... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...

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• ESO - The European ELT
• ALMA and the Large and Small Magellanic Clouds

. Space Telescope Science Institute . Cycle 20 Phase II Proposal Instructions . HST Phase II Proposal Instructions for Cycle 20 > Chapter 5: Visits, Exposures and Exposure Groups > 5.6 Exposure Number [Exposure_Number] . 5.6 Exposure Number [Exposure_Number] . APT will assign a unique integer number to an exposure. The smallest exposure number permitted is 1 , and the largest is 999 . Note that exposure numbers for coordinated parallels must (and will be) sequential; see Section 6.3 on page 105 .

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• A Quantitative Comparison of the Small Magellanic Cloud, Large Magellanic
• A Population of Accreted Small Magellanic Cloud Stars in the Large Magellanic
• Introduction to Patterns

... 2009 June 3 . VB 10: A Large Planet Orbiting a Small Star . Illustration Credit: JPL-Caltech , NASA . Explanation: Can a planet be as large as the star that it orbits? Recent observations have discovered that nearby Van Biesbroeck's star might have just such a large planet. ... Since faint M-type stars like VB 10 are so common, planetary system s surrounding them, including planets larger than their parent star, might be more common than planetary systems like our own Solar System . ...

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• APOD: February 16, 1999 - The Large and Small of M87
• Sternberg Astronomical Institute
• APOD: April 25, 1999 - Mimas: Small Moon with a Big Crater

... VB 10: A Large Planet Orbiting a Small Star . ... Credit: JPL-Caltech , NASA Explanation: Can a planet be as large as the star that it orbits? Recent observations have discovered that nearby Van Biesbroeck's star might have just such a large planet. ... Since faint M-type stars like VB 10 are so common, planetary system s surrounding them, including planets larger than their parent star, might be more common than planetary systems like our own Solar System . ... NASA Official: Jay Norris. ...

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• The Large and Small of M87
• Астронет > The Large and Small of M87
• Астронет > VB 10: A Large Planet Orbiting a Small Star

Next: *imcopy* - Compress an Up: Image Manipulation Previous: Image Manipulation . input file: rp90_a.imh . ... xr> images # need this package im> imcopy rp90_a[200:263,282:345] rp90_aa # extract 64x64 region from .imh file rp90_a[200:263,282:345]-->rp90_aa . ... As an example we make an input file for the smoothing task which needs small arrays or it takes too long to run. im> imcopy xdata$rp110590.qp[6830:7029,9290:9489] rp90_ab.imh # extract 200x200 region from the .qp file . ...

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• To compress and display a large (e.g. ROSAT) image
• Are smaller wheels faster?

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... HI in Elliptical Galaxies . ... Next Section: HI in small elliptical . ... Several properties of elliptical galaxies appear to change at an absolute magnitude around M Large elliptical galaxies (defined here as those with M brighter than -19) are usually dominated by an old stellar population (e.g. Bressan et al. 1996), and have most of their gas in a hot X-ray corona (Forman et al. ...

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• Small_scope_radio_jove
• ATNF Colloquium
• ALFA Images

M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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• Towards 1800
• Formation of the Earth

Storing and accessing the largest astronomical catalogues with the SAI CAS project S. Koposov1,2,3, O. Bartunov2, S. Karpov4 et al2. ... Why we want to build our own Catalogue Access Service The requirements for our CAS system The importance of the Database for the CAS (PostgreSQL & Q3C) The technical realization of CAS What has been already done Example of work TODO Storing and Accessing Astronomical Catalogues Existing projects CDS OpenSkyQuery CASjobs with SDSS They are all really great! ...

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... Earth is the tiny spot between Jupiter and the Sun). ... Distance Radius Mass Name Orbits (000 km) (km) (kg) --------- ------- -------- ------- ------- Sun 697000 1.99e30 Jupiter Sun 778000 71492 1.90e27 Saturn Sun 1429000 60268 5.69e26 Uranus Sun 2870990 25559 8.69e25 * Neptune Sun 4504300 24764 1.02e26 * Earth Sun 149600 6378 5.98e24 Venus Sun 108200 6052 4.87e24 Mars Sun 227940 3398 6.42e23 Ganymede Jupiter 1070 2631 1.48e23 + Titan ... Extrema .. ...

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• SmallBodies in the Solar System
• Titania
• Neptune

... The three optical trains for the cameras, and the pupil reimaging system, are mounted on a wheel, accurately driven by an external motor. ... The low-resolution spectroscopic mode uses the wide field camera and a suitable set of grisms and order sorting filters that are inserted in the parallel beam after the pupil. ... One of the five grisms can operate at four different orders, depending on the filter selected on the first filter wheel that acts as order sorter. ...

