... Since planets are expected to form out of the material in disks around young stars, the formation of a planet will thoroughly alter the structure of the circumstellar disk of their host star, forming significant gaps in the radial distribution of matter around the star. Additionally, processing of solids (annealing/crystallization) and changes in the overall gas/dust ratio are thought to happen during the planet formation process and are believed to alter the observational signature of the disk. ...

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• Exoplanet Caught on the Move | ESO

... 2010 July 4 . Companion of a Young, Sun-like Star Confirmed . ... Explanation: The first direct image of an extrasolar planet orbiting a star similar to our Sun has been confirmed. ... This sharp infrared image shows the young star's planetary companion positioned above and left of center. ... The discovery image, shown above , was taken in 2008 but confirmed only recently by noting that the planet stayed with its parent star as background stars slightly shifted over time. ... About APOD | ...

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• APOD: 2005 April 5 - Light from a Distant Planet
• APOD: 2009 June 3 - VB 10: A Large Planet Orbiting a Small Star

... Light from a Extra Solar Planet . ... The planet, illustrated in the above drawing , had its light detected by comparing the brightness of only the parent star, when the planet was behind the star, to the light emitted when both the planet and its parent star were visible. The Earth- orbit ing Spitzer Space Telescope made the observation in infrared light , where the intrinsic glow of the planet outshines the light it reflects from its central star. ... NASA Official: Jay Norris. ...

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• Journal "Peremennye Zvezdy"
• The 47 Ursae Majoris System
• VB 10: A Large Planet Orbiting a Small Star

... Planets . ... Earth Satellites . ... The newly discovered ?mega-Earth? ... Its sibling, the lava world Kepler-10b, is in the background (the two planets? proximity is grossly exaggerated) .?а Kepler-10c has a diameter of about 29 000 km, 2.3 times as large as Earth, and weighs 17 times as much. ... The first mega-earth to be discovered is Kepler-10c which orbits a star lying about 560 light years from the Sun in the constellation Draco. ... Astronomers Find a New Type of Planet: The ?Mega-Earth? ...

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• Kepler-11: a strange and crowded planetary system | Astronotes
• Kepler 36b and c: Too Close for Comfort | Astronotes
• Most Earth-like exoplanet found by ESO | Astronotes

home publications > mercury . SEARCH ASP SITE: Match ALL words Match ANY word . ... Publications of the ASP (PASP) . ... Planet-Building on the Grandest Scales . ... The extrasolar planets discovered to this time are believed to be giant gaseous planets similar to Jupiter and Saturn. ... This, together with the large masses of the extrasolar planets discovered to date, has led researchers to conclude that all the extrasolar worlds are giant gaseous planets similar to Jupiter and Saturn. ...

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• ASP: A Good Definition of the Word "Planet": Mission Impossible?
• ASP: Mercury's Time to "Shine"
• ASP: Guest Observer

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . Australia Telescope Compact Array . ... CSIRO, Australia's national science agency, operates a number of world-class radio astronomy observatories that are collectively known as the Australia Telescope National Facility or ATNF. ... CSIRO also manages the Murchison Radio-astronomy Observatory, where the Square Kilometre Array telescope infrastructure in Australia is to be centred. ...

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• Comission 31 Time
• Cosmic Engine: Planets
• Galaxy Lunch - Dave Lommen speaking on "Probing the first steps of planet

STScI . ... What is STScI . ... Spring Symposium Poster . ... This knowledge will pave the way for joining research from astronomy, Earth science, and biology to understand the past, present, and future of the Earth within its larger context as one of many habitable worlds throughout the Galaxy. Such work seeks to understand the formation and fate of the Earth as well as predict where and when different bodies will be suitable for both simple and complex forms of life. ... David Catling . ...

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• HST this week
• Observing Windows [Windows]
• Choosing Exposure Times

... Contents . ... Sidereal time . ... Mean longitude of the Moon, mean elements of the Moon's orbit and equator . ... Ephemeris for physical observations of the Sun . ... Ephemeris for physical observations of the Moon . ... Matrix elements for conversion to CIRS . ... Conversion of mean time to sidereal time (with accuracy 0.01 s ) . ... Conversion of sidereal time to mean time (with accuracy 0.01 s ) . ... Conversion of mean time to sidereal time (with accuracy 0.001 s and 0.0001 s ) . ...

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• AY2014 (contents)
• AY2012 (contents)
• AY2007 (contents)

... Tonight's Sky . ... Sky this Month . ... Star Atlas . ... Solar eclipse travelogue: Sulawesi delivers a spectacular eclipse . ... Chandra sees eclipsing planet in X-rays for first time . ... For the first time since exoplanets, or planets around stars other than the Sun, were discovered almost 20 years ago, X-ray observations have detected an exoplanet passing in front of its parent star. ... The main star in HD 189733 also has a faint red companion, detected for the first time in X-rays with...

