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100 Binocular Deep Sky Objects
100 Binocular Deep Sky Objects

Star Life Cycle Web Activity
Star Life Cycle Web Activity

... element can be used as fuel to burn and equilibrium is reached once again. Eventually the fuel sources run out and the star dies or explodes. The main fuel sources are Hydgroen, then Helium, then Carbon, then cool off to death. ...
Astronomy 114 – Summary of Important Concepts #2 1 Stars: key
Astronomy 114 – Summary of Important Concepts #2 1 Stars: key

here - British Astronomical Association
here - British Astronomical Association

... • It’s simple and fascinating to watch stars that are billions of miles away changing in brightness, and to learn about these systems from data that is obtained using your own eyes. • Your data, when combined with other observers’ data can be valuable and unique, and can make a real contribution to ...
Stars Of Orion Essay Research Paper 01
Stars Of Orion Essay Research Paper 01

... From the visible perspective, the most obvious things an observer of Orion can tell are the relative size, position and colour of the stars. Studying the colour of stars allows us to determining its temperature, which in turn is related to it’s mass. Temperature determines a star’s colour. Red star ...
hw5
hw5

SHELL H II REGIONS IN NGC 6334
SHELL H II REGIONS IN NGC 6334

ASTR 553/554 (1) : Questions
ASTR 553/554 (1) : Questions

... c. Using MV, = 4.82, calculate the Milky Way's absolute magnitude, MV. If viewed from Virgo (distance 15 Mpc) what would its apparent magnitude, mV be? Would an Alien equivalent of Charles Messier have included the Milky Way in his catalogue of bright nebulae? d. What is the apparent inclination of ...
Wazzat Mean - Peterborough Astronomical Association
Wazzat Mean - Peterborough Astronomical Association

... and Venus are best seen when at maximum elongation, and thus are highest above the horizon before sunrise or after sunset. Ephemeris A timetable with celestial coordinates that indicates where a planet, comet, or other body moving in relation to background stars will be in the sky. Its plural is eph ...
Stars
Stars

Homework 1 SOLUTIONS - University of Colorado Boulder
Homework 1 SOLUTIONS - University of Colorado Boulder

... 1. All stars are called “fixed stars” because they are all at fixed celestial locations. This means that at any one specific location on Earth they have fixed rising and setting locations (setting locations ALWAYS symmetrical to rising locations around the meridian) and a fixed angle with respect to ...
Homework #3 10 points Question #1 (2 pts) The brightest star in the
Homework #3 10 points Question #1 (2 pts) The brightest star in the

... iron? You can think the following way: let’s imagine that in a region of space A we found one massive star that exploded as a core collapse supernova, and in a region of space B we found several white dwarfs that all exploded as thermonuclear supernovae. The number of white dwarfs in the region B is ...
Far Ultraviolet Spectroscopic Explorer
Far Ultraviolet Spectroscopic Explorer

... Search data set for interesting individual objects that represent rare classes of objects. ...
Wien`s Law and Temperature
Wien`s Law and Temperature

Practice Questions for Exam 3
Practice Questions for Exam 3

... According to the inverse square law of light, how will the apparent brightness of an object change if its distance to us doubles? A. Its apparent brightness will increase by a factor of 4. B. Its apparent brightness will decrease by a factor of 4. C. Its apparent brightness will decrease by a factor ...
r*=13.6 km MPA1 EOS
r*=13.6 km MPA1 EOS

... Comptonized emission from the one visible hot spot and makes use of the Oblate Schwarzschild approximation for ray-tracing. We include a scattered light contribution, which accounts for flux scattered off an equatorial accretion disk to the observer including time delays in the scattered light. We g ...
ch 2 the sky
ch 2 the sky

... between two objects in the sky  Angular diameter – a measure of the size of an object in the sky  Scientific model – an intellectual concept designed to help us think about a natural process without necessarily being a conjecture of truth  South circumpolar constellation – one of the constellatio ...
Terrestrial Planet (and Life) Finder
Terrestrial Planet (and Life) Finder

The correct answers are written in bold, italic and underlined. The
The correct answers are written in bold, italic and underlined. The

... • the core of a red giant star, revealed when the outer layers are shed during the planetary nebula phase. • a white dwarf star that has cooled to a low temperature over its long lifetime. Stars with masses less that 8% of that of the Sun remain as long-lived, dim brown objects, never brightening li ...
Star Formation
Star Formation

Photoelectric Photometry of the Pleiades Student Manual
Photoelectric Photometry of the Pleiades Student Manual

... view is called the photoelectric aperture and is the portion of the sky being examined by the photometer. The desired star must be carefully centered within the aperture. Otherwise, some of the light from the star spills out of the aperture and is ...
`A ship flying in space:` Earth seen through the eyes of an astronaut
`A ship flying in space:` Earth seen through the eyes of an astronaut

... 1938. Hundreds of science fiction movies from the 1902 silent epic “A Trip to the Moon” (featured in the current film “Hugo”) to “Star Wars” to this year’s “Cowboys and Aliens” have fed a deep curiosity about intelligent beings elsewhere in the universe. Hang on to your hats, because reality is star ...
solutions
solutions

Evolution of a Star
Evolution of a Star

... has evolved into a giant. If the star equals one solar mass, then it becomes a red giant. If the star equals 100 solar masses, then it will become a supergiant. In about 5 billion years, our sun will become a giant. Once the red giant’s core uses its supply of helium, it contracts even more. As the ...
Deep Space Mystery Note Form 3
Deep Space Mystery Note Form 3

< 1 ... 127 128 129 130 131 132 133 134 135 ... 270 >

Cygnus (constellation)



Cygnus /ˈsɪɡnəs/ is a northern constellation lying on the plane of the Milky Way, deriving its name from the Latinized Greek word for swan. The swan is one of the most recognizable constellations of the northern summer and autumn, it features a prominent asterism known as the Northern Cross (in contrast to the Southern Cross). Cygnus was among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations.Cygnus contains Deneb, one of the brightest stars in the night sky and one corner of the Summer Triangle, as well as some notable X-ray sources and the giant stellar association of Cygnus OB2. One of the stars of this association, NML Cygni, is one of the largest stars currently known. The constellation is also home to Cygnus X-1, a distant X-ray binary containing a supergiant and unseen massive companion that was the first object widely held to be a black hole. Many star systems in Cygnus have known planets as a result of the Kepler Mission observing one patch of the sky, the patch is the area around Cygnus. In addition, most of the eastern part of Cygnus is dominated by the Hercules–Corona Borealis Great Wall, a giant galaxy filament that is the largest known structure in the observable universe; covering most of the northern sky.
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