Kitt Peak Nightly Observing Program

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Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

Kitt Peak Nightly Observing Program

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Transcription:

Kitt Peak Nightly Observing Program Splendors of the Universe on YOUR Night! Many pictures are links to larger versions. Click here for the Best images of the OTOP Gallery and more information. M35: An open star cluster of over 300 stars. It lies at a distance of 2,800 ly, near the foot of Castor, one of the Gemini twins. Could you see the tiny cluster NGC 2158 nearby? M36: The "Pinwheel Cluster." One of three bright open star clusters in the constellation of Auriga. It lies about 4,100 ly away, is about 14 ly across, contains about 60 stars, and is about 25 million years old. M37: The "Salt and Pepper Cluster." The second of three bright open star clusters in the constellation of Auriga. It is the brightest and richest of the three. It lies about 4,500 ly away, contains about 150 stars with a diameter of about 25 ly, and is an old cluster at roughly 450 million years old. M38: The "Starfish Cluster." The third of three bright open star clusters in the constellation of Auriga. It lies about 4,200 ly away, has a diameter of about 25 ly, and is 220 million years old.

M41: An open star cluster just below Sirius, the brightest star in the sky. It contains about 150 stars spread out over 25 lightyears, and is 2,300 ly away. M44: The "Beehive Cluster." A large, bright, diffuse open star cluster containing about 400 stars. It lies fairly close at a distance of under 600 lightyears away. Another nickname: "Praesepe." M45: The "Pleiades," the "Seven Sisters," or "Subaru". A bright, nearby star cluster in the last stages of star formation. It has six to seven bright stars along with hundreds of fainter stars. It lies about 440 lightyears away and is around 100 million years old. Coma Berenices: "Berenice's Hair," a giant Y- shaped open star cluster. It is only 280 lightyears away and appears a bit east of Leo.

The Hyades is the nearest open cluster to the Solar System at about 150 light-years away and thus one of the beststudied of all star clusters. It consists of a roughly spherical group of hundreds of stars sharing the same age, place of origin, chemical content, and motion through space. The Hyades Cluster appears in the constellation Taurus, where its brightest stars form a V shape along with the brighter red giant Aldebaran, which is not part of the cluster, merely lying along our line of sight. The age of the Hyades is estimated to be about 625 million years. The cluster core, where stars are most densely packed, has a diameter of about 18 light years. However, about one-third of confirmed member stars have been observed well outside this boundary, in the cluster's extended halo; these stars are probably in the process of escaping from its gravitational influence. "Double Cluster" (NGC 884 and NGC 869): These two star clusters are a treat for binoculars and telescope alike. Each is a congregation of many hundred stars around 50-60 light years in diameter. These clusters are both about 7500 light years away. M42: The Great Orion Nebula. This is a region of star formation about 1,300 ly away. It is roughly 30 ly across and contains enough material to make 2,000 stars the size of our sun.

M31: The Andromeda Galaxy, our nearest major galactic neighbor. It is a spiral galaxy, lies 2,500,000 lightyears away and has a diameter of 220,000 lightyears. This galaxy contains as much material as 1.5 trillion suns. Venus, the second planet, is the brightest natural object in the sky other than the Sun and Moon and is often erroneously called the morning star or evening star. It is completely wrapped in sulfuric acid clouds and its surface is hot enough to melt lead. The Green Flash: A smidge of green on the top of the sun as it sets (or rises). This rare event needs just the right atmospheric conditions. Milky Way: That clumpy band of light is evidence that we live in a disk-shaped galaxy. Its pale glow is light from about 200 billion suns!

Zodiacal Light: A faint, smooth glow marking the ecliptic (the plane of the solar system). It is sunlight scattered off of the gas and dust that orbits the sun. Congratulations; this is a rare sight! The Engagement Ring: Through binoculars, the North Star (Polaris) seems to be the brightest on a small ring of stars. Not a constellation or cluster, this asterism looks like a diamond engagement ring on which Polaris shines brightly as the diamond. Your Telescope Operator and Guide. Thank you for joining me this evening! See you soon!! The web page for the program in which you just participated is at Nightly Observing Program. Most of the above images were taken as part of the Overnight Telescope Observing Program. For more information on this unique experience please visit Overnight Telescope Observing Program. Copyright 2015 Kitt Peak Visitor Center