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Read the information on Hertzsprung
Read the information on Hertzsprung

... radiates in one second, but you can think of it as how bright or how dim the star appears. The luminosity scale is a "ratio scale" in which stars are compared to each other based upon a reference (our sun). The horizontal axis represents the star’s surface temperature (not the star’s core temperatur ...
The Mazzaroth (Zodiac)
The Mazzaroth (Zodiac)

... The later people of Mesopotamia took over the old Sumerian names for the constellations and still later the Greeks adopted them. The Greeks added many names of heroes and demigods to the list of constellations. The Romans used the Greek list but translated the names into Latin. About AD 150 the Egyp ...
Document
Document

... close to us (“only” 160,000 light years away) that with Hubble, we can see stars as small as ½ the Sun even in the most crowded star clusters. Image: Anglo-Australian Observatory ...
part iv: stars i
part iv: stars i

a MS Word version.
a MS Word version.

30 Doradus - HubbleSOURCE
30 Doradus - HubbleSOURCE

... close to us (“only” 160,000 light years away) that with Hubble, we can see stars as small as ½ the Sun even in the most crowded star clusters. Image: Anglo-Australian Observatory ...
here
here

... especially Jupiter, is close to that of the Sun. • The internal structures of these planets is completely different from that of the Earth. In particular, there is no hard surface. • These planets are relatively far from the Sun (more than 5 times the Earth-Sun distance), so heating by the Sun is no ...
Nucleosynthesis and the death of stars
Nucleosynthesis and the death of stars

... • For the majority of stars (~95%, corresponding to stars with initial masses of less than 8 M-Sun), direct nuclear fusion does not proceed beyond helium, and carbon is never fused. • Most of the nucleosynthesis occurs through slow neutron capture during the asymptotic giant branch (AGB), a brief ph ...
The Sun and Stars
The Sun and Stars

... What are stars? Where did they come from? How long do they last? During most of the day, we see only one star, the sun, which is 150 million kilometers away. On a clear night, about 6,000 stars can be seen without a telescope. Ancient astronomers believed that the sun and the stars were different fr ...
hubble_refurb
hubble_refurb

... decision, and would consider sending a shuttle to repair Hubble.[Zimmerman 2] As an engineer, Griffin had previously worked on Hubble's construction, and respected the discoveries the telescope brought to the science community.[Zimmerman 2] He agreed with the National Academy of Sciences that a robo ...
STELLAR FORMATION AND EVOLUTION
STELLAR FORMATION AND EVOLUTION

... temperature of 50,000 degrees Kelvin, the star cools very slowly. Consequently, as seen through a telescope, one of these tiny stars appears to be white hot. It has become a white dwarf. As the years pass by, white dwarfs simply cool off. And as their temperatures drop, their luminosities also decli ...
1Barycenter Our solar system consists of the Sun and the
1Barycenter Our solar system consists of the Sun and the

... Orbit means to move in a curved path around another something. In astronomy, celestial bodies are generally described as moving or orbiting some other celestial body. For example, the Moon is said to orbit or revolve around the Earth. The Earth doesn’t stays in position as the Moon circles it. Just ...
The solar system
The solar system

... terms. It could be hoped that expanding in a power series until a high rank would give an arbitrarily good precision. But LE VERRIER was one of the first to notice that the LINSTEDT series (since they bear that name) do not generally converge. In other words, there are terms whose denominator is ver ...
Temperate Earth-sized planets transiting a nearby ultracool
Temperate Earth-sized planets transiting a nearby ultracool

... parameter) as derived from their individual analyses does not favour this scenario. TRAPPIST-1 is a well characterized, isolated M8.0 ± 0.5-type dwarf star11 at a distance of 12.0 ± 0.4 parsecs from Earth as measured by its trigonometric parallax12, with an ...
Word Document - Montana State University Extended
Word Document - Montana State University Extended

... life has existed on the Earth for about the last 500 million years. It is still unclear exactly what chain of events lead up to the emergence of complex life on this planet. One of the factors that scientists believe to be necessary is a long period of relatively stable climate resulting from a stab ...
Galaxies – Island universes
Galaxies – Island universes

... now been measured accurately. It’s H = 70 km/sec for every additional megaparsec further out you look • Now we have our final rung in the Distance Ladder: Solve for D and get D=V/H ...
Jeopardy
Jeopardy

... Do all stars take the same path? ...
Astronomy 112: The Physics of Stars Class 1 Notes: Observing Stars
Astronomy 112: The Physics of Stars Class 1 Notes: Observing Stars

... calibrated off human senses, the system is, like human senses, logarithmic. Every five magnitudes corresponds to a change of a factor of 100 in brightness. In this class we will not make any further use of the magnitude system, and will instead discuss only fluxes from stars, which can be measured d ...
Slide
Slide

... • Earth-based measurements can typically be made to 0.03”, or to a distance of ~30 parsecs (pc) • Distances to several thousand stars are known this way. • The Hipparcos satellite extends the distance to ~200 pc, so distances to nearly one million stars can be measured with parallax. ...
Star Classification and its Connection to Exoplanets.
Star Classification and its Connection to Exoplanets.

... exoplanets, at 38%. The second pie chart uses data from the percentage of stars that have planets, so at around 6.6% of a total of around 18%, G stars make up about 37%, again the dominant planet host. Looking at the inferential statistics, one can conclude even more information from the hypothesis ...
to get the file
to get the file

... the Celestron, but we could not track many of the stars on our bright star list due to the fact that they either rose after dawn or set before dusk ...
TOOLS IN ASTRONOMY SPECTROSCOPY
TOOLS IN ASTRONOMY SPECTROSCOPY

... Introduction: Classifying stars based on brightness is somewhat problematic. A star’s apparent brightness can be affected by its distance from the observer, its size, or by the presence of interstellar dust. Instead, astronomers classify stars based on the major components of their spectra. Much lik ...
Cosmic Distance Ladder Terrence Tao (UCLA)
Cosmic Distance Ladder Terrence Tao (UCLA)

... At any given time, one can measure the position of the Sun and Mars from Earth, with respect to the fixed stars (the Zodiac). ...
A-level Physics (Specification A) Teacher guide Teacher guide
A-level Physics (Specification A) Teacher guide Teacher guide

... specification are applied to the design of telescopes. The relative merits of the two basic methods – reflecting and refracting – are discussed as well as the influence the design of the telescopes has on how well an image can be produced. Finally, the workings of a very common device used to collec ...
Star-D_Teacher_Guide - The University of Texas at Dallas
Star-D_Teacher_Guide - The University of Texas at Dallas

... * A white dwarf is a very small, hot star that is no longer on the main sequence ...
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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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