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Animals in “Light, Energy, and the EM Spectrum” Comic
Animals in “Light, Energy, and the EM Spectrum” Comic

... Sometimes the night sky goes to the dogs! Sirius, the “Dog Star” is the brightest star in our sky except the Sun. Find Sirius in the constellation which bears the Latin name Canis Major, Big Dog. Nearby, you can also see Canis Minor, Little Dog, with only 2 stars. The brighter of these two stars is ...
SGR and AXP – are they magnetars?
SGR and AXP – are they magnetars?

talk.wyse - Johns Hopkins University
talk.wyse - Johns Hopkins University

... high velocity dispersion – plausibly star cluster of Sgr dSph Available metallicity distribution based on four stars: two radial-velocity members at ~ 0.01 solar (Norris, RW et al. 2010), equal to that of the field halo, and of Sgr debris, two others very metalpoor, at 0.0003 solar ([Fe/H] ~ -3.5) ...
Quantum effects in astrophysics
Quantum effects in astrophysics

... levels of ordinary hydrogen by about one part in 2mP / me  3700 . In the visible part of the spectrum, this corresponds to a line shift on the order of 1.5 angstroms. This shift could be easily detected, yet, for many years, no deuterium was ever detected in any astronomical object. In contrast, th ...
Navigation: The Mariner`s Quadrant
Navigation: The Mariner`s Quadrant

Constellation Paper - Matt Hape`s Portfolio
Constellation Paper - Matt Hape`s Portfolio

... their flee from the assault of Typhon. Aphrodite and Eros were said to be tied together so they would not lose one another. These two fish were later honored by being placed in the heavens as the constellation Pisces. In Roman mythology it is a very similar story, but with Venus and Cupid rather th ...
Harappan Astronomy
Harappan Astronomy

... included from an external source that he attributes to the Harappans. Similarly, he suggests that the lunisolar calendar (and its synchronisation) that is in vogue in the Vedic literature is of no use to the nomadic people but are crucial for administration in cities and hence must be a Harappan pat ...
Document
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... oFirst measurements of the inclusive photon elliptic flow up to ET 15GeV have been done at RHIC energy with STAR BEMC. The elliptic flow of inclusive photons decreases with transverse momentum at high Pt but it is still finite up to Pt 15GeV. The finite value of inclusive photons elliptic flow a ...
Abstract - chara - Georgia State University
Abstract - chara - Georgia State University

... jovian and terrestrial. Low mass stars and brown dwarfs are very cool and faint and are therefore very hard to detect. Large scale infrared surveys are detecting a large number of these objects, which, due to magnitude limits, mostly turn out to be nearby. In the local stellar neighborhood they tend ...
Betelgeuse: an unauthorized biography
Betelgeuse: an unauthorized biography

... Rigel, β Ori, although exceptions are known to the rule of listing stars in constellations by decreasing apparent brightness. It is HD 39801, HR2061, classified as spectral type M2 Iab or M1-M2 Ia-Iab (Keenan and McNeil 1989). Betelgeuse is a Long Period Variable. The visible magnitude has been obse ...
Celestial Globes Armillary Spheres
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... requires the prior written permission of FSTC Limited. You agree not to adapt, alter or create a derivative work from any of the material contained in this document or use it for any other purpose other than for your personal non-commercial use. FSTC Limited has taken all reasonable care to ensure t ...
November, 2015 - The Baton Rouge Astronomical Society
November, 2015 - The Baton Rouge Astronomical Society

On the Cosmic Nuclear Cycle and the Similarity of Nuclei and Stars
On the Cosmic Nuclear Cycle and the Similarity of Nuclei and Stars

GG_CERN_0707
GG_CERN_0707

... Main Focus: Dwarf Spheroidals  Low luminosity, low surface-brightness satellite galaxies, ‘classical’ L ~ 106L, V ~ 24 mag/sq Extremely gas-poor Apparently dark-matter dominated  ~ 10km/s, 10 < ~ M/L <~ 100  Metal-poor, mean stellar metallicity < ~ –1.5 dex All contain old stars; extended ...
Paper - Astrophysics - University of Oxford
Paper - Astrophysics - University of Oxford

takes its time doing so. The coolest white dwarfs
takes its time doing so. The coolest white dwarfs

... that temperature remains constant throughout the star until just before the surface. The bottom portion shows the amount of degeneracy in the white dwarf. The white dwarf remains degenerate also until right below the surface. The drop in temperature occurs at about the same radius that the white dwa ...
see figure - Georgia Southwestern State University
see figure - Georgia Southwestern State University

... As the air moves around, even though the planets’ images move slightly, there are enough points on the image to make the average amount of light we receive keep relatively steady. (At any given time, some points are brighter than average and some are fainter.) ...
b. - UW Canvas
b. - UW Canvas

... Post-18.1: This graph shows the functional form of the dependence of the parallax angle on the distance an object is from Earth. If the minimum parallax angle we could measure were 0.5 arcsec, what is the maximum distance of a star that we could measure? ...
The Lyre of Orpheus - InteractiveStars.com
The Lyre of Orpheus - InteractiveStars.com

... Lyre is the most imaginative and creative of the signs. When they do, like Orpheus, they often strike a truly universal chord, which makes them fascinating to other people, for there can be something magical about them; a touch of other-worldly glamour which ensures that they will never lack friends ...
Seeing Red: Will Betelgeuse Go Supernova in
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... Fierce Orion raises his right arm that holds a warriors’ club, ready to strike down his foes. The red supergiant star Betelgeuse (pronounced “beetle juice”), also known as Alpha Orionis, forms his right shoulder. Because of its deep orange or topaz hue, it is called the Martial Star. Betelgeuse’s di ...
FOTO Imaging
FOTO Imaging

... of computer processing time can produce a very usable image from the original. Steve has been an amateur astronomer for more than 40 years. His interest in astronomy began just as the space age was beginning. He grew up on a farm in west-central Ohio where the skies were dark and the stars were brig ...
Study questions
Study questions

... Describe the experiments which showed that indigo buntings use the stars to navigate on their migratory journey. What experience, if any, was required for them to orient to the North Star (Polaris)? How did Stephen Emlen get them to orient to Betelgeuse rather than Polaris? How did the researchers d ...
Andromeda Galaxy www.AssignmentPoint.com The Andromeda
Andromeda Galaxy www.AssignmentPoint.com The Andromeda

11-Massive Stars
11-Massive Stars

... to understand the complex bipolar outflows in massive star formation and proof will require interferometer observations. The outflows are difficult to study because multiple outflows often emanate from the same large scale core. Clusters of stars form simultaneously in a core and the outflows origin ...
Introduction Introduction to to Astrophysics Astrophysics
Introduction Introduction to to Astrophysics Astrophysics

... children to centenarians. For others it is their vocation and becomes their profession. The word ‘astronomy’ itself derives from the Greek aster meaning ‘star’, and nomos meaning ‘law’, and originally referred to the mathematical laws governing the motion of the stars and planets. Astronomy essentia ...
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Ursa Minor



Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.
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