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Where Are the Distant Worlds? Star Maps
W here Are the Distant Worlds? Star Maps Abo ut the Activity Whe re are the distant worlds in the night sky? Use a star map to find constellations and to identify stars with extrasolar planets. (Northern Hemisphere only, naked eye) Topics Covered • How to find Constellations • Where we have found planets around other stars Participants Adults, teens, families with children 8 years and up If a school/youth group, 10 years and older 1 to 4 participants per map Materials Needed Location and Timing • Current month's Star Map for the Use this activity at a star party on a public (included) dark, clear night. Timing depends only • At least one set Planetary on how long you want to observe. Postcards with Key (included) • A small (red) flashlight • (Optional) Print list of Visible Stars with Planets (included) Included in This Packet Page Detailed Activity Description 2 Helpful Hints 4 Background Information 5 Planetary Postcards 7 Key Planetary Postcards 9 Star Maps 20 Visible Stars With Planets 33 © 2008 Astronomical Society of the Pacific www.astrosociety.org Copies for educational purposes are permitted. Additional astronomy activities can be found here: http://nightsky.jpl.nasa.gov Detailed Activity Description Leader’s Role Participants’ Roles (Anticipated) Introduction: To Ask: Who has heard that scientists have found planets around stars other than our own Sun? How many of these stars might you think have been found? Anyone ever see a star that has planets around it? (our own Sun, some may know of other stars) We can’t see the planets around other stars, but we can see the star. -
The Denver Observer June 2016
The Denver JUNE 2016 OBSERVER Mercury transits the Sun on May 9, 2016. The planet, seen at the lower left of the Sun's face, has a diameter of about 3,000 miles, but the Sun's 870,000 mile cross-section dwarfs the planet—even though the Sun is seen here at twice Mercury's distance from us. (Note the planet-sized sunspots above-left of solar center.) Image © Ron Pearson. JUNE SKIES by Zachary Singer The Solar System the Martian surface reveals itself. On observing runs over the last few If you haven’t been observing Mars, the “unusually bright orange weeks, with good seeing, early views did indeed yield so-so results, but object in Libra,” now is a really good time: As June begins, the plan- improved noticeably as the planet neared its highest point in the south. et is just past opposition, and even more recently past its closest ap- I was able to make out the Syrtis Major region easily, even though proach to Earth, when the planet’s disk spanned a full 18.6 arcseconds. moonlight was a factor in the initial sessions. It looms large in a telescope now, and even instruments of moderate One great tool for power bring satisfying images at 100 or 150X. By midmonth, Mars improving your view Sky Calendar will be highest around 11 PM, with the disk slightly smaller, at 17.9”; is a “Moon filter.” 4 New Moon by June 30th, though, the planet will have already crossed the Meridian By bringing the sheer 12 First-Quarter Moon at 10 PM, before the sky brightness of Mars’ mag- 20 Full Moon In the Observer is fully dark, and the disk nitude -2 disk down a 27 Last-Quarter Moon will have shrunk some- notch, the moon filter President’s Message . -
Stark Broadening of Spectral Lines in Plasmas
atoms Stark Broadening of Spectral Lines in Plasmas Edited by Eugene Oks Printed Edition of the Special Issue Published in Atoms www.mdpi.com/journal/atoms Stark Broadening of Spectral Lines in Plasmas Stark Broadening of Spectral Lines in Plasmas Special Issue Editor Eugene Oks MDPI • Basel • Beijing • Wuhan • Barcelona • Belgrade Special Issue Editor Eugene Oks Auburn University USA Editorial Office MDPI St. Alban-Anlage 66 4052 Basel, Switzerland This is a reprint of articles from the Special Issue published online in the open access journal Atoms (ISSN 2218-2004) in 2018 (available at: https://www.mdpi.com/journal/atoms/special issues/ stark broadening plasmas) For citation purposes, cite each article independently as indicated on the article page online and as indicated below: LastName, A.A.; LastName, B.B.; LastName, C.C. Article Title. Journal Name Year, Article Number, Page Range. ISBN 978-3-03897-455-0 (Pbk) ISBN 978-3-03897-456-7 (PDF) Cover image courtesy of Eugene Oks. c 2018 by the authors. Articles in this book are Open Access and distributed under the Creative Commons Attribution (CC BY) license, which allows users to download, copy and build upon published articles, as long as the author and publisher are properly credited, which ensures maximum dissemination and a wider impact of our publications. The book as a whole is distributed by MDPI under the terms and conditions of the Creative Commons license CC BY-NC-ND. Contents About the Special Issue Editor ...................................... vii Preface to ”Stark Broadening of Spectral Lines in Plasmas” ..................... ix Eugene Oks Review of Recent Advances in the Analytical Theory of Stark Broadening of Hydrogenic Spectral Lines in Plasmas: Applications to Laboratory Discharges and Astrophysical Objects Reprinted from: Atoms 2018, 6, 50, doi:10.3390/atoms6030050 ................... -
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. -
CONSTELLATION BOÖTES, the HERDSMAN Boötes Is the Cultivator Or Ploughman Who Drives the Bears, Ursa Major and Ursa Minor Around the Pole Star Polaris
CONSTELLATION BOÖTES, THE HERDSMAN Boötes is the cultivator or Ploughman who drives the Bears, Ursa Major and Ursa Minor around the Pole Star Polaris. The bears, tied to the Polar Axis, are pulling a plough behind them, tilling the heavenly fields "in order that the rotations of the heavens should never cease". It is said that Boötes invented the plough to enable mankind to better till the ground and as such, perhaps, immortalizes the transition from a nomadic life to settled agriculture in the ancient world. This pleased Ceres, the Goddess of Agriculture, so much that she asked Jupiter to place Boötes amongst the stars as a token of gratitude. Boötes was first catalogued by the Greek astronomer Ptolemy in the 2nd century and is home to Arcturus, the third individual brightest star in the night sky, after Sirius in Canis Major and Canopus in Carina constellation. It is a constellation of large extent, stretching from Draco to Virgo, nearly 50° in declination, and 30° in right ascension, and contains 85 naked-eye stars according to Argelander. The constellation exhibits better than most constellations the character assigned to it. One can readily picture to one's self the figure of a Herdsman with upraised arm driving the Greater Bear before him. FACTS, LOCATION & MAP • The neighbouring constellations are Canes Venatici, Coma Berenices, Corona Borealis, Draco, Hercules, Serpens Caput, Virgo, and Ursa Major. • Boötes has 10 stars with known planets and does not contain any Messier objects. • The brightest star in the constellation is Arcturus, Alpha Boötis, which is also the third brightest star in the night sky. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
A Code to Measure Stellar Atmospheric Parameters and Their Covariance from Spectra
MNRAS 467, 971–984 (2017) doi:10.1093/mnras/stx144 Advance Access publication 2017 January 19 ZASPE: a code to measure stellar atmospheric parameters and their covariance from spectra Rafael Brahm,1,2‹ Andres´ Jordan,´ 1,2 Joel Hartman3 and Gasp´ ar´ Bakos3†‡ 1 Instituto de Astrof´ısica, Facultad de F´ısica, Pontificia Universidad Catolica´ de Chile, Av. Vicuna˜ Mackenna 4860, 7820436 Macul, Santiago, Chile Downloaded from https://academic.oup.com/mnras/article-abstract/467/1/971/2929275 by Princeton University user on 28 November 2018 2Millennium Institute of Astrophysics, Santiago, Chile 3Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA Accepted 2017 January 17. Received 2017 January 13; in original form 2015 December 7 ABSTRACT We describe the Zonal Atmospheric Stellar Parameters Estimator (ZASPE), a new algorithm, and its associated code, for determining precise stellar atmospheric parameters and their uncertainties from high-resolution echelle spectra of FGK-type stars. ZASPE estimates stellar atmospheric parameters by comparing the observed spectrum against a grid of synthetic spectra only in the most sensitive spectral zones to changes in the atmospheric parameters. Realistic uncertainties in the parameters are computed from the data itself, by taking into account the systematic mismatches between the observed spectrum and the best-fitting synthetic one. The covariances between the parameters are also estimated in the process. ZASPE can in principle use any pre-calculated grid of synthetic spectra, but unbiased grids are required to obtain accurate parameters. We tested the performance of two existing libraries, and we concluded that neither is suitable for computing precise atmospheric parameters. -