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• A collection of images
• Hubble Finds Ozone on Jupiter's Moon Ganymede
• Problem Getting the Kernel small enough

... Telescopes . ... The time requests are accepted in an electronic version with on-line form in Russian or English. ... Unregistered request will be disregarded by the Large Telescopes Programm Committee. In exclusive cases the secreatry of the Committee is entitled to accept an observational time request given permission of the Chairman of the Committee or the director of the SAO RAS. The Program Committee considers generally one time request submitted by the principal applicant. ...

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• The Present and Future of Small and Medium Size Telescopes
• Metagalaxy sector, archive 2011
• Small telescopes short description

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

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• Starobinsky
• The X-ray Optics
• Massive X-ray Binaries

... The lava flow has visibly fewer impact craters than the background terrain, illustrating the general principle that crater numbers can reveal ages of surfaces. ... Dating Small Martian Features . ... The crater-counting system that scientists have used since the 1970s to determine the age of large geologic features on Mars will also allow them to date small features, such as riverbeds and lava flows, according to William K. Hartmann, a senior scientist at the Tucson-based Planetary Science Institute...

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• ASP: Eclipse Watching: Making a Solar Filter
• ASP: A Good Definition of the Word "Planet": Mission Impossible?
• ASP: The New and Improved Hubble Space Telescope

... Tonight's Sky . ... The Magazine . ... Observing . ... Magazine . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... large (8 inches or larger) . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ... Astronomy Magazine . ...

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• small (4 inches or smaller) | Astronomy.com
• How often does a large meteroid hit the Moon? Can I see such an impact? |
• very large telescope | Astronomy.com

Next: Calling Parameters Up: CAL_rgsGetScatter Previous: CAL_rgsGetScatter Contents . ... is the r.m.s. surface roughness for two scatter models; is either small or large for small angle scatter, and large angle scatter, respectively. ... Note that the surface roughness for the large angle scatter is parameterized as a function of wavelength and its value is obtained with . ... The fraction of scattered light for small/large angle scatter is . ... This is not performed by this function. ...

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• Home Page
• Array or vector scalar integers

... Formation of large-scale inhomogeneous magnetic structures in a turbulent convection". ... Magnetic fluctuations generated by a tangling of the mean magnetic field by velocity fluctuations are studied in a developed turbulent convection with large magnetic Reynolds numbers. ... This effect is caused by a negative contribution of the turbulent convection to the effective mean Lorentz force. ... The energy for this instability is supplied by the small-scale turbulent convection. ...

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• The Io Dynamo
• Creation of Space transportation system on the base of large length rope

... Title: Neutron Star Structure and Equation of State . ... Matter at supra-nuclear densities, while inaccessible in the laboratory, exists in abundance in the nearly 2000 neutron stars detected so far by radio surveys. ... Title: Studying Complex and Pre-biotic Molecules in the ISM using the Arecibo Observatory . ... 100 K) molecular gas, radio observations are important for studying the cold gas where complex molecules only show low-energy transitions with frequencies of less than about 12 GHz. ...

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• H I Midplane Poster for the 201st Meeting of the AAS, January, 2003
• Frontiers of Astronomy with the World's Largest Radio Telescope Frontiers of
• drift maps in J2000 coordinates

Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...

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• ASC home page

... 8, ``Celestial Mechanics'', 2002 Formation and migration of trans -- Neptunian objects S. I. Ipatov 1;2 1 Institute of Applied Mathematics, Moscow, Russia 2 NASA/GSFC, Greenbelt, USA We support the Eneev's idea [1] that the largest (with diameter d?100 km) trans ­ Neptunian objects ( TNOs ) moving now in not very eccentric orbits ... The total amount of water delivered to the Earth during the formation of the giant planets was about the mass of water in the Earth's oceans. ...

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• Keywords_312
• Keywords_327
• Keywords_196

... Previous: Multi-threaded Query Agent and Engine for a Very Large Astronomical Database . ... Dedicated tools have been developed at CDS in order to face the challenge of fast on-line access to very large astronomical catalogues. ... When a query to such a large catalogue is submitted to VizieR , the CDS database of catalogues and tables (Ochsenbein et al. 2000), a dedicated program handles the request, extracts and decodes the matching data, and sends its output back to VizieR. ... 1990, Russel et...

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• ADASS 2002 Conference Proceedings
• Methods for Structuring and Searching Very Large Catalogs
• Preface