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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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Risks Comparable to NEOs . ... The Increasing Rate of Discovery of Asteroids . ... Comet and Asteroid Collision Probabilities . ... Extreme albedo comets and the impact hazard (PDF Format) . ... Asteroid Impact Animations . ... Workshop on Scientific Requirements for Mitigation of Hazardous Comets and Asteroids - 2002 . ... The Spaceguard Survey Report, 1992 (PDF) . Tsunami from Asteroid/Comet Impacts . ...

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• Armagh Observatory Small Asteroids
• Solar System Research

... We can help students grasp the significance of Hubble's extremely keen eye, and learn a bit about angles and math in the process, with the following in-class activity. ... Looking through binoculars or telescopes allows us to magnify a small section of the sky. To measure sizes or distances in that small section, astronomers divide a degree into 60 smaller pieces called arcminutes, and further subdivide minutes into 60 smaller sections called arcseconds. ... 30 feet = . ... 36 seconds . ...

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• ASP: A Good Definition of the Word "Planet": Mission Impossible?
• ASP: Making Your Own Astronomical Camera
• ASP: More About Deep Space Objects and Cosmic Terms

... Because of the difficulties of working with and communicating with a satellite in low-earth orbit, and in order to make HST more efficient, virtually all actions taken by the spacecraft are planned weeks in advance. Only a small fraction of HST's time can be used for real-time actions that are at the discretion of the observer, and even then the only possible action is deciding which object in the field should be centered in the aperture before a subsequent observation is begun. ...

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• Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
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... ESO, the European Southern Observatory . ... ESO's Governing Bodies . ... Travel and Contacts . Travel to ESO Headquarters . ... ESO . ... Survey Telescopes . ... ESO 3.6-metre telescope . ... MPG/ESO 2.2-metre telescope . ... ESO 1-metre Schmidt telescope . ... The oddly shaped Pencil Nebula (NGC 2736) is pictured in this image from ESOтАЩs La Silla Observatory in Chile. This nebula is a small part of a huge remnant left over after a supernova explosion that took place about 11 000 years ago. ...

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• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
• First Rotation Period of Kuiper Belt Object Measured (ESO PR Photo 41/98)
• Detailed view of the Prawn Nebula from ESO's VST | ESO

... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...

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• Laboratory of spectroscopy and photometry of extragalactic objects : Devices
• Laboratory of spectroscopy and photometry of extragalactic objects :MOUSER
• Search for distant radio galaxies in SAO

... Click on an object in the solar system or choose from the list at left to learn more . The Arecibo Observatory planetary radar is the world's most powerful instrument for post-discovery characterization and orbital refinement of near-Earth objects. ... The Solar System Studies group is a department of the Arecibo Observatory, which is an NSF facility operated under cooperative agreement by SRI International, Universities Space Research Association (USRA), and la Universidad Metropolitana (UMET). ...

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• radioastron
• Using the Parkes Multibeam to search for HVC Analogs
• Simulations of 3 ALFA Surveys

In 1950 Jan Oort noticed that . no comet has been observed with an orbit that indicates that it came from interstellar space, . ... From this he proposed that comets reside in a vast cloud at the outer reaches of the solar system. ... Unfortunately, since the individual comets are so small and at such large distances, we have no direct evidence about the Oort Cloud. ... Its orbit is intermediate between the Kuiper Belt and what was previously thought to be the inner part of the Oort Cloud. ...

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• SAI Supernova catalog
• APOD: November 20, 1999 - Small Star
• APOD: June 5, 1997 - Small Star

... no comet has been observed with an orbit that indicates that it came from interstellar space, . ... From this he proposed that comets reside in a vast cloud at the outer reaches of the solar system. ... Unfortunately, since the individual comets are so small and at such large distances, we have no direct evidence about the Oort Cloud. ... T he Kuiper Belt is a disk-shaped region past the orbit of Neptune roughly 30 to 100 AU from the Sun containing many small icy bodies. ... Small Bodies .. ...

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• Parallax
• Astronomical Names
• Introduction to The Nine Planets

Next: ZGSC (Compressed GSC) and XSKYMAP . ... This is a preliminary report on an investigation of the quality and properties of plates digitized during creation of the Guide Star Catalog (GSC). The results will be vital for reclassifying GSC objects. ... Many objects are measured on more than one plate, and thus have multiple catalog entries. ... Among the shortcomings of the GSC are: biased magnitudes and incorrect classifications for certain objects, presence of artifact objects. ...

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• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
• TransVERSE: An Architecture for Configuring Astronomical Observations
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of

As a service to the astronomical community, we are recalibrating all archival Hubble Space Telescope Faint Object Spectrograph UV and optical spectrophotometry of active galaxies and quasars in order to extract uniformly calibrated spectrophotometric data for further detailed scientific investigations. ... NGC 4151 CLOUD F . NGC 5548 . ... NGC 4395 . ... NGC 4486 . ... NGC 4486 JET KNOT-A . ... NGC 4486 CLOUD-A . ... NGC 3031 . ... NGC 1068 . ... NGC 1068 CLOUD A . ... 1413+117A . ... NGC 4151 . ...

