... Kepler's 3rd Law . 21a.Applying 3rd Law . ... Besides the Moon, Earth now has many artificial satellites, put up by us earthlings for a variety of purposes. ... where for a satellite orbiting Earth at distance of one Earth radius R E , the constant k equals k=gR E 2 . ... The velocity for a circular Earth orbit at any other distance r is similarly calculated, but one must take into account that the force of gravity is weaker at greater distances, by a factor (R E / r) 2 . ...

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• Early Warning of Interplanetary Disturbances
• The Lagrangian Point L1

Besides the Moon, Earth now has many artificial satellites, put up by us earthlings for a variety of purposes. ... In principle, a satellite could then orbit just above its surface. ... Dividing both sides by m shows that the mass of the satellite does not matter, and leaves . ... Any slower and it loses altitude and hits the Earth ("2"), any faster and it rises to greater distance ("3"). ... This is Kepler's 3rd law , for the special case of circular orbits around Earth. ...

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Next: Front End Construction Up: Minutes of the 1st Previous: Minutes of the 1st . ... Calculated system temperature: 25-26K at 1525 MHz, 29-30K at 1375 MHz and 34-25K at 1225 MHz. ... Calculated G/T - again, center pixel better . ... Multi Beam Sky Footprint: Separation 2 beam widths between individual beams . ... Calculated Beam Comatic Level about 8 dB . ... German . ... Slide 1.9 shows calculated T sys with 2 points for each frequency; one is for the center beam and other is for the outside. ...

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• The Search for HVCs in Other Galaxies
• RFI Issues at AO
• The Evolution of Galaxies through the Neutral Hydrogen Window The Evolution of

... We have measured this "redshift" for the pink black holes, and allowed for it in our calculations. ... We see this effect in the emission from gas around these pink black holes, but it is far too small an effect to account for the pinkness. Thus the swirling motions of gas around or into the black holes cannot produc the colour. ... At first we thought that these things were normal blue black holes hidden behind clouds of interstellar dust, that absorbed the blue light and made them appear pink. ...

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... Public . Science . ... Science Users Information > Science Publications > Science Announcements . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... Science Announcements . ... Published: 17 Sep 2014 . An extended set of FAQs (Frequently Asked Questions) on data reduction is available . ... Published: 28 Aug 2014 . ... This feature is available for all ALMA programmes, except for science verification data. ...

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• ESO Workshop Local and Practical Information
• ESO Workshop
• ESO - The impact of Herschel surveys on ALMA Early Science. Garching, 16-19

... We can not observe the Universe when it is 1000 years old because a) there was no matter \b there were not photons \c the universe was opaque to radiation \d the speed of light was still changing at that time \e it had not begun its expansion \m Which of the following is a prediction ... heliocentric model for the Sola r System? \m \a stellar parallax \b retrograde motion \c Venus would never be observed at midnight \d different constellations would be seen at ...

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• Thermal History of the Universe
• Astronomy 123 Winter 2002
• Astronomy 121 Distance Education Class

Instrument Science Report OSG-CAL-97-06 Velocity Aberration Correction for Parallel Observations Colin Cox October 22, 1997 ABSTRACT The velocity aberration correction performed by the HST pointing control software is valid for the target direction only. ... For directions within 500 arcsec of the target the variation of the correction difference does not exceed 24 milli-arcsec. ... As HST orbits about the earth, the barycentric velocity and hence the velocity aberration correction varies. ...

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• http://www.stsci.edu/~mutchler/talks/Pluto_FIT.pdf
• http://www.stsci.edu/~mutchler/talks/Pluto_AAS.pdf
• Practical Validation of Results

Next: Young Energetic pulsars Up: A Tutorial on Radio Previous: The population of millisecond . Assuming a thin-screen model, calculate the apparent angular diameter of the Crab pulsar at 600 MHz. Assume that the apparent angular diameter = 100mas at 100 MHz. Calculate the apparent angular diameter at 600 MHz if the screen is located at 1% of the distance from the pulsar to the Earth. ... Calculate the parallax's for pulsars with distances of 100, 500, 1000, 5000, 10000 parsecs. ...

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• ASKAP Frequently Asked Questions
• ASKAP Early Science Community Workshop ASKAP Early Science Community Workshop
• Radio Continuum Measurements of Southern Early-type Stars

... Subject of Astronomy. ... Basis of Spherical and Practical Astronomy. ... Celestial Sphere. ... Changes of Star's Coordinates as a Result of Daily Rotation of Celestial Sphere. ... Time Measuring. ... Changes of Solar Equatorial Coordinates. ... Stellar Day, Stellar Time. ... Real Solar Time. ... Mean Solar Time. ... Connections between Stellar and Mean Time. ... Apparent Path and Configuration of Planets. ... Ways of Energy Transportation to Stellar Surface.Basis of Spectral Analysis. ... Solar...

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• Extragalactic Astronomy

Next: Conclusion Up: Old neutron star distribution Previous: Results of calculations . As is seen in Fig. , the old galactic neutron stars fill a thorus-like region extended up tens kiloparsecs above the galactic plane with sharp deficiency of stars toward the galactic axis. ... Now return to the crucial question about the applicability of the ergodicity principle to the dynamicas of stars in a real galaxy. ...

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• Be/X-ray binaries and candidates
• Canadian Paper Money - Questions Answers
• Extragalactic Gravitational Wave Background

otherwise stated, constants are denoted by the following symbols and may be taken to have the values below Elementary charge Speed of light in vacuum Planck constant Permeability of vacuum Permittivity of vacuum Unified atomic mass constant Rest mass of proton Rest mass of electron Boltzmann constant Avogadro constant Gravitational ... A pulse of light of frequency f is emitted from the space station towards the ship at exactly the time the ship passes the Earth in the Earth frame. ...

