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Star Map - Science Centre
Star Map - Science Centre

... “ground” ...
Motions in the Night Sky and the Celestial Sphere
Motions in the Night Sky and the Celestial Sphere

... Because a star map cannot make the ink darker as a way to describe how bright an object is, they will make the dot larger. Often, the Bayer designation is listed next to the stars. While the brighter stars have names, such as Sirius, most stars do not. Johann Bayer in 1603 suggested a naming method ...
HR Diagram Explorer
HR Diagram Explorer

... An actual HR Diagram is provided in the upper right panel with an active location indicated by a red x. This active location can be dragged around the diagram. The options panel allows you control the variables plotted on the x-axis: (temperature, B-V, or spectral type) and those plotted on the y-ax ...
Lec09_ch11_lifecycleofstars
Lec09_ch11_lifecycleofstars

... ASTR103, GMU, Dr. Correll ...
Lecture notes on Coordinte systems
Lecture notes on Coordinte systems

... is divided into 60 seconds. So there are 60 × 60 seconds in a degree. How are these related to minutes and seconds we are used. They are similar since we tell time by how fast the Earth takes to spin around, that is complete 360◦ . So an hour of time is also 360/24 degrees. – So measures of time lik ...
Proficiency Step #5--
Proficiency Step #5--

... Cygnus, and Altair in Aquilla). The Coathanger asterism (officially called Brocchi’s cluster) is very small and not at all noticeable with the naked eye—but easily viewed through binoculars. It is located about 1/3 of the way from Altair to Vega in the summer triangle in the constellation Vulpecula. ...
Lesson Plan G2 The Stars
Lesson Plan G2 The Stars

... good indicator of its distance. In Starry Night they will examine several different stars and they will see how some stars end their lives. ...
The Naked Eye Stars as Data Supporting Galileo`s
The Naked Eye Stars as Data Supporting Galileo`s

... would support Galileo's ideas regarding the stars being suns scattered through space. Data on the numbers of visible stars brighter than a given magnitude are given in Figure 3.10 ...
What is the “Meridian”?
What is the “Meridian”?

... You are in Bloomington and observe a star rising directly to the east. When this star reaches its highest point above the horizon, where will it be? (a) high in the northern sky (b) high in the eastern sky (c) high in the southern sky (d) high in the western sky (e) at the zenith ...
The Sun and the Stars
The Sun and the Stars

... (BD at 3640 falls into U-band) ...
Pulsating Variable Stars and The Hertzsprung - Chandra X
Pulsating Variable Stars and The Hertzsprung - Chandra X

... most mid-sized main sequence stars transition through as they evolve to the red giant branch. Miras have amplitude variations of more than 2.5 magnitudes. Mira (Omicron Ceti) is the prototype of Mira variable stars. The Sun will eventually become a pulsating Mira star. The Mira instability strip on ...
THE HR DIAGRAM
THE HR DIAGRAM

... Star  clusters  are  formed  from  giant  molecular  clouds  and  dust.  As  a  result,  the  stars  in  a  cluster  are  the  same  age  and  about  the  same  distance  from  Earth,  but  they  develop  in  a  range  of  masses.  Four  different  open  star  clusters  are  plotted  in  the  figure ...
The Evening Sky Map
The Evening Sky Map

... Multiple star system with 6 components. 3 stars visible in telescope. Dist=52 ly. With Castor, the twin sons of Leda in classical mythology. Dist=34 ly. Brightest star in Leo. A blue-white star with at least 1 companion. Dist=77 ly. The brightest star in Orion. Blue supergiant star with mag 7 compan ...
11 - Visual Magnitudes Project
11 - Visual Magnitudes Project

... Attached is a finding chart for the brighter stars in the open star cluster named Praesepe or M44 which lies in the constellation of Cancer, or Pleiades (M45) which lies in the constellation of Taurus. M44 and M45 are the 44th and 45th objects in the catalog compiled by Messier. Visual photometry is ...
uniview glossary - DMNS Galaxy Guide Portal
uniview glossary - DMNS Galaxy Guide Portal

