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Common Envelope Evolution Leading to Supernovae with Dense
Common Envelope Evolution Leading to Supernovae with Dense

... by a supernova can also be considered for the white dwarf case. A white dwarf spirals into the envelope of an evolved companion and continues to the core where strong accretion gives rise to a thermonuclear explosion. This scenario would be compatible with a double degenerate origin for Type Ia supe ...
b. - UW Canvas
b. - UW Canvas

... dependence of the parallax angle on the distance an object is from Earth. If the minimum parallax angle we could measure were 0.5 arcsec, what is the maximum distance of a star that we could measure? ...
File - Mr. Pelton Science
File - Mr. Pelton Science

... diameters up to 30 million ly across. • Galaxies close together often collide to form strangely shaped galaxies or galaxies with more than one nucleus (Andromeda) ...
Living with a Red Dwarf - Center for Space and Habitability (CSH)
Living with a Red Dwarf - Center for Space and Habitability (CSH)

... the atmosphere, and heat it to the point where the atmosphere can escape to space. • i.e. it’s the rocket fuel that brings molecules up to escape velocity and can launch atmosphere out of the gravity well. • Shorter wave ultraviolet drives photochemistry, and can break up heavy molecules into lighte ...
pierrehumbert_lecture_1
pierrehumbert_lecture_1

... the atmosphere, and heat it to the point where the atmosphere can escape to space. • i.e. it’s the rocket fuel that brings molecules up to escape velocity and can launch atmosphere out of the gravity well. • Shorter wave ultraviolet drives photochemistry, and can break up heavy molecules into lighte ...
Distance Measures: Parallax
Distance Measures: Parallax

... this background? This is because the center of your eyes are a few centimeters apart from each other, so each eye as a different point of view. Because stars are SO far away, their parallaxes are most conveniently measured in seconds of arc (arc seconds). The angular size of your thumb held at arm’s ...
CHAPTER 6 THE CELESTIAL SPHERE
CHAPTER 6 THE CELESTIAL SPHERE

Distance Measures: Parallax
Distance Measures: Parallax

Astronomy - Great Smoky Mountains Institute at Tremont
Astronomy - Great Smoky Mountains Institute at Tremont

... lamp, of course, is the sun. Have each student stand with his or her back to the lamp and hold the moon ball up at arm’s length so that some light shines on it. Explain that just like the Earth has day and night, so does the moon. Ask them to point to where it is night on their moons. Why is it nigh ...
doc
doc

... the 1880s when E. C. Pickering and Annie Cannon began to analyse the emission spectra of the visible stars. The stars they examined were placed into several ‘spectral classes’, each class being designated by a letter of the alphabet. Eventually the number of spectral classes was reduced to seven, th ...
A6 - Vicphysics
A6 - Vicphysics

... observing session and Jupiter is visible try and have your students observe it at the start of the session. See if the Giant Red Spot is visible. Also note the relative positions of the four Galilean moons (not all of them may be visible). View it again after a few hours and see if they can detect a ...
Lecture 2
Lecture 2

... • Andromeda (M31): largest and most massive • More than 1/3 are dwarf ellipticals ...
September - Rose City Astronomers
September - Rose City Astronomers

... The 600 power telescope, due to its popularity, was remarketed by a number of different companies with their own model numbers. Meade ran continual ads for the small refractor during the 1970s, and labeled it their Model #300 (or #305 for 1 ¼" accessories—they changed the color of the dewcap to whit ...
2015.09.20
2015.09.20

... Twenty-Fifth Sunday in Ordinary Time: 9/20/15—5:00 PM, 7:00, & 8:30 AM I have here a bottle of Brasso for cleaning brass products, a container of flying insect spray, and a can of Comet cleanser. One thing they all have in common is that these products are great in doing the things they are designed ...
Chapter 7 Formation of Stars
Chapter 7 Formation of Stars

