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Moitinho et al. - Wiley Online Library
Moitinho et al. - Wiley Online Library

... Furthermore, metallicity does not affect the colours of these stars significantly. Hence the only unknowns that remain in the CMD analysis are distance and age, which can also be uniquely derived provided that the photometry is deep enough so that a population sequence appears with a well defined mo ...
Gizmos: H-R Diagrams
Gizmos: H-R Diagrams

... Gizmo Warm-up In the early 1900s, astronomers were able to identify many star characteristics such as color, size, temperature, and luminosity—or how bright a star is. However, astronomers did not yet understand exactly how these characteristics were related. Using the H-R Diagram Gizmo™, you will d ...
CHAPTER 30: STARS, GALAXIES AND THE UNIVERSE Analyzing
CHAPTER 30: STARS, GALAXIES AND THE UNIVERSE Analyzing

... The second and longest stage in the life of a star is the main-sequence stage. During this stage, energy continues to be generated in the core of the star as hydrogen fuses into helium. A star that has a mass about the same as the sun’s mass stays on the main sequence for about 10 billion years. Sci ...
Chapter 12 - Indiana State University
Chapter 12 - Indiana State University

... • A spectrum also can reveal a star’s composition, temperature, luminosity, velocity in space, rotation speed, and other properties • On certain occasions, it may reveal mass and ...
Chapter 8: The Pennsylvanian Period in Alabama: Looking Up
Chapter 8: The Pennsylvanian Period in Alabama: Looking Up

... period of only a hunded thousand years, imagine the changes that would occur over 310 milion years! Rigel Kentaurus (Rigel Kent for short, also known as Alpha Centauri) is currently the nearest star (it is a system of 3). It is 4.3 light years away and is the third brightest star in the night sky. I ...
The Pennsylvanian Period in Alabama: Looking Up Astronomy and
The Pennsylvanian Period in Alabama: Looking Up Astronomy and

... Few animals spend their time stargazing, so we must imagine what we might have seen had we been there. For example, we can ask: would the Minkin site tetrapods have been able to see the constellation Orion, with its familiar bright stars like Betelgeuse and Rigel (Fig. 8.5), or the popular asterism ...
Star Magnitude - ScienceEducationatNewPaltz
Star Magnitude - ScienceEducationatNewPaltz

... are of Greek and Latin origins and Vega, Rigel, Aldebaran are Arabic derivations. In some cases two names are given to a star because some stars are referred to with multiple names. The designation column gives the star's designation by Johann Bayer's letter and John Flamsteed's number. Johann Bayer ...
Unit H557/02 - Advance Notice Article - June 2017
Unit H557/02 - Advance Notice Article - June 2017

... Professional astronomers measure brightness with a logarithmic scale called stellar magnitudes, but this is not appropriate here. We shall deal only with absolute brightness and apparent brightness. ...
Name: Astronomy Lab: The Hertzsprung-Russell (H
Name: Astronomy Lab: The Hertzsprung-Russell (H

... Sometimes the student of astronomy starts to become overwhelmed trying to understand the many measurements and observations astronomers make. Data concerning distance, brightness, color, spectral class, mass, temperature, motion, etc. all seem to be gathered in an attempt to impress the student with ...
There are 88 constellations in the sky around the Earth. 12 are the
There are 88 constellations in the sky around the Earth. 12 are the

... constellation, it lies between Aldberan in Taurus, and the Square of Pegasus. About 2000 years ago, the vernal equinox (the place the Sun rose on the first day of spring) was in the constellation Aries. Due to wobbling of the earth's axis, this is no longer the case, but Aries is still regarded as t ...
HR Diagram - TeacherWeb
HR Diagram - TeacherWeb

... Gizmo Warm-up In the early 1900s, astronomers identified many star characteristics such as color, size, temperature, and luminosity—or how bright a star is. Using the H-R Diagram Gizmo™, you will discover how some of these characteristics are related. Start by moving your cursor over the stars in th ...
Comet Lulin - indstate.edu
Comet Lulin - indstate.edu

... Since Comet Lulin will be moving opposite the motion of the Earth, it will appear to approach us and move away especially fast. Beginning in February 2009, Comet Lulin will rise at about midnight local time, and will be about 6th or 7th magnitude. This won't be bright enough to go out and look at ...
SMMP_BISANA - Infinity and Beyond
SMMP_BISANA - Infinity and Beyond

... stage, the fusion between astronomy and mythology is so complete that no further distinction is made between them"--the stars were no longer merely identified with certain gods or heroes, but actually were perceived as divine(Seznec, 37-40). ...
Analemma - Stony Brook University
Analemma - Stony Brook University

