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 The Night Sky

 

solar eclipse

 Solar and Lunar Eclipses
Eclipses of the sun and moon are rare and beautiful sights. The cause of each type of eclipse is essentially the same: the sun, Earth, and moon form a straight line in space with Earth’s shadow falling on the moon (a lunar eclipse) or the moon’s shadow touching Earth (a solar eclipse). However, the visual result is strikingly different.

Nothing quite matches the experience of viewing a total solar eclipse. The coal black disk of the moon set against the ghostly, pearly white corona, with solar prominences arranged like a necklace of rubies around the lunar limb, is a sight that will remain forever etched in a viewer’s mind. During an annular eclipse, the moon doesn’t completely cover the solar disk; at mideclipse a thin ring of sunlight briefly encircles the lunar disk. A partial solar eclipse isn’t as dramatic because the moon never completely hides the sun. Solar eclipses occur only during new moon; 

An eclipse of the moon can be equally dramatic, as the lunar surface turns a colorful red-orange hue from sunlight that’s filtered and bent by Earth’s atmosphere before it reaches the moon. Earth’s dark, central shadow is the umbra; for most observers a lunar eclipse really starts when the umbra first touches the lunar surface. The lighter shadow that surrounds the umbra is the penumbra and is difficult to detect. Totality occurs when the moon is completely immersed in Earth’s umbra.

Lunar Occultations
As the moon moves through the sky, it occasionally occults (passes in front of) a planet, star, or other celestial body, snuffing out its light. The object reappears on the moon’s opposite side up to an hour later. When a star is occulted, its light vanishes (and reappears) instantly. But when a planet or a star cluster is involved, the event takes longer to unfold.

 The Red Planet is about to be spectacular (This infor was for 2006) but very important for everyone alive at this time.
This month and next, Earth is catching up with Mars in an encounter that
will culminate in the closest approach between the two planets in
recorded history. The next time Mars may come this close is
in 2287. Due to the way Jupiter's gravity tugs on
Mars and perturbs its orbit, astronomers can only be
certain that Mars has not come this close to Earth
in the Last 5,000 years, but it may be as long as
60,000 years before it happens again.

The encounter will culminate on August 27th when
Mars comes to within 34,649,589 miles of Earth and
will be (next to the moon) the brightest object in
the night sky. It will attain a magnitude of -2.9
and will appear 25.11 arc seconds wide. At a modest
75-power magnification

Mars will look as large as the full moon to the naked eye.
Mars will be easy to spot. At the
beginning of August it will rise in the east at 10p.m.
and reach its azimuth at about 3 a.m.

By the end of August when the two planets are
closest, Mars will rise at nightfall and reach its
highest point in the sky at 12:30a.m. That's pretty
convenient to see something that no human being has
seen in recorded history. So, mark your calendar at
the beginning of August to see Mars grow
progressively brighter and brighter throughout the
month.  Share this with your children and grandchildren.

NO ONE ALIVE TODAY WILL EVER SEE THIS AGAIN

The Night Sky This Week

For  more info contact the 

nightskyinfo.com

The Planets

Mercury

 

Mercury is immersed deep in the glow of the Sun and cannot be observed until mid-January 2008, when it makes a brief appearance in the evening sky.

 

Venus

 

Early-morning skygazers will enjoy finding Venus. Our "sister planet" comes up in total darkness, about three hours before the first glimmer of dawn, and blazes in the southeast an hour before sunup.

 

Venus shines at magnitude -4.1, about ten times brighter than Sirius, the brightest of all stars. In fact, the planet is so bright, that you might try sighting it on very clear days with the naked eye after sunrise. If you can keep track of where it is through sunup, you should still be able to see it as a tiny white "speck" against the blue daytime sky.

