July 2, 2018 – Johnathan

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.

Big Dipper

The Big Dipper (also known as the Plough) is an asterism consisting of the seven brightest stars of the constellation Ursa Major. Four define a “bowl” or “body” and three define a “handle” or “head”. It is recognized as a distinct grouping in many cultures. The North Star (Polaris), the current northern pole star and the tip of the handle of the Little Dipper, can be located by extending an imaginary line from Big Dipper star Merak (β) through Dubhe (α). This makes it useful in celestial navigation.

Engagement Ring

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.

Teapot

The brightest stars in the zodiac constellation Sagittarius form the shape of a teapot, complete with lid, handle, and spout. The plane of the Milky Way runs through Sagittarius, and just over the spout and lid of the teapot, making it look as if steam is rising from the spout of the teapot. The center of our Milky Way galaxy is in the direction of this starry steam.

The Coathanger

Also called Cr 399, or Brocchi’s Cluster, this group of stars might remind you of a closet. The stars that make up The Coarhanger are not a part of a cluster, but instead, have randomly arranged themselves in a coathanger-like shape. Chaotic stellar orbital motion can sometimes make interesting shapes!

Boötes

Boötes has a funny name. Pronounced boh-OH-deez, this constellation’s name means sheepherder, or herdsman. It looks kind of like a kite, or a shoe. Some remember that “Boötes look like a boot” to help pick it out in the sky.

Hercules

Hercules is named for the famous hero of Greek mythology by the same name. It’s one of the larger constellations, but its stars are of only moderate brightness. The Keystone is a well known trapezoid-shaped asterism (association of stars that are not an official constellation) within Hercules. This constellation is host to M13 (Messier 13), a globular star cluster. Otherwise known as the Hercules Globular Cluster, M13 is home to 300,000 stars, and is just over 22,000 light-years away.

Leo

Leo is a fairly well known constellation, because the plane of the Solar System runs through it. Such constellations are called Zodiac Constellations. Leo has some notable, bright stars, in it to boot. The brightest of these, Regulus is at the bottom of a series of stars arrayed in the form of a sickle, or a backwards question mark. This constellation does look more or less like the side profile of a lion lying on the ground, with its head up.

Libra

Libra is a fainter constellation, but easy enough to spot, once you’re familiar with the shape. It lies along the ecliptic (the plane of the Solar System), so planets pass through now and then. The names of the two brightest stars of Libra, which are Zubeneschamali and Zubenelgenubi, come form Arabic, and mean “the northern claw”, and “the southern claw”, respectively. Libra was once considered to be part of the constellation Scorpius, the scorpion. Zubeneschamali and Zubenelgenubi were seen as the claws of the scorpion.

Lyra

Lyra is a small, but notable constellation. It is host to Vega—the fifth brightest star in the sky (or sixth, counting the Sun). Not far from Vega is Messier object 57—the Ring Nebula, which is perhaps the best known planetary nebula in our sky. Lyra’s name is Greek for lyre—a kind of harp.

Scorpius

Both the plane of the Solar System (called the ecliptic) and the plane of the Milky Way pass through Scorpius—the scorpion. As a result, you can find both the planets of our Solar System (which move along the ecliptic), and many kinds of deep sky objects in this constellation. Scorpius’s brightest star, Antares, is also known as the Heart of the Scorpion, because of it’s reddish hue and location in the chest of the scorpion. Being both red in color, and near the ecliptic, Antares is a rival of sorts to the planet Mars, which is also reddish in color, and occasionally passes through Scorpius. The name Antares means “opposing Mars”.

Virgo

Virgo’s brightest star Spica is found by following the curve of the handle of the Big Dipper (“arc to Arcturus, in Boötes, then spike to Spica”).The rest of the constellation isn’t particularly bright, but Virgo lies along the ecliptic—the plane of the Solar System, so bright planets pass through occasionally.

M104 Sombrero Galaxy

M104: A spiral galaxy like the Milky Way, nicknamed the “Sombrero Galaxy” because the lane of dust in the disk looks like the brim of such a hat. It is about 50,000 lightyears across and about 29 million lightyears away.

Ecliptic

The ecliptic is a path in the sky, forming a great circle around the Earth, which the Sun and other planets of the Solar System move along. It is formed where the plane of the Solar System intersects with the Earth’s sky.

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!

