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the entire issue as one large (23
the entire issue as one large (23

... a morphologist, and was preoccupied throughout his career with matters of classification. Though his early life was difficult, and his pursuit of astronomy as a career was opposed by his father, he took a position at Yerkes Observatory in 1926 and remained there for the rest of his working life. The ...
Hariprasad comes from well known Jyotish family in Andhrapradesh
Hariprasad comes from well known Jyotish family in Andhrapradesh

... 505 A.D. - Varahamihira There is no basis to confirm that any one of them is correct or wrong. They are based on the estimate of annual precession of equinoxes by respective Astronomers. They can at best be their best guess, because annual precession of equinoxes was not constant in the past and the ...
astro-ph/0303282 PDF
astro-ph/0303282 PDF

... image. These can be compared to the predicted brightness of extrasolar planets from models (Burrows et al. 1997, Burrows 2002, Marley 2002.) We could detect a 4-5 Jupiter-mass planet at the separation of the Epsilon Eridani dust ring and a 6-8 Jupiter-mass planet at the separations of the Vega dust ...
Sample pages 1 PDF
Sample pages 1 PDF

... expand again with latent energy from the radiation release and are eventually lost to space with an increase in the power of the stellar wind at this stage. Once the luminous outer envelope of the star is lost, the naked core is all that is left, a small, hot remnant with a fraction of the luminosit ...
A Synopsis of the Paper, “Optical Performance of the James Webb
A Synopsis of the Paper, “Optical Performance of the James Webb

... The WFE total for NIRCam is computed by the RSS of the OTE, ISIM, and WFS&C errors. Each of these subsystems have budgeted their allowable WFE to their respective individual components. For example a portion of the OTE allocation of 131 nm rms is allocated to design residual, alignment, and figure e ...
Pluto Gets Demoted
Pluto Gets Demoted

... Second, it has to be big enough to form a round or nearly round shape. Check! Pluto is quite a bit smaller than Mercury, the next smallest planet, but it is massive enough for its own gravity to create a spherical shape. Third, it has to “clear the neighborhood around its orbit.” This means that the ...
Astronomy and Astrophysics (ASTRO) Iowa State University – 2013-2014 1
Astronomy and Astrophysics (ASTRO) Iowa State University – 2013-2014 1

... asteroids. Extensive use of the planetarium is included. Students who take Astro 120 may count credit in only one of Astro 102 or 103 toward graduation. ASTRO 125L. The Sky and the Solar System Laboratory. (0-2) Cr. 1. F.S. Prereq: Concurrent or previous enrollment in ASTRO 120 Laboratory course to ...
18_Testbank - Lick Observatory
18_Testbank - Lick Observatory

... C) A black hole is truly a hole in spacetime, through which we could leave the observable universe. D) If the Sun magically disappeared and was replaced by a black hole of the same mass, Earth would soon be sucked into the black hole. E) If you fell into a black hole, you would experience time to be ...
Name: Period: ______ Brahe and Kepler Tycho Brahe Tycho Brahe
Name: Period: ______ Brahe and Kepler Tycho Brahe Tycho Brahe

... in Europe. He occupied this post until, in 1612, Emperor Rudolph II was deposed. In Prague Kepler published a number of important books. In 1604 Astronomia pars Optica ("The Optical Part of Astronomy") appeared, in which he treated atmospheric refraction but also treated lenses and gave the modern e ...
Report from the Subaru Telescope for External
Report from the Subaru Telescope for External

... proto-planetary disks with various morphologies. In addition, frontier pieces of research ...
Star Clusters in Mergers
Star Clusters in Mergers

... These clusters have properties similar to those seen in the mergers, but always fewer in number, and generally fainter in luminosity. It appears that wherever you have regions of star formation, you have young massive clusters being formed, not just in mergers ! ...
Meteorites: Fragments of Asteroids
Meteorites: Fragments of Asteroids

