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blackbody
blackbody

... 2) In the Applet, the closest temperature to 3391 K you can input is about 3364 K. The peak of the curve does indeed occur at about 900 nm which is in the infrared part of the spectrum (meaning wavelengths longer than the red light). Note the color of the star has a dusky reddish/brown appearance. Y ...
tut35 Magnitudes
tut35 Magnitudes

... Figure 4 illustrates the visibility of stars on sky background brightness based on magnitude/arcsecond2, for a trained observer with dark adapted vision. It shows why bright planets may be naked-eye visible during daylight, especially if one knows where to look. Normal daylight skies have magnitude ...
Pulsar properties - Pulsar Search Collaboratory
Pulsar properties - Pulsar Search Collaboratory

a to z of astronomy
a to z of astronomy

... the equator and ecliptic intersect. The vernal equinox occurs on or around March 21 each year and the autumnal equinox on or about September 21. The position in the sky of the vernal equinox is also known as the first point of Aries, and is the zero point for right ascension measurements. Despite it ...


... aperture telescope, this galaxy can only be seen in long exposure photographs on very large telescopes. The stars that make up sculptor are relatively faint, with Alpha Sculptor is shining at magnitude 4.3, but there are a few worth a good look: Eplison (ε) Sculptoris is a binary system with the mai ...
The Scales of Things
The Scales of Things

... Cepheid variable stars are pulsating stars, named after the brightest member of the class, Delta Cephei. Cepheids are brightest when they are hottest, close to the minimum size. Since all Cepheids are about the same temperature, the size of a Cepheid determines its luminosity. Thus there is a per ...
An Archive of Chandra Observations of Regions of Star Formation...
An Archive of Chandra Observations of Regions of Star Formation...

... The archive is designed to aid both the X-ray astronomer with a desire to compare X-ray datasets and the star formation astronomer wishing to compare stars across the spectrum. It brings together Chandra data on open clusters and other bright, variable, young stars for the study of the various physi ...
Today`s Powerpoint
Today`s Powerpoint

... 2. If you are in freefall, you are also weightless. Einstein says these are equivalent. So in freefall, the light and the ball also travel in straight lines. 3. Now imagine two people in freefall on Earth, passing a ball back and forth. From their perspective, they pass the ball in a straight line. ...
File
File

... On Table #1 below is found the name, right ascension, declination, visual magnitude, distance in light years, and spectral class of the 20 brightest stars found in Aries. Table #1 ("List of stars in Aries") ...
Vast Spaces Of The Universe
Vast Spaces Of The Universe

... Altair. It is a very conspicuous object and may be readily identified between two stars of medium brightness, the three being almost in a. line. The star above Altair, and about three times the Moon's apparent width away from it, is Gamma in Aquila ; that about four times the Moon's diameter below A ...
I Cloudy with a Chance of Making a star is no easy thing
I Cloudy with a Chance of Making a star is no easy thing

... suggesting that the balance recently tilted in favor of collapse. Other studies find evidence for external triggering. Thomas Preibisch of the Max Planck Institute for Radio Astronomy in Bonn and his collaborators have showed that widely distributed stars in the Upper Scorpius region all formed near ...
Document
Document

November News Letter - Boise Astronomical Society
November News Letter - Boise Astronomical Society

... handy, then scan downward from the middle star in Orion’s Belt. These stars represent his sword and the second star in the sword should look a little fuzzy. That fuzzy spot is located 1,300 light years away and it’s not a star. It’s a seething cauldron of star formation. Astronomers count at least 7 ...
Lesson 4. Wiens and Stefans Laws
Lesson 4. Wiens and Stefans Laws

The Final Flight of Atlantis - Westchester Amateur Astronomers
The Final Flight of Atlantis - Westchester Amateur Astronomers

14 Things You Didn`t Know About How the Sun Will Die
14 Things You Didn`t Know About How the Sun Will Die

... hydrogen and helium to densities where nuclear fusion can begin, and they are ignited, albeit for a short time. When this happens with the Sun, it will briefly be 2,100 times brighter than we see it now. 7. Some 7 or 8 billion years from now, the Sun will transform into a spectacular end state, crea ...
Measuring the masses of clusters
Measuring the masses of clusters

... and sin' = %/Dd ~ ' Note that &, ', (, and % are vectors, so must be added vectorially. Not important for the point-source case, but is important when modeling complex systems (like a cluster!) ...
A-level Physics A Question paper Unit 05 - Section 2A
A-level Physics A Question paper Unit 05 - Section 2A

... 3 (b) (ii) Give reasons for your answer to part (b)(i). ...
Compa ring between Spectroscopic and Photometric Method for
Compa ring between Spectroscopic and Photometric Method for

black holes activity
black holes activity

... A.How does the text describe the structure of the Sun? -the Sun is __________ sized, temperature, mass, radius and composition, making it easy for life to flourish on ____________ B.What happens in each layer of the Sun? -_______________- where nuclear fusion takes place which powers the Sun, found ...
Classifying Spectra PDF version - the Home Page for Voyager2
Classifying Spectra PDF version - the Home Page for Voyager2

... The spectral classes are specified by the letters O, B, A, F, G, K, M, L, T going hotter to colder. Each letter is subdivided by assigning a number 0 through 9 following the letter and going from hotter to colder. So B0 is colder than O9 and hotter than B1. Obviously not every type is shown. Origina ...
No. 53 - Institute for Astronomy
No. 53 - Institute for Astronomy

... who contributed to the study. The planets were confirmed by the NASA Infrared Telescope Facility (IRTF) and the W.M. Keck Observatory in Hawai‘i, as well as telescopes in California and Chile. The new discovery paves the way for studies of the atmosphere of a warm planet nearly the size of Earth. Th ...
1 pracovni list HR diagram I EN
1 pracovni list HR diagram I EN

... 5 Construction of H–R diagram for distant stars Use the same procedure from exercise 4 to construct a H–R diagram for distant stars at distances from 100 pc to 400 pc. To obtain data from the HIPPARCOS Catalogue of Stars decide on the correct value of the parallax (Plx). Use the same scale of axes ...
Planetary Nebula
Planetary Nebula

... What resemble dainty butterfly wings are actually roiling cauldrons of gas heated to more than 36,000 degrees Fahrenheit. The gas is tearing across space at more than 600,000 miles an hour -- fast enough to travel from Earth to the moon in 24 minutes! A dying star that was once about five times the ...
Killer Skies
Killer Skies

... luminosity and temperature. Also enables astronomers to sort the stars by their sizes. The diagram is named after its originators:Ejnar Hertzsprung in the Netherlands, and Henry Norris Russell in the United States. Note, temperature decreases to the right (unlike most graphs)!!! Historical now, so w ...
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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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