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Skywatch
March 2008
(newest at top)
This is Dudley Observatory's Skywatch Line for Friday, March 28, through Sunday, March 30, written by Alan French.
As shuttle missions deliver new parts to the International Space Station it grows in size, and as it gets larger it reflects more sunlight, so it also grows brighter. It is now brighter than any of the stars in the night sky, including Sirius, and approaches the brightness of Venus when it is high in our skies. You'll have a chance to see the ISS on each night over the weekend. As an added bonus, you'll also be able to see the Jules Verne – the Automated Transport Vehicle – that was built to deliver supplies. It does not appear as bright as the ISS, being smaller, but is as bright as an average star.
Some times will be given in hours, minutes, and seconds. Be sure to set your watch to the correct time.
On Friday night the ISS will appear moving up from the south southwestern horizon at 7:36 PM. It will be highest at 7:38:32 when it will be 35 degrees above the southeastern horizon, and will vanish in the east northeast at 7:41:12. Its path will bring in up just below Sirius, the brightest star in the night sky, across the southeastern sky, and then below Saturn. The fainter Jules Verne will follow almost the same path across the sky about two and a half minutes later. It may be somewhat difficult to spot because evening twilight will still brighten the sky.
The best and highest path this weekend will be Saturday night, and the current forecast is for clear skies. The ISS will first appear, coming up from the west southwestern horizon, at 7:58 PM. It will be highest and 71 degrees above the north northwestern horizon just before 8:01, and will vanish in the northeast at 8:03:32. As it crosses the sky it will pass just above Aldebaran, the brightest star in Taurus, the Bull, and then move through Auriga. Its path will then take it above the bowl of the Big Dipper, and then along the dipper's handle. The Jules Verne will follow about six minutes later.
Sunday's appearance will be the lowest of the three, but the ISS will still be east to spot. It will first appear at 8:20:22 PM in the west, reach its highest point at 8:22:57 when 29 degrees above the north northwestern horizon, and vanish in the northeast at 8:25:32. It will travel below Perseus, through the familiar “W” of Casseopeia, and below Polaris, the North Star. The Jules Verne will follow almost 11 minutes later. This is the latest of the three passes, and at the later hour, with darker skies, the Jules Verne should be easy to see.
This is Dudley Observatory's Skywatch Line for
Friday, March 21, through Sunday, March 23, written by Alan French.
The Moon was full early in the afternoon on Friday, so a bright waning
gibbous Moon will dominate the night sky this weekend. If you look toward
the east southeast on Saturday night at 9:45 you'll find the Moon almost
twelve degrees above the horizon. To the lower left of the Moon you'll see
the star Spica, the brightest star in the constellation Virgo. The Moon
will be close to Spica all night.
Star parties.are gatherings of amateur astronomers and their telescopes to
enjoy views of the night sky. Many clubs hold star parties, and they are
usually held at sites away from city lights. They are also often open to
the public. The local club, the Albany Area Amateur Astronomers, holds
public star parties at a variety of locations. The complete schedule for
“Star Parties West” for 2008 has just been published. It includes star
parties held in Indian Meadows Park in Glenville, and at George Landis
Arboretum in Esperance.
Indian Meadows Park is just off of Droms Road, not far from the YMCA, so
it is convenient and easy to reach for many people. It offers a good view
of the night sky, but suffers from light pollution. Most star parties
there are held when the Moon is visible. Landis Arboretum offers a fine
view of the night sky, and is away from significant light pollution,
offering dark skies. Star parties there are held when the skies are
moonless.
Both schedules are available on the web. Visit
www.timesunion.com
<http://www.timesunion.com/>, and click on “communities” in the menu
on the left side of the page. Scroll down and enter “astronomers” in the
Group search box. This will return a link to the club's web page. Click on
that, and when you get to the Albany Area Amateur Astronomers' page,
choose “Star Parties.” This will bring up a list of dates, and links to
maps for the star party locations.
If you do not have web access, or prefer a printed copy of the star party
schedule, call 374-8460 and ask to have one mailed to you.
For stargazers in the eastern part of the Capital District, there are also
star parties in Grafton Lakes State Part and other locations. These are
also listed on the web page.
One of the largest shows of equipment for amateur astronomers is at
Rockland County Community College in Suffern, NY, which is a two to three
hour drive from anywhere in the Capital District. The Northeast Astronomy
Forum, or NEAF, for short, features more than 80 vendors, world renowned
speakers, classes for beginners, one of the largest safe “solar” star
parties, and is preceded by a two day imaging workshop. This year NEAF is
being held on April 26 and 27. Visit
www.rocklandastronomy.com/neaf.htm
<http://www.rocklandastronomy.com/neaf.htm> for full information.