... The recovery of 1 Ceres was the beginning of a series of discoveries made over the next 7 years that culminated in the discovery of three additional asteroids: 2 Pallas, 3 Juno, and 4 Vesta. It became apparent that the space between Mars and Jupiter was not the home of a single planet but of several ...
Meteorites: Fragments of Asteroids - Beck-Shop
Meteorites: Fragments of Asteroids - Beck-Shop

Barium and europium abundances in cool dwarf stars and
Barium and europium abundances in cool dwarf stars and

... halo stars are of the r-process origin. Much observational efforts were invested in testing this idea. For extremely metalpoor stars with metallicities [Fe/H] ≤ −2.4 McWilliam (1998) has derived an average [Eu/Ba] = 0.69, consistent with pure rprocess nucleosynthesis provided that the data of Arland ...
Comets, the Kuiper Belt and the Oort Cloud
Comets, the Kuiper Belt and the Oort Cloud

... the plane in which the planets orbit (the ecliptic), and they have similar perihelion distances, very close to the sun. Figure 4 illustrates, using different colors, the different families of comets, most of which have been discovered since 1990. The Jupiter family (red dots in Figure 4) are a class ...
Optics and Telescopes PowerPoint
Optics and Telescopes PowerPoint

... except for the detector, called a bolometer. – IR scopes detect heat from warm gas or warm objects. “Warm” means not hot enough to glow in visible light. – These scopes must be kept very cold or the heat that the ‘scope itself radiates will swamp out what is being observed. ...
The ISO–SWS Spectrum of Planetary Nebula NGC 7027
The ISO–SWS Spectrum of Planetary Nebula NGC 7027

The Big Bang
The Big Bang

... If the dust weren’t there, this would probably be classified as an elliptical galaxy. Instead it’s usually called “peculiar”. ...
1 Pau Amaro Seoane - modest 15-s
1 Pau Amaro Seoane - modest 15-s

ASTRONOMY AND ASTROPHYSICS Barium and europium
ASTRONOMY AND ASTROPHYSICS Barium and europium

... halo stars are of the r-process origin. Much observational efforts were invested in testing this idea. For extremely metalpoor stars with metallicities [Fe/H] ≤ −2.4 McWilliam (1998) has derived an average [Eu/Ba] = 0.69, consistent with pure rprocess nucleosynthesis provided that the data of Arland ...
Focus and pointing adjustments necessary for laser guide star
Focus and pointing adjustments necessary for laser guide star

... commands are sent to the DM to correct sensed wavefront errors. However, several characteristics of the LGS differ from the NGS, and not all wavefront errors visible in an NGS are visible in an LGS. At Keck, the use of off-axis laser projection complicates the laser pointing model. Focus complicatio ...
Planet Hunters: The First Two Planet Candidates Identified by the
Planet Hunters: The First Two Planet Candidates Identified by the

... hot Jupiters, and atmospheric properties of transiting gas giant planets. The combination of Doppler and photometric measurements of transiting planets is particularly informative because it yields planet densities and enables theoretical modeling of the interior structure and composition of exoplan ...
A Very Dense Low-Mass Molecular Condensation in Taurus
A Very Dense Low-Mass Molecular Condensation in Taurus

... 3.1. Summary of the Present Search We detected H 1 3 CO + J = 3-2 emission only for 4 condensations whose H 1 3 CO + J = 1-0 antenna temperature exceeds 1 K. On the other hand, we did not detect H 1 3 CO + J — 4-3 emission toward any starless condensations. The intensity of these H 1 3 CO + lines ap ...
X-Ray Astronomy of Supernova Remnants
X-Ray Astronomy of Supernova Remnants

... Dying Stars and the Birth of the Elements ...
RXTE PCA Contributions to Monitoring Fast Transients
RXTE PCA Contributions to Monitoring Fast Transients

... Rapid Burster and GRS 1747-312: similar durations, different luminosities; XTE J1751-305 vs SAX J1808.4-3658: shorter, but higher luminosity. Many faint transients with distance estimates (from bursts or globular cluster membership) are just distant, not low luminosity at peak or low average dM/dt . ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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