 

Aim your telescope at Venus and you will see a 69-percent lit disk that spans 17" - the planet's phase waxes imperceptibly, to 71-percent lit, during the week. Simultaneously, the apparent size of Venus' disk shrinks from 17" to 16", as the planet's distance from Earth increases from 94 million miles to 97 million miles. Such changes are explained by the fact that Venus is on a smaller, faster orbit than Earth, and the morning star is now rapidly receding from us.

 

Finder map - one hour before sunrise, looking southeast.

 

Mars

 

Mars
The Red Planet reaches opposition
this month, and appears bigger
through a telescope than any time
until 2016. NASA
[larger image]
The most spectacular planet this month has to be Mars. December brings the Red Planet closer to Earth than at any time since the winter of 2005. If you have a telescope, even a small one, now is certainly the time to get it out.

 

Mars pokes above the horizon during evening twilight, among the background stars of Gemini the Twins, and is high up in fine view in the east by 9 P.M. local time. It gleams so brightly and with such a distinct ruddy hue, you will not confuse it with any other object. Through a telescope, the planet measures 16" across - nowhere near the record- breaking apparent diameter of 25" in August 2003, but bigger than Mars will appear again until 2016.

 

Mars is never easy to study visually, but this will be
your best chance! The best telescope for planetary observing is a large, high- quality refractor or a large Newtonian reflector with first-rate mirrors in perfect collimation (optical alignment). Fine planetary views can also be obtained with Schmidt-Cassegrains; there are no hard and fast rules in this respect.

 

In the end, the limiting factor is atmospheric seeing. Studying the planets means spending a lot of time at the eyepiece, waiting for brief glimpses through steady air. Just as important, the longer you watch, the better trained your eye becomes.

 

Finder map - 8 P.M. local time, looking east.

 

Jupiter

 

Jupiter is lost in the evening twilight; it sets just minutes after the Sun. Nevertheless, it is out there, on the other side of the Sun from Earth and 580 million miles away from our planet. It will return to view in mid-January 2008, low in the morning sky.

 

Saturn

 

Illustration of Saturn's Rings
This illustration shows a close-up of Saturn's
ring system. The rings are believed to have
formed after an icy moon was broken up
by an impact with a comet or asteroid.
NASA/CXC/M. Weiss
[larger image]
Saturn shines at magnitude +0.7 and remains in Leo throughout December, nearly due east of 1st-magnitude Regulus (Alpha Leonis). The planet rises an hour before midnight and climbs high enough by 5 A.M. local time to offer excellent views through a telescope. Saturn's disk measures 19" across this week, while the rings span 43" and appear closer to edge-on now than they have since 1997.

 

Saturn is the most striking member of our planetary family. With an equatorial diameter of about 75,000 miles, it is the second largest planet circling the Sun. Appearing as a bright yellowish object in our night sky, Saturn presents a maximum
apparent diameter of 20" and reaches magnitude -0.2 at opposition, when it lies closest to the Earth. This is about ten times fainter than Jupiter.

 

The planet's most attractive feature is, of course, the magnificent ring system. The rings consist of countless particles of water ice, ranging in size from small grains to irregularly shaped pieces generally a few feet across. It is interesting to note that if all of the material of the rings of Saturn were formed into a single moon, the moon would be about the mass of Janus (one of the smallest of Saturn's moons) and only 1/20,000 the mass of the Earth's Moon.

 

Finder map - one hour before sunrise, looking southwest.

 

Uranus

 

William Herschel
A portrait of William Herschel,
discoverer of Uranus. Library of
Congress
[larger image]
Glowing at magnitude +5.9, Uranus pops into view in binoculars, even from moderately light-polluted sites. Look for it in Aquarius the Water-bearer, 2° southwest of 4th-magnitude Phi Aquarii. Through a telescope, the planet displays a disk 3.4" in diameter sporting a distinct blue-green hue.

 

The famous German-English amateur astronomer William Herschel discovered Uranus in 1781, and once astronomers realized it was an unknown world, the size of the solar system doubled. Uranus was the first new planet to be found since antiquity, but at the outset it was not at all clear that a new world had been spotted.