Perhaps I'll see you at NEAF, or a future star party.
Skywatch line for Wed. & Thurs., March 19 & 20, 2008:
by Ray Bogucki
At precisely 1:49 a.m., EDT on Thursday, March 20, the center of the Sun will cross the celestial equator as it moves north. This event is known as the vernal equinox and it marks the official beginning of Spring. Several special circumstances are connected to the vernal equinox. On Thursday, the Sun will rise due east on the theoretical horizon, spend 12 hours in the sky, and set due west, again on the theoretical horizon. It is one of the two days in the year when a line from the center of the Sun to the center of the Earth is precisely perpendicular to the rotational axis of the Earth. From that day on, the angle will decrease slowly from 90 degrees until June 20, at the summer solstice, when the Sun-Earth line makes an angle of 66 and a half degrees with the northern end of Earth's rotational axis, its maximum tilt toward the Sun. This tilt places the Sun at its maximum height in our noontime sky for the year, and gives us about 15 hours of sunlight. The vernal equinox also marks the day when the northward motion of the Sun reaches its maximum rate, giving us the maximum rate of increase in the number of sunlit hours each day. At the unique location of theNorth Pole, the Sun will reappear, after an absence of six months, circling around the horizon like the hands of a gigantic clock. It will then remain above the horizon for six months of continuous daylight until it sets at the autumnal equinox in September for six months without the Sun. If we define one day as the time period from one sunrise to the next, one day at the North Pole is just one year long.
On Friday, the Moon reaches its Full phase, rising in the east as the Sun sets in the west. The time of Full Moon is not a favorite with astronomers who often seek out faint galaxies and nebulas for observing. The Full Moon brightens the sky and washes out faint objects. But bright objects, such as planets, are still viewable. Mars, currently located near the feet of the Gemini twins, continues to decrease in size and brightness as the Earth speeds away from it, but our rust-colored, near neighbor, still being explored by satellites and rovers, remains a lure. Saturn, still outshining the nearby bright star Regulus, high in the southeast at nightfall, remains one of the most glorious objects in the night sky. The rings are tilted from our line of sight by 9 degrees. The angle of tilt will decrease during the year until at next Christmas time the rings will form a thin line, looking like a knitting needle stuck through a ball of yarn. Saturn is well past opposition and the Sun is now shining on it partly from the side. In a telescope, look for the shadow of the planet falling on the rings behind it and giving a wonderful 3-dimensional aspect to the view.
This is the Skywatch Line for Monday and Tuesday, March Seventeenth and Eighteenth.
by Joe Slomka
The Sun sets at 7:01 PM, with night falling at 8:39. Dawn breaks at 5:26 AM and ends with sunrise at 7:01 AM.
After sunset, the Moon is the first thing we see, high in the South. Saturn will be next. Saturn appears golden, compared to the star Regulus, to Saturn's immediate West. Mars is the last planet to pop into view. This Mars-Moon-Regulus-Venus line is quite impressive on Monday nights, spanning almost fifteen degrees. Tuesday night finds the twelve-day-old Moon even closer to Regulus and Saturn; their lineup should occupy a single binocular view.
Mars appears high in the southeast, near Castor's foot, in Gemini. Mars also lies within a binocular view of the open star cluster M-35. This star cluster can be visible to keen-eyed observers on the best, and darkest, of nights. In binoculars, it appears as a hazy sprinkling of stars. A telescope shows curves of stars with an orange star in the middle. By midnight, Mars is high in the southwest; it sets about 3:20 AM.
Gemini is an ancient constellation. The constellation was recognized as “Twins” by many cultures. Castor and Pollux, in Greek legends, were the sons of a mortal and Zeus. They crewed the legendary Argonaut. Ancient sailors prayed to them for a safe voyage. The phrase “By Jiminy” harks back to an ancient oath. The stars are approximately equally bright.
Tuesday's Moon sets about daybreak, with Saturn setting an hour later. Wednesday's Moon sets thirty minutes after first light. Saturn sets a half-hour before Sunrise.
Meanwhile, Jupiter has risen about 4 AM. Jupiter appears off the handle of teapot-shaped Sagittarius. Jupiter glows amid dimmer Milky Way stars. The setting Saturn and rising Jupiter occupy most of brightening sky.
