily participate in the Great World Wide Star Count citizen-science campaign. The campaign asks participants to match one of 7 different charts of Cygnus with what the participant sees toward Cygnus. Chart 1 has only a few stars. Chart 7 has many. What they will be recording for the campaign is the chart with the faintest star they see. In many cases, observations over years will build knowledge of how light pollution changes over time. Why is this important to astronomers? What causes the variation year to year? The focus is on light pollution and the options we have as consumers when purchasing outdoor lighting and shields. -
The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 a Good Way to Start – Find North
The expression "dog days" refers to the period from July 3 through Aug. 11 when our brightest night star, SIRIUS (aka the dog star), rises in conjunction* with the sun. Conjunction, in astronomy, is defined as the apparent meeting or passing of two celestial bodies. TAAS Fabulous Fifty A program for those new to astronomy Friday Evening, July 20, 2018, 8:00 pm All TAAS and other new and not so new astronomers are welcome. What is the TAAS Fabulous 50 Program? It is a set of 4 meetings spread across a calendar year in which a beginner to astronomy learns to locate 50 of the most prominent night sky objects visible to the naked eye. These include stars, constellations, asterisms, and Messier objects. Methodology 1. Meeting dates for each season in year 2018 Winter Jan 19 Spring Apr 20 Summer Jul 20 Fall Oct 19 2. Locate the brightest and easiest to observe stars and associated constellations 3. Add new prominent constellations for each season Tonight’s Schedule 8:00 pm – We meet inside for a slide presentation overview of the Summer sky. 8:40 pm – View night sky outside The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 A Good Way to Start – Find North Polaris North Star Polaris is about the 50th brightest star. It appears isolated making it easy to identify. Circumpolar Stars Polaris Horizon Line Albuquerque -- 35° N Circumpolar Stars Capella the Goat Star AS THE WORLD TURNS The Circle of Perpetual Apparition for Albuquerque Deneb 1 URSA MINOR 2 3 2 URSA MAJOR & Vega BIG DIPPER 1 3 Draco 4 Camelopardalis 6 4 Deneb 5 CASSIOPEIA 5 6 Cepheus Capella the Goat Star 2 3 1 Draco Ursa Minor Ursa Major 6 Camelopardalis 4 Cassiopeia 5 Cepheus Clock and Calendar A single map of the stars can show the places of the stars at different hours and months of the year in consequence of the earth’s two primary movements: Daily Clock The rotation of the earth on it's own axis amounts to 360 degrees in 24 hours, or 15 degrees per hour (360/24). -
Detection and Characterization of Hot Subdwarf Companions of Massive Stars Luqian Wang
Georgia State University ScholarWorks @ Georgia State University Physics and Astronomy Dissertations Department of Physics and Astronomy 8-13-2019 Detection And Characterization Of Hot Subdwarf Companions Of Massive Stars Luqian Wang Follow this and additional works at: https://scholarworks.gsu.edu/phy_astr_diss Recommended Citation Wang, Luqian, "Detection And Characterization Of Hot Subdwarf Companions Of Massive Stars." Dissertation, Georgia State University, 2019. https://scholarworks.gsu.edu/phy_astr_diss/119 This Dissertation is brought to you for free and open access by the Department of Physics and Astronomy at ScholarWorks @ Georgia State University. It has been accepted for inclusion in Physics and Astronomy Dissertations by an authorized administrator of ScholarWorks @ Georgia State University. For more information, please contact [email protected]. DETECTION AND CHARACTERIZATION OF HOT SUBDWARF COMPANIONS OF MASSIVE STARS by LUQIAN WANG Under the Direction of Douglas R. Gies, PhD ABSTRACT Massive stars are born in close binaries, and in the course of their evolution, the initially more massive star will grow and begin to transfer mass and angular momentum to the gainer star. The mass donor star will be stripped of its outer envelope, and it will end up as a faint, hot subdwarf star. Here I present a search for the subdwarf stars in Be binary systems using the International Ultraviolet Explorer. Through spectroscopic analysis, I detected the subdwarf star in HR 2142 and 60 Cyg. Further analysis led to the discovery of an additional 12 Be and subdwarf candidate systems. I also investigated the EL CVn binary system, which is the prototype of class of eclipsing binaries that consist of an A- or F-type main sequence star and a low mass subdwarf.