 

Herschel's telescope provided the world's best view of the new object, but even Herschel thought he had discovered a comet. His journal record for his first sighting on Tuesday, March 13, 1781,
documents his suspicion: "In the quartile near Zeta Tauri the lowest of the two is a curious either Nebulous Star or perhaps a Comet". Four nights later, Herschel observed it again. Despite its lack of a tail, he concluded - because it had moved - that he had a comet on his hands.

 

Independent observatories soon verified the existence and motion of Herschel's new "comet", but attempts to determine its orbit and predict its position failed. It was obvious that this object was much more distant than anyone had thought, and calculations soon showed it to be a planet, moving far beyond the orbit of Saturn. After some discussion it was named Uranus, after the Greek god of the sky.

 

Finder map - field width 15°, stars to magnitude +8.

 

Neptune

 

Neptune is about six times dimmer than Uranus, but if you have access to a dark, clear sky and carefully examine the finder map below, you should have no trouble in finding it with a small telescope. The planet lies among the stars of Capricornus, the Sea Goat, a mere 2° northeast of 4th-magnitude Iota Capricorni.

 

Telescopes show little of Neptune - even though it is four times Earth's diameter, Neptune lies 2.85 billion miles away and so appears only 2.4" across. You are going to need at least a 4-inch telescope with a magnification of no less than 150-power, just to turn Neptune into a tiny blue dot of light. The best views are in the early evening, when Neptune lies in the southwest.

 

Neptune takes almost 165 years to complete one journey around the Sun, so that it was discovered less than one "Neptunian year" ago. Like Uranus, Neptune shows a light bluish color (from methane in the atmosphere). The main constituents are molecular hydrogen and helium; methane makes up a minor amount.

 

Neptune's atmosphere is marked by cirrus clouds and large storms, most notably the Great Dark Spot. This darker bluish-gray region circling the planet's Southern Hemisphere rotates counterclockwise in a few days. A region of high pressure, the Dark Spot is surrounded by white clouds of ammonia and is similar to storms on Jupiter.

 

Finder map - field width 15°, stars to magnitude +8.5.

 

Pluto

 

The dwarf planet is too deep in the solar glare and cannot be observed until early March 2008, when it will reappear in the morning sky.

 

The Deep Sky

Taurus, the Bull, is an ancient constellation that dates back to when bulls were worshipped in the Middle East. His face is marked by the V-shaped cluster of stars called the Hyades, his glinting red eye is the bright star Aldebaran and his long horns are tipped by the stars Zeta and Beta Tauri.

 

The Hyades (also catalogued as Melotte 25) are one of the major tourist attractions in the sky. In Greek mythology they are sisters, the daughters of Aethra and Atlas (the giant who carried the heavens on his shoulders) and half-sisters to the Pleiades. The Greeks told that the Hyades nursed the infant Dionysus, a son of Zeus, and were rewarded with a
The Hyades and the Pleiades
Within the borders of the constellation Taurus
are two celebrated star groups, the Hyades
(lower left in the image) and the Pleiades
(upper right). Lynn Laux
[larger image]
place in the sky. The name Hyades means "the rainy ones", because they were associated with wet and stormy weather.

 

Legend says that there were five Hyades, but fifteen shine brighter than 5th magnitude and are visible to the naked eye. Binoculars quickly raise that number into the dozens - in fact, hundreds of stars lie inside the cluster's 5.5° span. More than 130 of them are brighter than 9th magnitude and, therefore, visible in binoculars under reasonably dark skies.

 

The brightest star in the Hyades is Theta-2 Tauri, at magnitude +3.4. It teams with magnitude +3.8 Theta-1 Tauri to form a wide naked eye double star, just southwest of brilliant Aldebaran (Alpha Tauri). Aldebaran, an orange giant star about 150 times as luminous as our Sun, looks as though it is a member of the star cluster, but it is not. It is actually a foreground object that merely happens to lie about halfway between the Hyades and ourselves.