... • Perseus, Andromeda, Pegasus, Cetus, Cepheus, and Cassiopeia are all to be found in the fall evening sky. • Perseus holds the head of Medusa (the variable star Algol - the Ghoul - is her eye). • As punishment for her vanity, Queen Cassiopeia, as a circumpolar constellation, is condemned to hang ups ...
Properties of Supernovae
Properties of Supernovae

... explosion results from the death of a massive star which has consumed its entire fuel supply. The apparent magnitude of a supernova brightens by about 10 magnitudes within a few hours, and for a few months the luminosity of the star is comparable to the luminosity of the entire parent galaxy. Supern ...
Table of Contents - Imiloa Astronomy Center
Table of Contents - Imiloa Astronomy Center

... - An H-Beta filter is also helpful to photograph. ...
Today: Magnitude Terminology Photometry Applications Reading
Today: Magnitude Terminology Photometry Applications Reading

... Vega); typically obtained by calculating differential  magnitude w.r.t. a known standard star. ...
Student Exploration Sheet: Growing Plants
Student Exploration Sheet: Growing Plants

... Gizmo Warm-up In the early 1900s, astronomers were able to identify many star characteristics such as color, size, temperature, and luminosity—or how bright a star is. However, astronomers did not yet understand exactly how these characteristics were related. Using the H-R Diagram Gizmo™, you will d ...
The Southern Fall PDF - Treasures of the Southern Sky
The Southern Fall PDF - Treasures of the Southern Sky

... Lacaille during his visit to South Africa in 1751–2. It is 8500 light-years away, and the component stars are all very young. The cluster is rather more compact than the Jewel Box Cluster, and there are traces of blue reflection nebulosity associated with the brighter stars and the red emission nebu ...
The Life Cycle of Stars Stars are a fascinating part of our universe
The Life Cycle of Stars Stars are a fascinating part of our universe

... longest stage in star’s life cycle. Small stars can remain here for billions of years fusing hydrogen into helium while larger stars remain for only millions of years. Smaller stars fuse atoms much slower than larger stars and therefore live much longer lives. As stars “age,” the outer layers of gas ...
Classifying the Spectra of Stars:
Classifying the Spectra of Stars:

... make measurements of the "strength of a line" or an absorption feature in a stellar spectrum, we will use a feature called The Equivalent Width. In an absorption line less energy is transported than in the neighboring continuum. The continuum represents the area where the pure blackbody emission spe ...
Using Photometric Data to Derive an HR Diagram
Using Photometric Data to Derive an HR Diagram

... plotted vertically, using Microsoft Excel. The photometry was performed using the software Imagine-32 at UCSB. ...
View poster
View poster

... PMT • The star sensor uses a photomultiplier tube (PMT) which collects the light from the stars and the Moon and amplifies the signal so we can analyze it. ...
Nearby Stars - How far away is it
Nearby Stars - How far away is it

... Getting back to nearby stars, here‘s Wolf 359. It is another dim red star. In fact, it‘s one of the least luminous stars known. Star Trek fans may recognize Wolf 359 as the scene of a great battle between the Federation and The Borg. Lalande 21185 - 8.32 light years Lalande 21185 is another dime red ...
August Newsletter
August Newsletter

... There are five August constellations right above us (in the southern hemisphere) and include some of the most spectacular and well-known objects in the sky. The centre of our Milky Way galaxy is located in the direction of Sagittarius and because of this Sagittarius contains more deep sky objects th ...
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Canis Major

Canis Major /ˌkeɪnɨs ˈmeɪdʒər/ is a constellation in the southern celestial hemisphere. In the second century, it was included in Ptolemy's 48 constellations, and is counted among the 88 modern constellations. Its name is Latin for ""greater dog"" in contrast to Canis Minor, the ""lesser dog""; both figures are commonly represented as following the constellation of Orion the hunter through the sky. The Milky Way passes through Canis Major and several open clusters lie within its borders, most notably M41.Canis Major contains Sirius, the brightest star in the night sky, known as the ""dog star"". It is bright because of its proximity to our Solar System. In contrast, the other bright stars of the constellation are stars of great distance and high luminosity. At magnitude 1.5, Epsilon Canis Majoris (Adhara) is the second brightest star of the constellation and the brightest source of extreme ultraviolet radiation in the night sky. Next in brightness are the yellow-white supergiant Delta (Wezen) at 1.8, the blue-white giant Beta (Mirzam) at 2.0, blue-white supergiants Eta (Aludra) at 2.4 and Omicron1 at 3.0, and white spectroscopic binary Zeta (Furud), also at 3.0. The red hypergiant VY Canis Majoris is one of the largest stars known, while the neutron star RX J0720.4-3125 has a radius of a mere 5 km.
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