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• Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets,
• Newly discovered planet in the Hyades cluster could shed light on planetary
• Kepler discovers multiple planets orbiting a pair of stars | Astronomy.com

Meteor outburst profiles and cometary ejection models . ... The spatial structure of meteor streams, and the activity profiles of their corresponding meteor showers, depend firstly on the distribution of meteoroid orbits soon after ejection from the parent comet nucleus, and secondly on the subsequent dynamical evolution. ... This paper describes how a trail cross section can be calculated once an ejection model has been assumed. ...

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• Armagh Astropark: The Planets
• Armagh Observatory
• Meteor showers at Mars

... 142,800 Mean density (kg/m^3) .. ... 5.203 Rotation period (length of day in Earth hours).. 9.8 Revolution period (length of year) (in Earth years). 11.86 Obliquity (tilt of axis) (degrees).. 3.08 Orbit inclination (degrees).. 1.3 Orbit eccentricity.. 0.048 Mean surface temperature (K)........................ 120 (cloud tops) Visual geometric albedo.. 0.44 Atmospheric components.............................. 90% hydrogen, 10% helium, .07% methane Rings.. ...

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• Astronomy HyperText Book: Planetary Motion
• Intelligent Life On Earth?
• Astronomy HyperText Book

Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System Characteristics Formation Exosolar Planets Class 3 Stars The Sun Stellar Evolution of Low and High Mass Stars Deaths of Stars Exotic Stars Class 4 Galaxies Galaxy Classification Formation of Galaxies Galactic Evolution ... So far, one planet has been studied by this method. ...

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Proposal Identification No.: ... Proposal Type: General Category: Observation Category: Time Requested this semester: Hours Next Semester: Hours already used for this pro ject: Additional Hours required to complete pro ject: Minimum Useful Time : Expected Data Storage: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 50 50 0 0 1 hour 100-500 GB Continuation of timing observations of the planets pulsar , PSR B1257 +12 We have recently completed 50-day, high-cadence timing ...

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• http://www.naic.edu/vscience/schedule/2015Fall/WolszczantagP2997.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/WolszczantagP3033tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/WolszczantagP2997tp.pdf

Thanks to numerous ground and space-based surveys, we are now aware of over 1800 planets orbiting other stars, with another nearly 5000 candidates from the Kepler Mission awaiting confirmation. ... The answer to this question lies in the study of young planets and their formation environments. In this talk I will show how high-precision time series data from space telescopes is beginning to illuminate the conditions surrounding planet formation and the star-disk connection. ...

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• COALA - Computational Astrophysics Laboratory
• Michele Bannister - Research
• Dougal Mackey - CV

Next: Imaging by an Optimizing Method . ... A big advantage of this numerical integrator is its stability: the error in the semi-major axis and the eccentricity depends only on the step size and does not grow with an increasing number of time steps. ... As the integration time increases, the numerical results become more contaminated by various errors. ... A new symplectic integrator produces no secular truncation errors in the actions of a Hamiltonian system. ...

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• Real-Time Systems

... Lyndon B. Johnson Space Center . ... Steven R. Swanson (PH.D.) . NASA Astronaut . ... NASA EXPERIENCE: Swanson joined NASA as a systems engineer and a flight engineer in the Aircraft Operations Division of NASAтАЩs Johnson Space Center working on the Shuttle Training Aircraft (STA). ... After completing Astronaut Candidate training, which included intensive instruction in Shuttle and International Space Station systems, he was assigned to the Astronaut Office Space Station Operations Branch. ...

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• Astronaut Bio: Peter J. K. Wisoff 11/2001
• Astronaut Bio: Mark C. Lee 10/2006
• Astronaut Bio: Jay Apt 06/1997

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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• jg0009
• jg0021
• jg0020

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA Exposure Time Calculator Help v1.0
• VISTA Integration Time DIT Recommendations
• Publications about VISTA

The apparent path of the Sun across the sky. ... The path of the Sun across the celestial sphere is very close to that of the planets and the moon. ... In one year, as the Earth completes a full circuit around the Sun (drawing above), the Earth-Sun line and its continuation past Earth sweep the entire plane. ... Since the Sun and Earth are in the plane of the ecliptic, the line is automatically in that plane too; if the moon is also on the same line, it must be in the plane of the ecliptic as well. ...

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• Introduction to The Nine Planets
• Why do people want to explore Mars
• Solar System Data

Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

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