... charged, they interact with these magnetic fields, and solar wind particles are swept around planetary magnetospheres. Life on Earth has developed under the protection of this magnetosphere. At times of increased solar activity, particles in the solar wind reach inward along the magnetic field lines ...
Photoelectric Photometry of the Pleiades
Photoelectric Photometry of the Pleiades

... 6. Record the magnitude measurements of the star reading on the Photoelectric Photometry Data Sheet on page 14 of this manual. Record the measurements of the star reading for all three filters before choosing another star. Also displayed is the signal-to-noise ratio or SN Ratio of the reading. A hig ...
Photoelectric Photometry of the Pleiades Student Manual
Photoelectric Photometry of the Pleiades Student Manual

... of paper. Be sure your graph’s y axis runs from 0 at the top to 25 at the bottom as shown above. Creating too small a graph will make it difficult to plot data accurately. You will then create a second graph like the first on a clear plastic sheet. On this second graph you will plot a group of main ...
ted_2012_power_of_design
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... therapy and stem cell transplantation, which remains an investigational area of treatment. ...
Determining the Sizes of Stars Using the HR Diagram
Determining the Sizes of Stars Using the HR Diagram

... after finishing their time as a main sequence star. These stars grow in radius, and can change temperature dramatically, but they do not change much in luminosity. ● White Dwarfs: White dwarfs are the end states of stars less than around 6 times the mass of the Sun. The white dwarf is the core of th ...
visual photometry - El Camino College
visual photometry - El Camino College

... human eye can detect stars brighter than about 6th magnitude when in a very dark site (far from city lights). Unfortunately, around El Camino, the eye can barely see 4th magnitude stars due to all of the light pollution from the surrounding LA city lights. However, with the additional light collecti ...
Visual Photometry - El Camino College
Visual Photometry - El Camino College

... human eye can detect stars brighter than about 6th magnitude when in a very dark site (far from city lights). Unfortunately, around El Camino, the eye can barely see 4th magnitude stars due to all of the light pollution from the surrounding LA city lights. However, with the additional light collecti ...
First young loose association in the northern hemisphere?
First young loose association in the northern hemisphere?

... presence of nearby gas can help to disentangle them from older ones. Nevertheless, in the RasTyc sample, we discovered 4 lithium-rich field stars displaying the same space motion, which are located within a few degrees from each other on the celestial sphere near the Cepheus-Cassiopeia complex and a ...
Constituents of the Milky Way
Constituents of the Milky Way

... Measuring Ages of Individual Stars For individual stars that aren’t in clusters (like the Sun), we can’t use the cluster turnoff method to measure an age. For instance, a lone G star might be young, or it might be 10 billion years old. How do we measure its age? The universe contained only hydrogen ...
Pretty Pictures of the Cosmos
Pretty Pictures of the Cosmos

... depths of a light-polluted city. Also known as the Seven Sisters and M45, the Pleiades is one of the brightest and closest open clusters. The Pleiades contains over 3000 stars, is about 400 light years away, and only 13 light years across. ...
February 2013 - astronomy for beginners
February 2013 - astronomy for beginners

... Lyrae and is the 5th star in Lyra. In the chart above it can be found just north (above) the brightest star α (Vega). The two pairs of the double double are labelled as ε1 and ε2 and are separated by 208″. In turn each pair is separated by just 2″, about 160 AU (1 AU = Earth / Sun distance). The fou ...
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Crux



Crux /ˈkrʌks/, located in the deep southern sky, is the smallest yet one of the most distinctive of the 88 modern constellations. Its name is Latin for cross, and it is dominated by a cross-shaped asterism that is commonly known as the Southern Cross. Although visible to the Ancient Greeks, it was seen as part of the constellation Centaurus, and not defined or accurately mapped till the 16th century.Known as Acrux, blue-white Alpha Crucis is the constellation's brightest star and the bottom star of the cross. Nearly as bright are Beta and Gamma, while Delta and Epsilon make up the asterism. Many of the constellation's brighter stars are members of the Scorpius–Centaurus Association, a loose group of hot blue-white stars that appear to share a common origin and motion across the Milky Way. Two star systems have been found to have planets. The constellation also contains four Cepheid variables visible to the naked eye under optimum conditions. Crux also contains the Jewel Box, a bright open cluster, and the Coalsack Nebula, the most prominent dark nebula in the sky.
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