The final set of planets is Venus and Mercury. They rise within minutes of each other; consequently they are quite close, again within a single binocular field. Venus is the brightest and first seen. In telescopes, Venus appears almost "full," while Mercury is two-thirds illuminated. Both planets rise later daily, and are so low that local obstructions may prevent observation.
Clear Skies
Joe Slomka
This is Dudley Observatory's Skywatch Line for Friday, March 14, through Sunday, March 16, written by Alan French.
The Moon was at first quarter early Friday, so a waxing gibbous Moon will dominate the evening hours over the weekend. This would be an ideal weekend to explore the lunar surface. Even binoculars will reveal some of the mountains and craters, and any birding scope or astronomical telescope will reveal a wealth of details. The Moon is best observed when it is high in the sky, and the Moon's path is now taking it well above the horizon. It is highest when it is due south, and this will happen at convenient times this weekend.
The Moon will be highest at 7:30 PM on Friday night, somewhat before the sky is completely dark. Be sure to look for reddish Mars very close to the Moon on Friday evening.
On Saturday evening it will be best placed at 8:30 PM, and by Sunday night it will appear highest at 9:26. There is no need to make sure you are out at the “best” times – the lunar surface will still be very well seen as long as the Moon is more than thirty degrees above the horizon. The steadiest views, however, revealing the most detail, are likely to be during the hour around when it is highest.
Although the features of the Moon are unchanging, the changes caused by the rising or setting Sun are fascinating to watch. Right now the line between light and darkness, known as the terminator, is the sunrise line, and more and more of the Moon's visible face is moving into bright sunlight. Right along the terminator shadows are longest, and detail stands out in bold relief. It is here that you will have the best view of craters and mountains.
If you look just over into the darkness you will find some areas of light. Some are mountain peaks just catching the light of the rising Sun. Others are high crater walls just seeing the first light of the lunar day. If you watch for a little while, the changes caused by the rising Sun will be obvious. More of the mountains will appear. The entire crater wall will slowly be revealed, and light will begin illuminating the craters floor. Sometimes the changes can be very striking. Also note how much things change from night to night as we move toward Full Moon.
The space shuttle Endeavor is now docked to the International Space Station. Although the pair is passing over our area in the morning sky, and the passes are somewhat low in the sky, it is always fun to see the ISS when a shuttle mission is there. The ISS will be visible Saturday, Sunday, and Monday mornings, with the highest pass on Sunday. Times will be given in hours, minutes, and seconds, and the ISS will look like a bright star gliding across the sky.
Look for the ISS on Saturday morning rising from the northwestern horizon at 6:14:32 AM. It will be highest at 6:16:56 when 23 degrees above the north northeastern horizon, and will vanish in the east northeast at 6:19:20. Its path will take it right through Cassiopeia.
On Sunday the ISS will move upward from the northwestern horizon at 6:36:37 AM. It will be 47 degrees above the north northeastern horizon at 6:39:25, and will vanish at 6:42:12 in the east southeast. Its path will take it past the front of the Big Dipper, and just above Polaris, the North Star.
The ISS will first appear at 5:25:23 AM on Monday as it moves out of the Earth's shadow 19 degrees above the north northwestern horizon. It will be highest at 5:26:26 when 23 degrees above the north northeastern horizon, and will vanish in the east northeast at 5:28:48. Its path will take it through Cassiopeia.
Skywatch line for Wed. and Thurs., March 12 and 13, 2008:
by Ray Bogucki
Last month, we experienced the once-in-four-year event of having a date of February 29 in our calendar. This year is known as a "leap year" and its history, based on the orbit of the Earth around the Sun, is quite fascinating. Many ancient societies were keenly aware of the correlation between the positions of Sun, Moon and stars in the sky and their daily activities. For example, ancient Egyptian farmers knew that when the brilliant star Sirius rose in the east just before dawn on the first day of summer, they should plant their crops in anticipation of the flooding of the Nile River which replenished nutrients in the soil.
The marvelous massive stone structure in England known as Stonehenge, was built beginning in 2800 BC as a primitive calendar and almanac. On the Yucatan peninsula in Mexico, the Mayans built a sophisticated temple to monitor, with great precision, the changes in the nighttime sky. These and many other structures were capable of predicting the exact times of equinoxes, solstices, eclipses, etc.