Scintillation

The twinkling of star light is a beautiful effect of the Earth’s atmosphere. As light passes through our atmosphere, its path is deviated (refracted) multiple times before reaching the ground. Stars that are near to the horizon will scintillate much more than stars high overhead since you are looking through more air (often the refracted light will display individual colors). In space, stars would not twinkle at all. Astronomers would like it if they could control the effects of this troubling twinkle.

Zodiacal Light

Zodiacal light is the faint, smooth glow marking the ecliptic (the plane of the solar system). It is sunlight scattered off of gas and dust that orbits the Sun. This is a rare sight, only visible under very dark skies, and best viewed early in the year when the Ecliptic is higher above the horizon.

M6 The Butterfly Cluster

M6, the “Butterfly Cluster” is an open star cluster, located near the tail of Scorpius, next to another open cluter: M7. Containing a few hundred stars, it is smaller than neighbor cluster M7, at about 12 light-years across, and is 1,600 light-years away.

M7 Ptolemy Cluster

M7, also known as the “Ptolemy Cluster” is an open star cluster near the “stinger” of Scorpius. It is a group of suns in a gravitational dance, 25 light-years across and about 1,000 light-years away.

M57 Ring Nebula

M57: The Ring Nebula. This remnant of a dead star looks exactly as it’s name says – a ring or doughnut shape cloud of gas. The nebula is about 2.6 lightyears across and lies about 2,300 lightyears away.

Jupiter

Jupiter is the largest planet in the Solar System, a “gas giant” 11 Earth-diameters across. Its atmosphere contains the Great Red Spot, a long-lived storm 2-3 times the size of the Earth. The 4 large Galilean satellites and at least 63 smaller moons orbit Jupiter.

Saturn

Saturn, the second-largest planet in the Solar System, is known for its showy but thin rings made of ice chunks as small as dust and as large as buildings. Its largest moon, Titan, has an atmosphere and hydrocarbon lakes; at least 61 smaller moons orbit Saturn.

Double Double (ε Lyr)

The Double-Double (ε Lyrae) looks like two stars in binoculars, but a good telescope shows that both of these two are themselves binaries. However, there may be as many as ten stars in this system! The distant pairs are about 0.16 light-year apart and take about half a million years to orbit one another. The Double-Double is about 160 light-years from Earth.

3.5 Meter WIYN Telescope

The WIYN Observatory is owned and operated by the WIYN Consortium, which consists of the University of Wisconsin, Indiana University, National Optical Astronomy Observatory (NOAO), the University of Missouri, and Purdue University. This partnership between public and private universities and NOAO was the first of its kind. The telescope incorporates many technological breakthroughs including active optics hardware on the back of the primary mirror, which shapes the mirror perfectly, ensuring the telescope is focused precisely. The small, lightweight dome is well ventilated to follow nighttime ambient temperature. Instruments attached to the telescope allow WIYN to gather data and capture vivid astronomical images routinely of sub-arc second quality. The total moving weight of the WIYN telescope and its instruments is 35 tons. WIYN has earned a reputation in particular for its excellent image quality that is now available over a wider field than ever before through the addition of the One Degree Imager optical camera.

Mayall 4 Meter Telescope

The Mayall 4 Meter Telescope was, at the time it was built, one of the largest telescopes in the world. Today, its mirror—which weighs 15 tons—is relatively small next to the mirrors of the world’s largest telescopes. Completed in the mid-’70s, the telescope is housed in an 18-story tall dome, which is designed to withstand hurricane force winds. A blue equatorial horseshoe mount helps the telescope point and track the sky. A new instrument called DESI (Dark Energy Spectroscopic Instrument) will soon be installed on the 4-meter. Once installed, DESI will take spectra of millions of the most distant galaxies and quasars, which astronomers will use to study the effect of dark energy on the expansion of the universe.

The Mayall 4 Meter is named for Nicholas U. Mayall, a former director of Kitt Peak National Observatory who oversaw the building of the telescope.

McMath-Pierce Solar Telescope

The Mc Math Pierce Solar Telescope is actually 3 telescopes-in-one. It was, at the time of its completion in the 1960s, the largest solar telescope in the world. It will remain the largest until the completion of the Daniel K. Inouye Solar Telescope (DKIST) in 2018. The Solar Telescope building looks like a large number 7 rotated onto its side. The vertical tower holds up 3 flat mirrors, which reflect sunlight down the diagonal shaft—a tunnel which extends 200 feet to the ground, and another 300 feet below ground, into the mountain. At the bottom of this tunnel are the three curved primary mirrors, which reflect the light of the Sun back up to about ground level, where the Sun comes into focus in the observing room.

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 © 2018 Kitt Peak Visitor Center


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