Long Delayed Echo: New Approach to the Problem
Geometrical joke(r?)s for SETI. R. T. Faizullin OmSTU, Omsk, Russia Since the beginning of radio era long delayed echoes (LDE) were traced. They are the most likely candidates for extraterrestrial communication, the so-called "paradox of Stormer" or "world echo". By LDE we mean a radio signal with a very long delay time and abnormally low energy loss. Unlike the well-known echoes of the delay in 1/7 seconds, the mechanism of which have long been resolved, the delay of radio signals in a second, ten seconds or even minutes is one of the most ancient and intriguing mysteries of physics of the ionosphere. Nowadays it is difficult to imagine that at the beginning of the century any registered echo signal was treated as extraterrestrial communication: “Notable changes occurred at a fixed time and the analogy among the changes and numbers was so clear, that I could not provide any plausible explanation. I'm familiar with natural electrical interference caused by the activity of the Sun, northern lights and telluric currents, but I was sure, as it is possible to be sure in anything, that the interference was not caused by any of common reason. Only after a while it came to me, that the observed interference may occur as the result of conscious activities. I'm overwhelmed by the the feeling, that I may be the first men to hear greetings transmitted from one planet to the other... Despite the signal being weak and unclear it made me certain that soon people, as one, will direct their eyes full of hope and affection towards the sky, overwhelmed by good news: People! We got the message from an unknown and distant planet. -
Harappan Astronomy
In Nakamura, T., Orchiston, W., Sôma, M., and Strom, R. (eds.), 2011. Mapping the Oriental Sky. Proceedings of the Seventh International Conference on Oriental Astronomy. Tokyo, National Astronomical Observatory of Japan. Pp. xx-xx. THEORETICAL FRAMEWORK OF HARAPPAN ASTRONOMY Mayank N. VAHIA Tata Institute of Fundamental Research, Mumbai, India and Manipal Advanced Research Group, Manipal University, Manipal – 576104, Karnataka, India. E-mail: [email protected] and Srikumar M. MENON Faculty of Architecture, Manipal Institite of Technology, Manipal – 576104, Karnataka, India. E-mail: [email protected] Abstract: Archaeo astronomy normally consists of interpreting available data and archaeological evidence about the astronomical knowledge of a civilisation. In the present study, we attempt to „reverse engineer‟ and attempt to define the nature of astronomy of a civilisation based on other evidence of its cultural complexity. We then compare it with somewhat sketchy data available so far and suggest the possible manner in which their observatories can be identified. 1 INTRODUCTION The Harappan civilisation lasted from about 7,000 BC to 2,000 BC. At its peak it spread over an area of more than a million square kilometres, and boasted more than 5,000 rural centres, over a dozen which had population densities >3 per m2 (Kenoyer, 1998, Possehl, 2002, Agarwal, 2007, Wright 2010). Harappan culture evolved and merged and transformed over this period (Gangal et al., 2011), and it also went through a complex evolutionary pattern (Vahia and Yadav, 2011a). It was the most advanced pre- iron civilisation in the world. It is no surprise, therefore, that the Harappans had a vibrant intellectual tradition. -
Readingsample
Stellar Physics 2: Stellar Evolution and Stability Bearbeitet von Gennady S. Bisnovatyi-Kogan, A.Y. Blinov, M. Romanova 1. Auflage 2011. Buch. xxii, 494 S. Hardcover ISBN 978 3 642 14733 3 Format (B x L): 15,5 x 23,5 cm Gewicht: 1024 g Weitere Fachgebiete > Physik, Astronomie > Astronomie: Allgemeines > Astrophysik Zu Inhaltsverzeichnis schnell und portofrei erhältlich bei Die Online-Fachbuchhandlung beck-shop.de ist spezialisiert auf Fachbücher, insbesondere Recht, Steuern und Wirtschaft. Im Sortiment finden Sie alle Medien (Bücher, Zeitschriften, CDs, eBooks, etc.) aller Verlage. Ergänzt wird das Programm durch Services wie Neuerscheinungsdienst oder