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• http://www.mrao.cam.ac.uk/~kjbg1/exams/2006_paper.pdf
• http://www.mrao.cam.ac.uk/~kjbg1/exams/2008_paper.pdf
• http://www.mrao.cam.ac.uk/~kjbg1/exams/2010_paper.pdf

... Re : ICMP send rate limit / ignoring ( Jukka Santala ) . ... 1) I haven't yet rebooted with this code ... wish me luck ;) 2) Am I missing something? ping -f and ping -l get mostly ignored Here's the bit of code , in icmp_reply () right at the beginning (after local varable definitions) : #ifndef CONFIG_NO_ ICMP _LIMIT if(!xrlim_allow( icmp _param- icmph.type, skb- nh.iph- saddr)) return; #endif I'll let you know how my tests with the thing proceed ;) (Sorry ...

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• Saturn's Moon Phoebe
• Frequently Asked Questions
• New Moons of Uranus

... What is there beyond the edge of the universe? ... This is often illustrated by newspaper headlines: "Scientist sees face of God, confirms Big Bang model" (a reference to results from the Cosmic Background Explorer satellite), "Is the cosmos younger than some of the stars it contains? ... The Lone Universe . ... We cannot reproduce it; we cannot take another one and see what happens to it; we cannot compare it to anything else, as astronomers routinely do with planets, stars, and galaxies. ...

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• ASP: VOLVELLES! Early Paper Astronomical Computers
• ASP: Science@Saturn: Cassini-Huygens Mission to Saturn and Titan
• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises

... satvelsrc computes as a function of time the component of the spacecraft velocity vector in the direction of given celestial source. ... SAS_ODF . or named via the generic command line parameters -o or -odfdir (see taskmain for details). ... The source coordinates obtained from the ODF can be overridden with the command line paramters withsrccoord=yes srcra=<ra> srcdec=<dec> and withorthosrc=yes defines a fictitious source in the direction perpendicular to the orbital plane. ...

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• Description

... These questions, among the most important and baffling to astronomers since the beginning of the modern astronomical era, might well be answered by a new space satellite mission. The Rotating Jets of Comet Hyakutake . ... The Compton Observatory Turns Five . ... Earlier this April, NASA's Compton Gamma Ray Observatory, completed its fifth successful year in orbit, exploring the gamma ray sky. ... Unexpected X-rays from Comet Hyakutake . ... Uranus's Moon Oberon: Impact World . ... April . ...

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Astronotes Armagh Planetarium's Stellar Blog! ... Moon . ... Alien Life . ... Space Flight . ... Posted on April 7, 2016 | 2 Comments Armstrong and Aldrin were the first two people on the Moon when Apollo 11 landed there in July 1969. ... Continue Reading.. ... Posted on October 23, 2014 | ... Posted on August 1, 2014 | ... 27 Comments In July 1969, those who could gathered around available television sets and radios for the moment that human life would leave their first trace on the Moon. ...

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• Human Exploration | Astronotes
• Space Flight | Astronotes
• ALMA: Europe's Giant Eye on the Sky | Astronotes

... Tonight's Sky . ... PHASE т?? ... Supernova showered Earth with radioactive debris . ... Astronomy for Kids . ... Swift satellite records early phase of gamma-ray burst . ... United Kingdom astronomers, using a telescope aboard the NASA Swift satellite, have captured information from the early stages of a gamma-ray burst - the most violent and luminous explosions occurring in the universe since the Big Bang. ... Only registered members of Astronomy.com are allowed to comment on this article. ...

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• Study questions dates for cataclysms on early Moon, Earth | Astronomy.com
• GRB theory questioned | Astronomy.com
• Even more questions for a cloudy night | Astronomy.com

... Data is taken from Hilton (2011): Active M3-M5, 332 hours on 4 stars observing 157 flares; Active M6-M8, 59 hours on 4 stars observing 39 flares; Less Active M3тАУM5, 147 hrs on 8 stars observing 28 flares; Inactive M0-M2, 256 hours on 16 stars observing 9 flares; Inactive M3-M5, 153 hours on 6 stars observing 3 flares; Active M0-M1, data from Moffett (1974), Doyle Mathiouidakis (1990) and Dal Evren (2011), 156 hours on 2 stars observing 63 flares. ...

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• Irregular Satellite Research
• Astronomy Survey - Questions Proposal | International Year of Astronomy in
• Terry Mosely's Bulletins

The velocity corrected for infall of the Local Group towards Virgo is noted vvir . It is calculated as: vvir = vlg + 208 cos(theta) Where vlg is the velocity relative to the Local Group, 208 km/s is the infall velocity of the Local Group according to Theureau et al. 1998 and Terry et al. 2002 and where theta is the angular distance between the observed direction and the direction of the center of the Virgo cluster (SG 104 -2). ...

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• Ned Wright's Cosmology Tutorial
• Results and discussion
• Documentation: LEDA: parameter: vrot

... 2014 Irkutsk-Listvyanka, Russia G r o u p language English Theoretical round General note. ... Footstep of babr. ... Draw in real scale a picture of image of the sunspot "footstep of babr" (see picture and condition of the previous problem) obtained in the focal plane of the LSVT. ... Orion's Belt. ... Estimate at what distance from the Babr the Penguin was, if the shining of the "fourth star of Orion's Belt" approximately corresponds to that of the three others in the picture. ... ISS near Zenith. ...

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• http://www.issp.ac.ru/iao/apao/2015/booklet/b15_ap15_o_en_ab.pdf
• http://www.issp.ac.ru/iao/2015/booklet/b11_ia15_p_en_b.pdf
• Rules and regulations for a participant