The production of an orderly calendar to incorporate this important information was a challenge. By the time of Julius Caesar, the measurement of dates was pretty chaotic. Most calendars at that time were based on the "tropical year", the precise length of time it took the Earth to complete one orbit of the Sun from one vernal equinox to the next. This period was known to be 365 and one quarter days. Thus, every four years, on a 365-day calendar, the date of the vernal equinox would fall back by one day. On the advice of Sosigenes, his Greek astronomical advisor, Caesar introduced, in 45 BC, the Julian calendar, in which every year divisible by four would include an extra day to keep the date of the vernal equinox constant.
The Julian calendar was in use until 1582. The problem was that the precise tropical year was not exactly 365 and a quarter days, but 365 days, 5 hours, 48 minutes and 46 seconds. By 1582, the discrepancy of 11 minutes and 14 seconds per year had dropped the date of the equinox back 10 days.
Pope Gregory XIII corrected this discrepancy by proclaiming that the day following October 4, 1582, would be October 15, thus removing the ten extra days from the year. Then, he further reformed the calendar by cleverly ordering that the leap years would remain, but those century years not divisible by 400 would not be leap years. Thus, the years 1700, 1800, and 1900, although divisible by 4, would not add the extra day, while the years 1600, 2000, etc. would remain leap years. The Gregorian calendar is the one we use today and it is accurate to one day in 33 centuries. If only the physical forces that set the Earth spinning in its orbit over 4 billion years ago had given us a tropical year of exactly 360 days, we could have 12 equal months of 30 days, and we would never have to tinker with the calendars.
This is the Skywatch Line for Monday and Tuesday, March Tenth and Eleventh.
by Joe Slomka
The Sun sets at 6:53 PM, with night falling at 8:30. Dawn breaks at 5:39 AM, ending with sunrise at 7:13.
As the sky darkens, a four-day-old Moon, high in the southwest, attracts our attention. Mars and Saturn are next to appear. Mars is moderately high in the southeast, while Saturn is much lower in the eastern firmament. Both are almost equally bright.
After nightfall, Mars is now found near Castor's foot, in Gemini. Although Mars fades and dwindles from its vivid appearance a few months ago, it is still quite bright and its red color stands out against mostly white stars. During March and April, Mars marches eastward across Gemini. Both Mars and Gemini are bright enough to track by naked eye viewing every available night
Saturn is also on the move, slowly closing in on Regulus, the brightest star in Leo. While Saturn appears small in our telescopes, it is so radiant that even small telescopes show it off. Binoculars hint at the rings; even small telescopes display the rings. While its main feature is the intricate ring system, the planet itself is worthy of study. Saturn is a smaller brother of Jupiter; both are gas giant plants - large balls of mostly hydrogen gas. Jupiter is noted for its very active systems of cloud zones and belts. Saturn has these too, although much more subtle. Patient observers with large telescopes can track these changes.
First light sees both gas giants at opposite ends of the horizon. Saturn prepares to set, while Jupiter has already risen. Both planets have moons visible to amateurs. Jupiter's can be seen with binoculars, while small telescopes capture Saturn's. Astronomical almanacs, magazines and websites help the observer identify these distant bodies.
Just before sunrise, Venus and Mercury rise within minutes of each other and appear quite low in the East. Both planets fill a single binocular field. Venus is the brightest and most illuminated. Mercury appears to Venus' upper right as a dimmer crescent copycat. These planets require an unobstructed horizon to watch their month-long pairing.
Clear Skies
Joe Slomka
This is Dudley Observatory's Skywatch Line for Friday, March 7, through Sunday, March 9, written by Alan French.
The weekend skies will be dark and moonless, except for a brief glimpse of a thin crescent young Moon just after sunset Saturday and Sunday nights. On Saturday, look for a very slender crescent ust above the western horizon at 6:40 PM. Look for it again above the western horizon at 7:30 PM on Sunday. Watch the Moon during the coming week as it moves higher into the sky and heads toward first quarter, which will occur early next Friday.
Learning the constellations is easy if you start with a familiar star pattern and work from there. Most people know the Big Dipper, an obvious pattern of bright stars that form part of the constellation Ursa Major, the Big Bear. It is an excellent guide to finding other constellations.
The Big Dipper is toward the northeast early in the evening. The four stars marking the bowl are highest and the top of the bowl opens toward the north. The three stars that form the handle dangle down toward the horizon.
As you may know, the Dipper can be used to find Polaris, the North Star, which is at the end of the Little Dipper's handle. The stars that of the Little Dipper also make up the constellation Ursa Minor, the Little Bear.