Zusammenstellungen von Büchern zu Sonderpreisen. Der Shop führt mehr als 8 Millionen Produkte. Chapter 8 Pre-Main Sequence Evolution As can be seen from the calculations of cloud collapse described in Sect. 7.2,stars with mass M>3Mˇ appear in the optical range immediately near to the main se- quence. Objects of lower mass exist for part of the time as optical stars with radiation due to gravitational contraction energy. Consider evolution of a star from its ap- pearance in the optical region until it reaches the main sequence, and its central temperature becomes sufficiently high to initiate a nuclear reaction converting hy- drogen into helium (see review [105]). 8.1 Hayashi Phase The pre-main sequence evolution of stars takes place at not very high temperatures, when a non-full ionization of matter and large opacity cause such stars to be almost convective. This fact was first established by Hayashi [461, 462], who took into account a convection in constructing evolutionary tracks for contracting stars in the HR diagram (see Fig. -
Brightness Profiles of Early-Type Galaxies Hosting Seyfert Nuclei
A&A 469, 75–88 (2007) Astronomy DOI: 10.1051/0004-6361:20066684 & c ESO 2007 Astrophysics The host galaxy/AGN connection Brightness profiles of early-type galaxies hosting Seyfert nuclei A. Capetti and B. Balmaverde INAF - Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy e-mail: [capetti;balmaverde]@oato.inaf.it Received 2 November 2006 / Accepted 15 March 2007 ABSTRACT We recently presented evidence of a connection between the brightness profiles of nearby early-type galaxies and the properties of the AGN they host. The radio loudness of the AGN appears to be univocally related to the host’s brightness profile: radio-loud nuclei are only hosted by “core” galaxies while radio-quiet AGN are only found in “power-law” galaxies. We extend our analysis here to a −1 sample of 42 nearby (Vrec < 7000 km s ) Seyfert galaxies hosted by early-type galaxies. From the nuclear point of view, they show a large deficit of radio emission (at a given X-ray or narrow line luminosity) with respect to radio-loud AGN, conforming with their identification as radio-quiet AGN. We used the available HST images to study their brightness profiles. Having excluded complex and highly nucleated galaxies, in the remaining 16 objects the brightness profiles can be successfully modeled with a Nuker law with a steep nuclear cusp characteristic of “power-law” galaxies (with logarithmic slope γ = 0.51−1.07). This result is what is expected for these radio-quiet AGN based on our previous findings, thus extending the validity of the connection between brightness profile and radio loudness to AGN of a far higher luminosity. -
Snake River Skies the Newsletter of the Magic Valley Astronomical Society
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting MVAS President’s Message June 2018 Saturday, June 9th 2018 7:00pm at the Toward the end of last month I gave two presentations to two very different groups. Herrett Center for Arts & Science College of Southern Idaho. One was at the Sawtooth Botanical Gardens in their central meeting room and covered the spring constellations plus some simple setups for astrophotography. Public Star Party Follows at the The other was for the Sun Valley Company and was a telescope viewing session Centennial Observatory given on the lawn near the outdoor pavilion. The composition of the two groups couldn’t be more different and yet their queries and interests were almost identical. Club Officers Both audiences were genuinely curious about the universe and their questions covered a wide range of topics. How old is the moon? What is a star made of? Tim Frazier, President How many exoplanets are there? And, of course, the big one: Is there life out [email protected] there? Robert Mayer, Vice President The SBG’s observing session was rained out but the skies did clear for the Sun [email protected] Valley presentation. As the SV guests viewed the moon and Jupiter, I answered their questions and pointed out how one of Jupiter’s moons was disappearing Gary Leavitt, Secretary behind the planet and how the mountains on our moon were casting shadows into [email protected] the craters. Regardless of their age, everyone was surprised at the details they 208-731-7476 could see and many expressed their amazement at what was “out there”.