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Questions - Clever Teach
Questions - Clever Teach

... (iii) One theory of the origin of the Universe predicted that there should be cosmic background radiation with a wavelength of about 1 mm. Explain why scientists had to wait until the development of space flight before they could study this radiation in detail. ...
FREE Sample Here
FREE Sample Here

... expansion rate, the Big Bang must have occurred about 14 billion years ago. We are “star stuff” because most of the atoms in our bodies (all the elements except for hydrogen, since our bodies generally do not contain helium) were made by stars that died long ago. These elements were released into sp ...
Workbook IAC
Workbook IAC

... months. Comets appear to be bright balls with fat tails. They do not fall rapidly in the sky; you would have to watch one for hours or days to see its movement. The center of a comet is a ball of frozen gas, dust, and water. Like planets or moons, comets orbit around the Sun. The comet that causes ...
Project 5: Globular cluster
Project 5: Globular cluster

HD 140283: A Star in the Solar Neighborhood that Formed Shortly
HD 140283: A Star in the Solar Neighborhood that Formed Shortly

... stars (whose V magnitudes range from 11.9 to 16.6). Due to space limitations, the details of this process will be published elsewhere, but we summarize here. For spectral classification, we obtained digital spectra with the WIYN 3.5m telescope and Hydra spectrograph at Kitt Peak National Observatory ...
The Fundamental Plane, Stellar Popula6ons
The Fundamental Plane, Stellar Popula6ons

... environment
(NN/local
density/cluster
radius/cluster
richness)?
   What
is
origin
of
the
‘Blt’
of
the
FP
and
its
variaBon
with
λ?

 How
much
is
due
to
stellar
populaBon
variaBons
and
how
much
 is
due
to
structural
non‐homology
or
variaBons
in
Mstar/Mdark?
   What
is
the
origin
of
the
sca7er
about
 ...
Lecture-25 Notes - Georgia Southern University Astrophysics
Lecture-25 Notes - Georgia Southern University Astrophysics

Finnish Centre for Astronomy with ESO
Finnish Centre for Astronomy with ESO

Searching for Dwarf Galaxies and Population III Star
Searching for Dwarf Galaxies and Population III Star

... a result, the primary identifying feature in the rest-frame ultraviolet spectra of early stars is a strong HeII (1640 Å) emission line. One of the best environments to discover these sources is the chemically unevolved surroundings of a large galaxy or proto-cluster of galaxies at high redshift. The ...
Notes - Bill Wolf
Notes - Bill Wolf

... Absolute and Apparent Magnitude Obviously how bright a star appears on earth is only somewhat related to how bright the star actually is, since varying distances can make a star appear brighter or dimmer. Astronomer then use the word brightness generically to talk about how bright a star appears fro ...
Jupiter`s Radio Signals
Jupiter`s Radio Signals

Circular ac
Circular ac

... or nearly 4.5 × 1015 km) from Earth in the constellation Lyra.[1][2] The planet was discovered by NASA's Kepler spacecraft using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. NASA announced the confirmation of the exoplanet on 6 ...
Chapter 13 The Stellar Graveyard
Chapter 13 The Stellar Graveyard

... We do not know exactly how, but if there are charged particles trapped by the strong magnetic field of the neutron stars near the magnetic poles, the strong magnetic field directs the radiation field along the magnetic axis of the neutron stars. • If the axis of the magnetic dipole is not aligned wi ...
Talk - The Department of Astronomy and Astrophysics
Talk - The Department of Astronomy and Astrophysics

sections 12-15 instructor notes
sections 12-15 instructor notes

10 Astrophysics (Option E)
10 Astrophysics (Option E)

... would see the stars moving round in the same way as you would see objects in your room move if you sat on a spinning chair. Stars on the horizon move horizontally, but if you look up they make circles with the pole star in the middle. If you time this rotation, you would find that one complete revol ...
sachkov_2013 - Putting A Stars into Context
sachkov_2013 - Putting A Stars into Context

... earth elements (PrIII and NdIII) have large RV amplitude up to 1 km/s while lines of BaII and FeII show no detectable RV variations ...
Project 2. CCD Photometry
Project 2. CCD Photometry

... Although we think of interstellar space as a vacuum, it is in fact filled with tenuous  gas and dust. Like a smoke‐filled room, the gas and dust along the line of sight to a  star  dim  the  starlight  by  absorbing  and  scattering  the  light.  This  effect  is  called  interstellar extinction. If ...
The Cosmic Perspective Star Stuff
The Cosmic Perspective Star Stuff

... a)  Yes, all stars create heavier elements than carbon when they become a supernova. b)  Yes, but there would be far fewer heavier elements because highmass stars form elements like iron far more prolifically than low-mass stars. c)  No, the core temperatures of low-mass stars are too low to fuse ot ...
Review: How does a star`s mass determine its life story?
Review: How does a star`s mass determine its life story?

The hawaiian star compass and the unit circle
The hawaiian star compass and the unit circle

the astrolabe - IREM Aix
the astrolabe - IREM Aix

... 1. Matrix or mother: a disc of brass or bronze 10 to 50 cm in diameter which accommodates the various parts of the instrument. 2. Tympanum: an engraved plate that is placed on the mother. Designed for a given latitude, certain astrolabes possess several of these. 3. Spider (or Rete): a perforated di ...
A Tour of the Radio Universe
A Tour of the Radio Universe

... This mosaic image is the sharpest wide-angle view ever obtained of M82. The galaxy is remarkable for its bright blue disk, webs of shredded clouds, and fiery-looking plumes of glowing hydrogen blasting out of its central regions. Throughout the galaxy's center, young stars are being born 10 times fa ...
Asteroseismology of Solar-Like Stars
Asteroseismology of Solar-Like Stars

... The two types of standing wave oscillations within a star are called g (gravity) and p (pressure) modes. In gravity modes the restoring force for the oscillation is the gradient of the gravitational acceleration within the star, they are also known as buoyancy waves. A parcel of gas within a star wi ...
has occurred over the past 14 billion years COSMIC DOWNSIZING
has occurred over the past 14 billion years COSMIC DOWNSIZING

... have apparently been assembling from the earliest times until the present. The supermassive black holes that are still active, however, do not exhibit the same behavioral patterns as the distant quasars. Quasars are voracious consumers, greedily gobbling up the material around them at an enormous ra ...
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Ursa Major



Ursa Major /ˈɜrsə ˈmeɪdʒər/ (also known as the Great Bear and Charles' Wain) is a constellation in the northern celestial hemisphere. One of the 48 constellations listed by Ptolemy (second century AD), it remains one of the 88 modern constellations. It can be visible throughout the year in most of the northern hemisphere. Its name, Latin for ""the greater (or larger) she-bear"", stands as a reference to and in direct contrast with Ursa Minor, ""the smaller she-bear"", with which it is frequently associated in mythology and amateur astronomy. The constellation's most recognizable asterism, a group of seven relatively bright stars commonly known as the ""Big Dipper"", ""the Wagon"" or ""the Plough"" (among others), both mimicks the shape of the lesser bear (the ""Little Dipper"") and is commonly used as a navigational pointer towards the current northern pole star, Polaris in Ursa Minor. The Big Dipper and the constellation as a whole have mythological significance in numerous world cultures, usually as a symbol of the north.The third largest constellation in the sky, Ursa Major is home to many deep-sky objects including seven Messier objects, four other NGC objects and I Zwicky 18, the youngest known galaxy in the visible universe.
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