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MASS – LUMINOSITY RELATION FOR MASSIVE STARS
MASS – LUMINOSITY RELATION FOR MASSIVE STARS

... Near the stellar surface we have Mr ≈ M and Lr ≈ L, and adopting κ ≈ κe = const, we may integrate equation (s2.3) to obtain ...
AY5 Announcements
AY5 Announcements

... Evolution  of  <8MSun  Stars •  For stars less than 8Mo these last slides describe the evolution pretty well. There are some differences in the details that depend on the initial main-sequence mass. •  For stars that start with 4Mo, it gets hot enough in the cores to ignite start carbon fusion on ...
AJAstroProject
AJAstroProject

... million ly away. • It is in the same group as M95 (Previous) and M96 not photographed. • In this exposure you can see two other galaxies, NGC3384 and NGC3379. • NGC3384 is in the Leo Group I and NGC3379 is a more distant galaxy. This was a 90sec exposure through the V-filter. ...
Small images
Small images

... collapses to a neutron star and the energy released explodes the rest of the star. But what if the explosion fizzled? What if the iron core collapsed to an object too massive to be a neutron star – a black hole. A star without rotation would then simply disappear.... But what if the star had too muc ...
Tutorial: Continuous Spectra
Tutorial: Continuous Spectra

... The energy carried by the photon determines the position of the electromagnetic wave on in the electromagnetic spectrum. If the resulting frequency is within the visible window, the energy of the photon will determine the color of the electromagnetic wave. ...
In Retrospect: Kepler`s Astronomia Nova
In Retrospect: Kepler`s Astronomia Nova

... the centre of the Universe around which everything in the celestial domain revolves. Kepler was the first to realize that orbits are better described by ellipses traversed at nonuniform speed than by combinations of ‘perfect’ circular motions on which orbits had hitherto been modelled. Like a modern ...
The Hertzsprung-Russell Diagram
The Hertzsprung-Russell Diagram

... Most stars lie in the main sequence because if a star is hotter it is brighter. Thus you would expect stars of the same size but different temperatures to form a diagonal line since “hotter means brighter” That Main-Sequence is steeper than a ‘same-size diagonal” shows that larger mass ‘normal’ star ...
AST 301 Introduction to Astronomy - University of Texas Astronomy
AST 301 Introduction to Astronomy - University of Texas Astronomy

... to about ½ AU, and it will become more than 100 times more luminous than it is now. Life will not be pleasant on Earth. The core of the Sun will be mostly helium, and will continue to contract and heat up. When the temperature in the core reaches about 108 K (about 1 million years after the Sun leav ...
Galileo, Newton and Gravity 1/31
Galileo, Newton and Gravity 1/31

... • gravity causes elliptical orbits where planet moves faster when closer to the Sun as force of gravity is larger there • Third Law actually D3 =(Msun + Mplanet) x P2 D=distance from Sun and P=period  weaker force further away gives longer period • As mass Sun much larger can mostly ignore mass pla ...
The Naked Eye Era
The Naked Eye Era

Earth, Moon, and Sun - Effingham County Schools
Earth, Moon, and Sun - Effingham County Schools

... 27. How did the Earth form? While solar gas and dust (nebula) were swirling around and slowly condensing to form the Sun, a small part of the nebula escaped the Sun’s gravity and became trapped in an orbit around the Sun. 28. Why do we have a leap year every four years? The Earth actually takes 365 ...
Foundation 1 - Discovering Astronomy
Foundation 1 - Discovering Astronomy

... Winter solstice ...
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Are constellations just mythic figures in the sky?

... Winter solstice ...
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... Young stars which are still accreting material are called T-Tauri Stars. Because mass is piling on, they sometimes have explosive outbursts. ...
R - Uplift North Hills Prep
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... This question is about gravitation. A binary star consists of two stars that each follow circular orbits about a fixed point P as shown. The stars have the same orbital period T. Each star may be considered to act as a point mass with its mass concentrated at its centre. The stars, of masses M1 and ...
Lesson 3 The Solar System
Lesson 3 The Solar System

... • People noticed the bright lights in the sky changed. • A solar system has stars like the sun as well as moons and planets. • All but 2 planets have one or more than one moon. ...
2. - Quia
2. - Quia

... 1. Would it be practical to travel to Sirius by any of the modes of travel listed on your chart? Why or why not? 2. The Voyager spacecraft were equipped with CDs that contain pictures and sounds depicting our world. One of the Voyager spacecraft is actually headed towards Sirius. If there is an inte ...
Lesson 3 The Solar System - Delaware Valley School District
Lesson 3 The Solar System - Delaware Valley School District

... • People noticed the bright lights in the sky changed. • A solar system has stars like the sun as well as moons and planets. • All but 2 planets have one or more than one moon. ...
Luminosity Classes
Luminosity Classes

... In general the less dense a star is the more luminous it will be (because it has more surface area). Luminosity and the thickness of the absorption lines are combined to group stars into Lumniosity Classes. Luminosity Classes are combined with spectral class to describe Stars. The Sun is Class V so ...
Exoplanets. I
Exoplanets. I

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IMPORTANT HISTORICAL DATES AND EVENTS

... The planets where shaped by the nearby sun and ended up rocky, small and dense, with at least one, Earth, orbiting at just the right distance to hold on to watery oceans and host the chemical of life. The planets can be divided up into two groups of four. Closest to the sun are the four inner planet ...
Four Homework Assignments
Four Homework Assignments

... three timescales for main-sequence stars with masses of 0.5, 1.0, 2.0, 4.0, 6.0, and 10.0 M . (b) What general conclusions (plural) can you draw from what you find? tnuc ∼ 0.1 × ...
Astronomy 15 - Homework 3 - Due Wed. April 24 1) As we`ll see
Astronomy 15 - Homework 3 - Due Wed. April 24 1) As we`ll see

... Now, another practical use of this comes from the fact that, in many circumstances, the high-order terms get very small very fast. If a < 1 this will be true, and the factorial in the denominator also does its part. This makes the Taylor series a powerful tool for determining the behavior of a funct ...
MSci Astrophysics 210PHY412 - Queen's University Belfast
MSci Astrophysics 210PHY412 - Queen's University Belfast

... The existence of a superwind is suggested by two independent variables. The high density observed within the observed shells in stellar ejecta, and relative paucity of very bright stars on the AGB. The latter (Prialnik P. 161) comes from the number of AGB stars expected compared to observed is >10. ...
teaching_sci_bib
teaching_sci_bib

... luminosity at the same rate the greenhouse gases were removed from our atmosphere so Earth could maintain a life-friendly constant temp ...
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Aquarius (constellation)



Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for ""water-carrier"" or ""cup-carrier"", and its symbol is 20px (Unicode ♒), a representation of water.Aquarius is one of the oldest of the recognized constellations along the zodiac (the sun's apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
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