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• The AstroStat Slog Blog Archive [ArXiv] A fast Bayesian object detection
• Very Low Mass PMS Objects
• Source Selection

... Angular size depends on distance, the farther away an object is, the smaller an angle it covers. ... SDSSJ1430: A Galaxy Einstein Ring . ... IC 4406: A Seemingly Square Nebula . ... These detailed Hubble Space Telescope close-ups feature Jupiter's ancient swirling storm system known as the Great Red Spot. They also follow the progress of two newer storm systems that have grown to take on a similar reddish hue: the smaller "Red Spot Jr." (bottom), and smaller still, a "baby red spot". ...

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• Moon Games

Shakht N.A., A.A.Afanas'eva, D.L. Gorshanov, E. V.Poliakow (Pulkovo Observatory, Russia): Title: Long-term photographic observations for selected objects of Pulkovo program: measurements and results. Abstract: The selected objects, observed at Pulkovo observatory during long time period have been of intense interest among astronomers, and now they are the most important aims for space investigations. ... Now we believe, that they also are interesting for observation during space mission Gaia. ...

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... After all we cannot send a probe to the star Altair to confirm that it is 17 light years away. ... The "Bessel determined that the star 61 Cygni was about ten light years away" Earth goes around the Sun in one year, so in six month it is in the opposite position in its orbit. ... In 1838 Bessel determined that the star 61 Cygni had a parallax of 0.314 arcseconds and therefore the star was about ten light years away (today the distance is more precisely measured to be 11.4 light years). ...

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• V774104: a Dark World Putting a New Light on the Solar System? | Astronotes
• Other Galaxies | Astronotes
• Universe | Astronotes - Part 2

IV International Astronomy Olympiad . ... Text of these problems is available also . ... To solve every problem you may use constants and well-known values you know by heart. ... The apparent diameter of the Moon, as seen from the Earth, is 31'. ... Can you observe a star with magnitude . ... Consider the stars as black bodies. ... Estimate the diameter of a black hole constructed using this patent from a ship with the mass of 5000 tn (1 tn = 1000 kg). ... What stars would you observe this nigth? ...

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• Problems of the 1-st International Astronomy Olympiad
• The International Olympiad of Euro-Asian Astronomical Society

... What is an intelligence or an intelligent life? ... Various particular cases, new regimes, original approaches etc. being attractive as they could, all this is a pale shade of a real process of cognition. ... May an infinitely complicated object be indeed so simple? ... An intelligence could not arise in an infinitely complicated universe! ... There are two possibilities: whether our imagination of infinitely complicated object is incorrect or the surrounding world is not infinitely complicated. ...

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• Natalya Raguzova Home Page
• The Radiopulsar PSRB1259-63 - a Probe in the Stellar Wind Plasma
• Be/X-ray binaries and candidates

... This file irassss.dat 180 16740 IRAS Small Scale Structure Catalog Sources assoc.dat 58 5178 Information about positional associations with sources in other catalogs meaning.txt 80 235 Details of ... Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- PSCname IRAS source name 11 A1 --- BMFlg Number of bands in 2): These fields are blank if the source was not detected in the corres- ponding IRAS band. ...

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• Group IAG
• Non-classified objects
• Not-classified objects

Radio astronomy and the Square Kilometre Array telescope (SKA) Stars, galaxies and other cosmic objects give out radio waves as well as light and other radiation. ... The SKA will detect the radio waves from distant objects in space, enabling astronomer s to answer many impor tant questions about the Univer se. ... One possible design for the Square Kilometre Array, in which the individual elements that collect the radio waves are 15-m diameter dishes, grouped into patches 200 metres across. ...

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• casacore: casa::LELCoordinates Class Reference
• casacore: casa::ObjectStack< T > Class Template Reference
• casacore: casa::ROStandardStManAccessor Class Reference

... Kuiper belt objects are icy bodies in the outer solar system. ... Views of Kuiper Belt Objects . Object 1993 SC . This image shows a small part of the discovery frames of 1993 SC, one of the brightest Kuiper-Belt objects so far discovered. ... Assuming that Object 1993 SC reflects light much like other primitive asteroids and comets in the out solar system, the diameter is around 300 kilometers (186 miles), or just a quarter the size of Pluto's moon Charon. ... Comet Shoemaker-Levy 9 Impact . ...

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• How to Become a Star (ESO Press Release 01/01)
• Next VLT Instrument Ready for the Astronomers (PR Photos 05a-c/00)
• Youngest Brown Dwarf Yet in Multiple Stellar System (ESO Press Release 16/00)

Pulkovo NEO Page . ... EPOS Software Package . ... EPOS ( E phemeris P rogram for O bjects of the S olar system) is the Windows PC application for study and ephemeris support of observations of the Solar system objects. ... It controls the part of common data and transfers the control to one of the programs that solve the restricted set of tasks. ... So with the EPOS software package one can calculate the accurate ephemerides for many objects and get the quick illustration of their motion as well. ...

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• Pulkovo NEO Page: Observations