Astronomy Picture of the Day . Bright Stars, Dim Galaxy . ... These two clusters of bright, newly formed stars surrounded by a glowing nebula lie 10 million light-years away in the dim, irregular galaxy cataloged as NGC 2366. ... THEMIS of Mars . ... Spinning Black Holes and MCG 6 30 15 . ... These dramatic stellar explosions that destroy stars and disperse elements that compose people and planets are not so well understood that astronomers can accurately predict when a star will explode - yet. ...

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... self-absorption - the absorption of light shining on an object by a process similar to that which produced the light originally; if a cloud emits less light than it absorbs from other clouds behind it, this net loss of light, termed self-absorption , causes the foreground cloud to appear darker than the background field (the term is from spectroscopy, where small absorption dips sometimes occur in larger emission lines, making the latter look as if it is absorbing part of itself) . ... HISA Main ...

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... 2001 October 26 . Elements in the Aftermath . ... CXC , NASA . ... And so a supernova explosion , a massive star's inevitable and spectacular demise, blasts back into space debris enriched in heavier elements to be incorporated into other stars and planets (and people! ... Just below and left of center, a point like object in the Chandra image suggests that the enriching supernova also produced a pulsar in its aftermath, a rotating neutron star remnant of the collapsed stellar core. ...

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• APOD: October 29, 1995 - Radioactive Clouds in the Milky Way
• APOD: 2003 August 11 - Elements of the Swan Nebula
• APOD: May 9, 1996 - Supernova Remnant: Cooking Elements In The LMC

... STScI-PRC00-30 HUBBLE PEEKS INTO A STELLAR NURSERY IN A NEARBY GALAXY NASA's Hubble Space Telescope has peered deep into a neighboring galaxy to reveal details of the formation of new stars. Hubble's target was a newborn star cluster within the Small Magellanic Cloud, a small galaxy that is a satellite of our own Milky Way. ... Astronomers are especially keen to study star formation in the Small Magellanic Cloud, because its chemical composition is different from that of the Milky Way. ...

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• K-band Arcetri Obscured Supernova Search - SNe Intro
• NASA's Observatorium--Image Gallery: Stars
• APOD: October 18, 1999 - NGC 3603: An Active Star Cluster

Astronotes Armagh Planetarium's Stellar Blog! ... Solar System . ... Planets . ... This bizarrely shrunken planetary system was found by NASAтАЩs Kepler mission, hence the parent star has been named Kepler-11. ... Planetary scientist and Kepler science team member Jack Lissauer said ?These six planets are mixtures of rock and gases, possibly including water.тАЭ €аNone of these strange new worlds are likely to be home to any form of life; their surface conditions are simply too extreme. ...

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• Cepheids Inconstant Stars which break the rules | Astronotes
• Kepler-10c: the First Mega-Earth | Astronotes
• Most Earth-like exoplanet found by ESO | Astronotes

... Archives . ... With relief, they have presentation files from the previous workshop . ... The workshop title may not attract astronomers but the contents, tools, methodologies, and theory are modern astronomy friendly. ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...

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• The AstroStat Slog massive data
• The AstroStat Slog Blog Archive mini-Workshop on Computational AstroStatistics
• The AstroStat Slog Blog Archive Open and Shut [Equation of the Week]

3) Planets and Brown Dwarfs . ... By its nature, this method is most sensitive to massive planets orbiting close to their stars. ... That means that some of the more massive extrasolar planets could actually be brown dwarfs (although the statistics of the finds suggest that most of them are not). ... Another possible difference between brown dwarfs and massive planets is how they are born. ... They would base the fundamental definition on the mode of formation: a planet is built from planetesimals. ...

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• ASP: An Ancient Universe - The Age of the Chemical Elements
• ASP: Why Should We Care About Exploding Stars?
• ASP: Book Review

Astronomers have found a radio pulsar with a companion at least 11 times the mass of the Sun - the most massive pulsar companion known. The identity of the companion is uncertain: it may be a massive late-type (red) star, a massive but compact blue star, or possibly a black hole. ... The probability of this late-type star being there by chance, and not being the pulsar companion, is only about 1.3%," says team member Dr. Fernando Camilo of Columbia University. ... So what can the companion be? ...

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• HIPASS Bright Galaxy Catalog
• ATNF Colloquium
• HI mass calculator

. Computer Ephemeris. Elements of osculating planetary orbits. Explanations. Each row contains at 0h of Time Dynamical Terrestrial of specified date in system of mean equator and ecliptic J2000.0 the ecliptic osculating elements of heliocentric orbit: inclination of orbital plane (degrees), longitude of ascending node (degrees), argument of perigelion (degrees), semimajor axis (astronomical units), mean motion (degrees per day), eccentricity (dimensionless), mean anomaly (degrees).