... Formation of Stars Substantial direct and indirect information indicates that stars are born in the clouds of gas and dust that we call nebulae. • Basics are well understood, many details are not. • We shall have to gloss over various sticky points with assumptions that will be justified by the obse ...
Chapter 8 Formation of Stars
Chapter 8 Formation of Stars

... Formation of Stars Substantial direct and indirect information indicates that stars are born in the clouds of gas and dust that we call nebulae. • Basics are well understood, many details are not. • We shall have to gloss over various sticky points with assumptions that will be justified by the obse ...
VENUS: The Dual Goddess and Star Goddess
VENUS: The Dual Goddess and Star Goddess

... This, I believe, has a fuller and richer psychological implication for the person who possesses the Uranian (Evening Star) Venus versus the Pandemos (Morning Star) Venus. The Pandemos Venus is one who inhabits the earth, is connected to the physical world and the physical sensations of the body, and ...
Chapter 12: The Life Cycle of Stars (contʼd)
Chapter 12: The Life Cycle of Stars (contʼd)

... •  the period of a massive star's life when carbon, nitrogen, and oxygen are fusing in different shells outside the core •  a type of hydrogen fusion that uses carbon, nitrogen, and oxygen atoms as catalysts •  the process by which helium is fused into carbon, nitrogen, and oxygen •  the perio ...
As far as - Sangeeta Malhotra
As far as - Sangeeta Malhotra

... performed spectroscopy on the HUDF target region between October 2002 and January 2003, using about 10 percent of the time that went into imaging. We quickly discovered that GRAPES is not just an extragalactic survey, for the HUDF distance scale starts within our own galaxy. The closest object we ha ...
Astronomy Timeline
Astronomy Timeline

... 130 B.C. - Greek astronomer Hipparchus develops the first accurate star map and star catalogue, and a reliable method to predict solar eclipses 46 B.C. - Julius Caesar, after consulting the astronomer Sosigenes of Alexandria, introduces the Julian Calendar, a regular year of 365 days divided into 12 ...
Colour-magnitude diagrams of the post
Colour-magnitude diagrams of the post

... Goranskii (1979) discovered an RR Lyrae star in this cluster, and constructed a light curve. The RR Lyrae is outside our frame. Placing his data for this star of V = 15.7 and (B −V ) = 0.5 on our CMD, we see that it is at the correct magnitude level of the HB, and at the RR Lyrae gap, and can be con ...
JHK standard stars for large telescopes: the UKIRT Fundamental
JHK standard stars for large telescopes: the UKIRT Fundamental

... from Landolt’s (1983) equatorial UBVRI standards and the compilation of potential Hubble Space Telescope (HST ) reference sources by Turnshek et al. (1990), supplemented by additional main-sequence objects with solar-like colours from the old open cluster M67 (Eggen & Sandage 1964) and subgiants fro ...
the UKIRT Fundamental and Extended lists
the UKIRT Fundamental and Extended lists

... from Landolt’s (1983) equatorial UBVRI standards and the compilation of potential Hubble Space Telescope (HST ) reference sources by Turnshek et al. (1990), supplemented by additional main-sequence objects with solar-like colours from the old open cluster M67 (Eggen & Sandage 1964) and subgiants fro ...
a changing cosmos - Whittier Union High School District
a changing cosmos - Whittier Union High School District

... of gravitational energy. A blast wave ejects the star's outer layers into space. The Crab nebula supernova remnant is incredibly bright, even though it looks quite dim at our distance from it—6,300 light-years. If we were to observe it from much closer, we would find that it puts out 1000 times as m ...
The Norma cluster (ACO3627) – II. The near-infrared Ks
The Norma cluster (ACO3627) – II. The near-infrared Ks

... making optical observations particularly sensitive to galaxies where star formation is taking place, the NIR is much less affected by short bursts of star formation and therefore a better indicator of galaxy mass (Andreon & Pelló 2000). The NIR has the advantage of high resolution and sensitivity t ...
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Perseus (constellation)



Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.
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