 

Because the Hyades are so scattered, telescopes cannot take the cluster all in at once; even some binoculars cannot squeeze its full extent into their fields of view. The best view of the Hyades will be through binoculars that have fields of view between 8° and 10° in diameter. Anything less and the clustering effect will be lost.

 

To astronomers, the Hyades are one of the most important star groups in the sky, because all of the cluster's stars share a common motion. They drift slowly through space toward a point a few degrees east of Betelgeuse in Orion, a fact first demonstrated by the American astronomer Lewis Boss in 1908.

 

From the movements of its stars, the distance to the Hyades Cluster has been accurately determined - it lies 151 light-years from us. This distance can be used to derive absolute magnitudes for cluster members of different kinds, and these values are in turn used as calibrators for determinations of distances to other stellar aggregates. In this way, the distance to the Hyades is the first stepping-stone in our scale of the Universe. 

 

 
 

 

Voyager 2
An artist's concept of Voyager 2,
the only spacecraft to have
visited far-off Neptune and its 13
moons. Voyager 2 is now 7.5
billion miles from Earth, more
than twice the distance from the
Sun as Pluto. NASA/JPL
[larger image]
Neptune
Seek out Neptune in the constellation Capricornus the Sea Goat, 2° northwest of the 4th-magnitude star Gamma Capricorni. The distant world lies 2.8 billion miles from Earth and glows dimly at magnitude +7.9. Because Neptune is pretty low in the morning sky you will need at least a 4-inch telescope to see it and resolve its disk, only 2.4" in diameter.
Neptune is a cold, dark world. With a mean solar distance of 2,798 million miles (30.11 astronomical units), light levels at Neptune are more than 800 times dimmer than they are on Earth. Noon on Neptune would appear no brighter than what a human would experience at dusk on Earth. Even the Sun would take on an appearance more like a star than the bright disk seen from our home planet.

Because Neptune is so distant, so far, only one spacecraft, Voyager 2, has visited the planet - a flyby in 1989. The spacecraft observed Neptune almost continuously between June and October of that year. It measured the planet's radius and interior rotation rate, confirmed that Neptune has rings, and discovered six new moons. Voyager 2 also recorded pulses of radio emission, zonal cloud bands, and large scale storm systems with up to 1,500 miles per hour winds - the strongest measured on any planet.
The strength of the radio signals received from Voyager 2 measured just one ten-quadrillionth of a watt (1/1016). It took 40 huge radio antennas on four continents to absorb enough energy to interpret the signals.
Finder map - field width 15°, stars to magnitude +8.5.

Pluto
The dwarf planet Pluto lies in northern Sagittarius and is highest above the horizon in the predawn sky.
Pluto glows at magnitude +13.9, making it similar to many stars in this Milky Way region. As a result, it is a challenge to spot. An 8-inch telescope on a perfect night brings Pluto to the edge of visibility. For a direct view, however, you will want to use at least a 10-inch scope.
Pluto was discovered in 1930 as a result of an extensive search by American astronomer Clyde Tombaugh. Astronomers have argued since the late 1990s that Pluto's small size, less than one-fifth the diameter of Earth, and a weird tilted orbit that takes it inside Neptune's orbital path every couple hundred years make Pluto more like a Kuiper Belt body than a full-fledged planet.
On August 24th 2006, the International Astronomical Union (the organization responsible for classifying planets) passed a new definition of planet that excludes Pluto and puts it in a new category of "dwarf planet".
The two finder maps below will help you identify Pluto. First locate its general position on the coarse finder map, and after you have identified the 10th-magnitude guide star Tycho 6250-745-1 use the fine finder map which shows the position of the dwarf planet on each night of the week.
Coarse finder map - field width 4°, stars to magnitude +12.
Fine finder map - field width 1°, stars to magnitude +14.5.