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The Significance of Mega Stars
The Significance of Mega Stars

Today in Astronomy 102: electron degeneracy pressure and white
Today in Astronomy 102: electron degeneracy pressure and white

... period (plus Newton’s laws), we know that the mass of Sirius B is 1.00M . q From its observed color (blue-white), we know that its temperature is rather high: T = 29,200 K, compared to 5,800 K for the Sun and 10,000 K for Sirius A. q Its luminosity is only 0.003L , much less than that of Sirius A ...
P10263v1.2 Lab 6 Text
P10263v1.2 Lab 6 Text

... parsecs away, the Small Magellanic Cloud (a small satellite galaxy orbiting our own Milky Way) is about 53,000 parsecs away, making observations of individual stars much more difficult. Thus, we cannot use the Pleiades method with the Small Magellanic Cloud since the only individual stars we can suc ...
ISIMA lectures on celestial mechanics. 3
ISIMA lectures on celestial mechanics. 3

November - Hawaiian Astronomical Society
November - Hawaiian Astronomical Society

... charts! Maybe something was orbiting these stars. From the details of the bolometer readings—which channels lit up and so on—you would guess that this stuff took the form of majestic fields or rings of icy and rocky particles. It would be a new kind of disk, a discovery worth writing home to Madrid ...
Chromospherically young, kinematically old stars
Chromospherically young, kinematically old stars

... Received 3 July 2001 / Accepted 18 December 2001 Abstract. We have investigated a group of stars known to have low chromospheric ages, but high kinematical ages. Isochrone, chemical and lithium ages are estimated for them. The majority of stars in this group show lithium abundances much smaller than ...
Chapter 14 Neutron Stars and Black holes
Chapter 14 Neutron Stars and Black holes

... Example: Her X-1 2 Msun (F-type) star ...
VISIBLE STARS AS APPARENT OBSERVATIONAL EVIDENCE IN
VISIBLE STARS AS APPARENT OBSERVATIONAL EVIDENCE IN

... These opponents of Copernicus make certain calculations based on the premise that, although the earth's motion in its annual orbit produces some curious and extremely large changes in the case of the planets, it does not cause any similar effects in the case of the fixed stars; they calculate that t ...
The Milky Way: Home to Star Clusters
The Milky Way: Home to Star Clusters

... It is difficult to obtain a clear picture of the Milky Way’s structure as we are living on the inside, looking out across one of its spiral arms. We will never be able to travel far way enough to see the Galaxy in its entirety, but to gain some perspective on the size, scale and structure, we can st ...
Motions in the Night Sky and the Celestial Sphere
Motions in the Night Sky and the Celestial Sphere

Pattern recognition of star constellations for spacecraft
Pattern recognition of star constellations for spacecraft

... in attitude determination by the stars is as follows: some image forming device (e.g., a CCD-camera) is directed towards the stars. If the image can be matched to a reference, the direction of the imaging device is known, and thus the attitude of the spacecraft. One approach is to sweep the sky with ...
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Red Giant Structure There are two important characteristics for the
Red Giant Structure There are two important characteristics for the

Vulcan Chasers
Vulcan Chasers

... Joseph Le Verrier of France stood at the pinnacle o the astronomical world. His calculations had leCl to one of the supreme discoveries of astron­ orny ­ Neptune, a giant world circling the sun in tlii frigid realm beyond Uranus, the hitherto most remote known planet. Neptune had been sighted by Joh ...
Neil F. Comins - Kuwait Life Sciences Company
Neil F. Comins - Kuwait Life Sciences Company

... discovery and interpretation. Dozens of these conceptdriven, experiential walkthroughs allow students to make observations, draw conclusions, and apply their knowledge. Interwoven with multimedia, activities, and questions, students receive a deep, self-guided exploration of the concepts. ...
Bushnell North Star 127mm Maksutov Cassegrain review
Bushnell North Star 127mm Maksutov Cassegrain review

PDF format
PDF format

... b)  The apparent brightness is inversely proportional to distance. c)  The apparent brightness is proportional to distance. d)  The apparent brightness is inversely proportional to the square of the distance. e)  The apparent brightness is proportional to the distance ...
Stars - Emera Astronomy Center
Stars - Emera Astronomy Center

... to these images, as well as their drawings, to describe their flame. In stars, just as in Earth-bound fires, blue is hotter than yellow, and yellow is hotter than red. The Sun is much hotter than a candle flame. Unlike a candle, the Sun uses nuclear fusion as its energy source, not a chemical reacti ...
sections 16-18 instructor notes
sections 16-18 instructor notes

... iii. by examining orbits of high velocity stars. Such stars are nearby halo stars that have high apparent velocities relative to the Sun because most of their orbital motion is in the direction of the Galactic centre. The results depend upon the assumption that all such stars are bound to the Galax ...
Photometry of star clusters with SalsaJ - Eu-Hou
Photometry of star clusters with SalsaJ - Eu-Hou

... out when we have all of the star in the aperture, but keeps rising gradually as more and more of the background sky is included. From this graph, we can see that the best radius to use is about 15 - this is around the point where most of the star’s intensity is included in the aperture, but minimise ...
Ground-Based Astrometry 2010-2020
Ground-Based Astrometry 2010-2020

Astrophysical parameters of ten poorly studied open star clusters
Astrophysical parameters of ten poorly studied open star clusters

ATA2010
ATA2010

... If we see stars which are rich in -elements relative to iron, this means that the chemical evolution of the gas from which they formed happened quickly (~ 108 yr), before there was time for the SNIa to generate a lot of iron etc To measure the abundances of chemical elements accurately, we need hig ...
Lecture 1: Introduction to exoplanetary transits
Lecture 1: Introduction to exoplanetary transits

Astronomy Report Southern Cross Authors Maria Constanza Pavez
Astronomy Report Southern Cross Authors Maria Constanza Pavez

... This circumpolar constellation (always situated above the horizon) of the South Hemisphere, is located between the Centauri and the Fly constellations, just above the Polar Antarctic Circle and it is crossed by the Milky Way. The Crux is visible the whole year between 25 N and 90 S degrees of latitu ...
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