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• Dynamics of Space Flying
• Celestial Mechanics
• Introduction to Astronomy

The Sun is our nearest star and the source of energy for life on Earth. ... For centuries astronomers wondered whether they were clouds floating in the Sun's atmosphere, but we now know that they really are huge regions of magnetic field, about as intense as the field at the poles of an iron magnet. ... Such abrupt events were named solar flares , and what made them especially interesting was that occasionally, after a prominent flare, a magnetic storm would erupt on Earth. ...

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• Kuiper-Oort
• From Stargazers to Starships
• Venus

Some astronomers ignore low-mass stars because they aren t very bright. However, stars with initial masses between about 0.8 Msun and 8 Msun (AGB stars) play an important role as the main site of the slow neutron capture (s-)process, which produces roughly half of the elements heavier than iron. ... From this work, we will see have a better understanding of AGB nucleosynthesis, the chemical evolution of globular clusters, and the properties of helium-rich stars. ...

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• The High-Z SN Search Description
• IAU Commission #34 (Interstellar Matter)
• GSAOI Magellanic Cloud Planetary Nebulae Science Page

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

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• (Untitled)
• ENGAMPLE
• AY2016 (contents)

Orbital intersection . ... Structure of Taurid stream . ... Meteoroid swarm and Taurid fireballs . ... The following four diagrams schematically show four different Taurid orbits and the orbits of Earth and Jupiter. ... The Taurid stream contains particles (small, solid grains) at different stages of their precession cycles. ... The study of when a meteor stream can produce a meteor shower is the study of when precession brings orbits to intersection with Earth, or e.g. with Mars . ...

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• W.M. Napier, Senior Research Fellow
• High-Mass Star Formation
• Stars Beyond Maturity

Next: Triple with velocity curves Up: Fit scenarios Previous: Double-lined spectroscopic binary Contents . Add the remaining astrometric orbital elements to the fit parameters, and vary the secondary mass only. ... In this case, you may add also the primary mass to the fit parameters as the system is now constrained just like a double-lined spectroscopic binary. ...

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• Richest Planetary System Discovered | ESO
• ESO - Thesis Topic: Testing the non-universality of the low-mass end of the
• Single-lined spectroscopic binary

XMM-Newton observation of the core of the massive cluster Cyg OB2 located in the constellation Cygnus, 4,700 light-years from Earth. The cluster contains massive O-type stars that shine brightly in X-rays. Cyg OB2 #9 is seen as the bright star just below the central star, and in 2008 was determined to be a binary system. ... Hundreds of lower mass stars also fill the field of view, which spans nearly 22 x 16 arcminutes. ...

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• The most massive star | Astronomy.com
• What is the heaviest element that astronomers can detect? | Astronomy.com
• How massive must a colliding body be to disturb Earth's orbit? | Astronomy.com

... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...

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• New LBV Stars in the Andromeda Galaxy
• Galaxy sector, archive 2000
• New Luminous Variable Star in M33

... Format of the orbital elements | Estimation of the extrapolation errors | Version 1" of the orbital elements collection, determined by KIAM during flight and used for operations planning . Version 2" of the of the orbital elements collection, modified by IKI during flight and recommended for the orbital calculations during scientific data processing . ... Three kinds of the INTERBALL Auroral probe (IB_AUR) orbital elements' collections are presented here. ... IKI RAN | SSC IKI RAN | ...

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• (S-7a) The Black Hole at the Center of our Galaxy
• The Sun
• From Stargazers to Starships

... Главная . ... Новости . ... Проекты . Любителям астрономии . Проект ISON . ... Подробнее . ... Категория: Новости проекта ISON . ... Метки: Космический мусор ,љ Астероиды ,љ Гамма-всплески ,љ Любителям астрономии ,љ Кометы љ . ... Метки: Космический мусор ,љ Астероиды ,љ Любителям астрономии љ . ... Новости обсерваторий проекта] - Обсерватория Кубанского государственного университета от Иванов А - 09.04.2016 11:08:49 . ... 1999-2013 Copyright "Астрономия и Телескопостроение" . ...

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FEATURES OF RSC ENERGIA'S MARTIAN MISSION CONCEPT . ... for the interplanetary . ... Then, using propulsion units, this vehicle is injected into the interplanetary trajectory, and over the next few months the vehicle transits to Mars. ... A special lander separates from the main section of the vehicle to take to the Martian surface the mission crew or a part of the crew. ... Key data on the interplanetary vehicle of the RSC Energia concept . ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• S.P. Korolev RSC Energia - ISS - ISS Russian Segment
• S.P.Korolev RSC Energia - LAUNCHERS
• S.P.Korolev RSC Energia - UNIVERSAL SPACE PLATFORM

Some peculiarities of orbits of observed comets. ... Icarus, 2005 Simulation and reality Distribution of anti-perihelia of short-period comets with e 0.9 ( ecliptic coordinates ) Distribution of anti-perihelia of short-period comets with e 0.9 ( ecliptic coordinates ) Distribution of anti-perihelia of long-period comets with 0.9 e 1 ( ecliptic coordinates ) ­ ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/perminov.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/kovalenko.pdf
• http://www.gao.spb.ru/english/publ-s/viii-rfs/p077.pdf