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- ESA Earth Online
- ESA Earth Online

Experimental single photon exchange along a space link of 7000 km
Experimental single photon exchange along a space link of 7000 km

... To reduce the effect of the fluctuation of the pointing error on µsat estimation, we divided the whole passage in intervals of 10 s, calculating for each interval the mean µrec . With this method we computed µsat for each analysis slice, distinguishing those where µsat ≤ 1, 1 < µsat ≤ 2, and µsat > ...
Goal: To understand the structure and makeup of our own Milky Way
Goal: To understand the structure and makeup of our own Milky Way

GG_CERN_0707
GG_CERN_0707

... • Neither the local disk, nor star clusters, nor spiral arms, nor GMC, nor the solar system, have associated DM: Given the absence of a very local enhancement, what is the smallest scale on which DM is concentrated? How can sub-halos in dSph galaxies with star ...
Abundances and possible diffusion of elements in M 67 stars⋆
Abundances and possible diffusion of elements in M 67 stars⋆

Age Distributions of Low Mass Stars in the Rho Ophiucus Molecular
Age Distributions of Low Mass Stars in the Rho Ophiucus Molecular



Publisher: Emily Barrosse Acquisitions Editor: Kelley Tyner
Publisher: Emily Barrosse Acquisitions Editor: Kelley Tyner

US - Real Science
US - Real Science

... hundred times the mass of our Sun. But they do not fully understand how such objects could be created out of ordinary stars. NGC 1313 is an intriguing study for astronomers. This new image demonstrates again how the FORS instrument can capture the beauty and stunning complexity of galaxies - and how ...
a report on pulsars, written for PHAS1901
a report on pulsars, written for PHAS1901

... dispersion. All electromagnetic radiation moves at a constant speed through a vacuum, but is slowed proportionally to it's wavelength when it travels through a medium. the interstellar medium is often regarded as a vacuum, but in actual fact is occupied by atoms and free electrons, albeit at extreme ...
FREE Sample Here
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... sky. Most people today no longer have an understanding of the basic appearance or motions of the sky. The three Window on Science (WOS) discussions in this chapter present very important concepts in all sciences. WOS 2-1 focuses on the development of scientific arguments. It is important to emphasiz ...
What is the minimum size of a star that will go supernova? A. Half
What is the minimum size of a star that will go supernova? A. Half

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chapter 2 - Test Bank 1

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PPS
PPS

... Spectra of stars and galaxies are obtained by using prisms attached to telescopes to split the incoming light into its rainbow pattern - a technique which goes right back to Isaac Newton's discovery that light can be split into its component colours in this way. The spectrum can then be photographed ...
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...  Match cycles of the moon to corresponding positions of Earth, moon, and sun.  Explain why the constellations visible in the night sky change throughout the year. As.1.2  Use scientific notation and astronomical units (AU, light year) to compare distances.  Place astronomic objects (planets, moo ...
absolute brightness: The apparent brightness a star would have if it
absolute brightness: The apparent brightness a star would have if it

... eclipsing binary: Rare binary-star system that is aligned in such a way from Earth we observe one star pass in front of the other, eclipsing the other star. Eddington limit: The limit beyond which the radiation force on matter is greater than the gravitational force. electric field: A field extendin ...
Altitude and Azimuth 4 page
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... ALTITUDE: The angle of an object above the horizon. Altitude is measured in degrees along a line perpendicular to the horizon, to the object of interest. An object on the horizon has an Altitude of 0 o, an object directly overhead has an Altitude of 90o. AZIMUTH: The angle from North clockwise along ...
absolute brightness: The apparent brightness a star would have if it
absolute brightness: The apparent brightness a star would have if it

... eclipsing binary: Rare binary-star system that is aligned in such a way from Earth we observe one star pass in front of the other, eclipsing the other star. Eddington limit: The limit beyond which the radiation force on matter is greater than the gravitational force. electric field: A field extendin ...
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... catalog that lists information about the star. For example, PSR J1302-6350 is a type of star known as a pulsar -- hence the PSR in its name. The symbols indicate the star's location in the sky. The 1302 and the 6350 are coordinates that are similar to the longitude and latitude designations used to ...
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... were observed 50-100 times, on scales of hours to months. Here, we present results for the L1688 cloud in  Oph. Young stellar objects (YSOs) are intrinsically variable on a wide range of time scales and in almost all wavelength regions. In fact, YSOs were originally discovered by their optical vari ...
Unit 44: Astronomy
Unit 44: Astronomy

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Coordinate Systems - AST 114, Astronomy Lab II for Spring 2017!
Coordinate Systems - AST 114, Astronomy Lab II for Spring 2017!

... Longitude is also measured in degrees, arcminutes and arcseconds, but unlike latitude there is no natural or physical characteristic of the Earth from which to set the zero point in longitude. As a result of global navigation, and what is now history, the British established a zero point in longitud ...
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19. Our Galaxy 19.1 The Milky Way Revealed Our goals for learning

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Practice Exam for 3 rd Astronomy Exam

... has a mass of about 100 solar masses. If the fragment were any more massive it would further fragment into smaller pieces as it continued to collapse from the large energy it releases during further collapse. The smallest fragment that forms a star has a mass of about 0.1 solar masses. If the fragme ...
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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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