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Color and Temperature of Stars
Color and Temperature of Stars

... A star's color depends on its surface temperature. Astronomers measure star temperatures in a metric unit known as the Kelvin. One Kelvin equals exactly 1 Celsius degree (1.8 Fahrenheit degree), but the Kelvin and Celsius scales start at different points. The Kelvin scale starts at -273.15 degrees C ...
FOURTH GRADE UNIVERSE - Math/Science Nucleus
FOURTH GRADE UNIVERSE - Math/Science Nucleus

... Stars are balls of gas that emit energy created by fusion, a nuclear reaction within the star. There are many sizes and brightness of stars, ranging from super hot, blue-white stars (over 20,000°K) to cool red stars (3,000°K). Our Sun is a medium yellow star, towards the small and cool end of the sp ...
newsletter - Thanet Astronomy Group
newsletter - Thanet Astronomy Group

The Sculptor dwarf irregular galaxy SDIG: present and past
The Sculptor dwarf irregular galaxy SDIG: present and past

... excess of 0 mag, whereas LW81 suggested that the colour excess for SDIG should be similar to the colour excess of the Sculptor dwarf spheroidal, for which studies of the colourmagnitude diagram reveal E(B - V) = 0.02 mag. The RC3 (de Vaucouleurs et al. 1991) lists a colour excess of zero, which is d ...
15_Testbank
15_Testbank

... D) Because there is still uncertainty over what generates the energy in stellar cores. E) Because it refers to stellar masses and these were difficult to measure accurately. Answer: B 16) Which of the following statements about spectral types of stars is true? A) The spectral type of a star can be u ...
Recitation Ch6
Recitation Ch6

... 6-13 Effect on blood of walking. A person is walking, his arms swing through approximately a 45° angle in (½) s. As a reasonable approximation, we can assume that the arm moves with constant speed during each swing. A typical arm is 70.0 cm long, measured from the shoulder joint. (a) What is the ac ...
Ch 13 Death of Stars(4-5?-13)
Ch 13 Death of Stars(4-5?-13)

... • Black Holes: M more than 3 solar masses. Nothing stops the collapse and produces an object so compact that escape velocity is higher than speed of light; hence, not even light can escape. •NOTE: these are the masses of the dead stars NOT the masses they had when they were on the main sequence ...
Ch. 13 Death of Stars(11-16-10)-3
Ch. 13 Death of Stars(11-16-10)-3

... • Black Holes: M more than 3 solar masses. Nothing stops the collapse and produces an object so compact that escape velocity is higher than speed of light; hence, not even light can escape. •NOTE: these are the masses of the dead stars NOT the masses they had when they were on the main sequence ...
JUPITER AND SPEED OF LIGHT
JUPITER AND SPEED OF LIGHT

... and Europa, show similarities to the terrestrial planets, such as volcanism and internal heating [4]. The four largest satellites, known also as “Medician Stars” (named after Galilei's tutor Cosimo de’ Medici) or the “Galilean moons” were first discovered in January 1610 by Galileo Galilei. As he wr ...
VLT/FORS Surveys of Wolf-Rayet Stars beyond the
VLT/FORS Surveys of Wolf-Rayet Stars beyond the

... Once the core hydrogen is exhausted, the star leaves the main sequence and becomes a blue supergiant, and ultimately a red supergiant (RSG) for stars with initial mass up to perhaps 20–30 MA. Observationally, there is an absence of luminous RSGs, known as the Humphreys-Davidson limit, such that init ...
the K-12 Teacher Resource Packet for
the K-12 Teacher Resource Packet for

... Astronomy comes from the Greek words for ‘star’ and ‘law.’ As a science, it focuses primarily on the study of space, its objects, and phenomena outside of the Earth itself. The Development of Astronomy Astronomy is considered one of the oldest sciences. The study of the stars and plants began more o ...
Starry Dome: Astronomy in Art and the Imagination
Starry Dome: Astronomy in Art and the Imagination

Recent Measurements of Millisecond Pulsar Masses
Recent Measurements of Millisecond Pulsar Masses

... New Globular Cluster Searches: 35 New MSPs! • Motivated by the spectacular Terzan 5 results (30 new MSPs to date!), we decided to use the same observing system to search for pulsars in other globular clusters. • So far we have found 35 new MSPs in other globular clusters! • Eleven of these were fou ...
Chapter 25 - Taylor County Schools
Chapter 25 - Taylor County Schools

... Mercury is only 36 million miles from the Sun and orbits it every 88 days. It has a very elliptical orbit and moves approximately 30 miles per second. Mercury rotates very slowly and its “day” is 59 Earth days. Mercury has a rocky, crust surface with many craters. This gives it the appearance much l ...
PHYS3380_110415_bw - The University of Texas at Dallas
PHYS3380_110415_bw - The University of Texas at Dallas

... ・When the star becomes convective, it moves up the AGB greatly increasing in luminosity at roughly constant temperature. Low mass stars are not, however, massive enough to reach the ignition temperature of carbon before the core becomes completely supported by degenerate electron pressure (which hal ...
Northrop Grumman Space Primer
Northrop Grumman Space Primer

Answers for the HST Scavenger Hunt
Answers for the HST Scavenger Hunt

... Image shows the Antennae galaxies, which are margining. What are the two orange blobs in the picture? The orange blobs to the left and right of image center are the two cores of the original galaxies. ...
Here - Astrophysics Research Institute
Here - Astrophysics Research Institute

... Earth's rotation axis precesses slowly, with a period of 25,600 years. This happens because the Earth is not quite spherical, but is oblate and tilted. Therefore, the direction of the Sun's gravity does not pass directly through the Earth's centre of rotation. The overall effect is that the position ...
Project 8 : Stellar Spectra: Classification
Project 8 : Stellar Spectra: Classification

The Life of the Sun
The Life of the Sun

... Helium Flash. At this point the Sun becomes what we call a Horizontal Branch Star. Now you have a new segment in the evolution of the Sun. This phase can also be called the sub-giant phase of the Star. Here you have the Star happily burning Helium, it bloats itself back out. It gets hotter in the co ...
PowerPoint - Louisiana State University
PowerPoint - Louisiana State University

... Eudoxus and MUL.APIN ...
“Astronomy Picture of the Day” Leads to a Research Breakthrough
“Astronomy Picture of the Day” Leads to a Research Breakthrough

... model as the only possible progenitor for SNR 0509-67.5. This is the first time anyone has been able to definitively identify the progenitor of a Type Ia supernova, but it is important to note that this is only for one particular system. If it were true that all Ia supernovae came from the same ty ...
Temperatures of Stars
Temperatures of Stars

Slide 1
Slide 1

... But its energy output was larger in the past; could have been 100 times brighter than the Moon as seen from Earth ...
Unit 11: Astronomy
Unit 11: Astronomy

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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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