To find Polaris, start with the star at the bottom of the bowl's front. Imagine a line extending from that star, through the star at the top of the front of the bowl, and extending across the sky. The first reasonably bright star you encounter will be the North Star. If you are where the skies are fairly dark, you should be able to see the outline of the Little Dipper extending from Polaris. Under light polluted skies, you may only see Polaris and the two stars that mark the front of the bowl.
Now we can use the Big Dipper and Polaris to find the constellation Cassiopeia, the Queen. Start at the top star at the back of the Big Dipper's bowl, where the handle joins the bowl. Draw an imaginary line extending from there to Polaris, and then continue it across the sky. You'll soon come to a bright star that marks one end of a big “W” in the sky. This is Cassiopeia.
Finally, we'll journey from the Big Dipper to Leo, the Lion. Start at the middle of the bowl's bottom. Picture a line perpendicular to the bottom and extending away and toward the southeast. It will reach a pair of bright stars – Regulus, the brightest star in Leo, and Saturn, a wandering visitor to the constellation. Regulus marks the end of a backwards question mark, which outlines Leo's head, and a triangle of stars forms the lion's hindquarters.
Saturn's largest and brightest moon, Titan, can be spotted through almost any telescope. Depending on the type of telescope you use, Titan will be either just above or just below Saturn, and less than two Saturn diameters away, on Saturday night, making identification easy.
We start daylight savings time on Sunday night, meaning we set our clocks ahead one hour and lose an hour, which we regain on the first Sunday in November – November 2. Oddly, there are no real studies that prove any major advantages to daylight savings time. Some show it provides a marginal savings of energy, and others find it actually increases energy use. For skywatchers, daylight savings time means that the mid-summer skies do not get completely dark until after 10:00 PM.
Skywatch line for Wed. and Thurs., March 5 & 6, 2008:
by Ray Bogucki
Since the spectacular pairing of Venus and Jupiter at the beginning of February, Jupiter has continued to climb higher into the eastern predawn sky, while Venus has dropped lower so that they are now about 30 degrees apart. Venus is now in a close approach to its companion inner planet, Mercury. They will appear very close together for the next few weeks. If you know a dark site that has an unobstructed view to the east, check each morning about 5:30, an hour or 45 minutes before sunrise. Venus has faded a little in brightness, but its brilliant point of light will still be easily visible to the naked eye. Binoculars will help to find Mercury in the same field of view as Venus. Check soon because the Sun rises 2 or 3 minutes earlier each day and the planets will be rising each day into a brighter sky. The other two bright planets, Mars and Saturn, are up and well placed for observing at nightfall. Mars is close to the feet of Gemini the Twins, high in the southwest, while Saturn remains close to the bright star Regulus in Leo the Lion in the southeast.
New Moon occurs on Friday, providing us with dark, moonless evening skies for the next week. This is a good opportunity to find and study an intriguing class of objects known as open star clusters. These close groupings represent stars that were formed at roughly the same time from a particular cloud of interstellar gas and dust. They are extremely useful to professional astronomers who can study the evolutionary processes in a group of stars, all of which have a similar age and composition, and lie at the same distance from the Earth.
For casual observers, the lure is their elegant structure. Perhaps the most familiar of all open clusters is the Pleiades, the seven daughters of the mythical Atlas, who was thought to support the Earth on his shoulders. It can be found one or two fist-widths to the northwest of Aldebaran, the bright red eye of Taurus the Bull. At a casual glance it appears as a bright fuzzy spot in the sky, but a more careful study shows 6 or 7 distinct stars, obvious even to the naked eye. In binoculars or a small telescope, the appearance of the several dozen stars, at about 400 light-years distance, is breathtaking.
About halfway between the "W" shape of the constellation Cassiopeia and the bright cluster of stars in Perseus, is another faint fuzzy patch of light which was noted by the Greek astronomer, Ptolemy, 2,000 years ago and is now called the Perseus Double Cluster. In binoculars or a small telescope, we see two separate clusters very close together, each with over 100 stars. The western cluster lies a distant 7,200 light-years away and is a remarkably young 5 million years old. The eastern group is a little farther away and even younger at about 3 million years old. These two sparkling clusters, appearing to lie close together along our line of sight, are considered to be one of the most remarkable sights in the night sky.
This is the Skywatch Line for Monday and Tuesday, March
Third and Fourth.
by Joe Slomka
The Sun sets at 5:45 PM, with night falling at 7:21. Dawn breaks
at 4:51 AM, ending with sunrise at 6:25.
As the sky darkens, the bright star Sirius and the Red Planet Mars occupy
the southeast. Mars is due south, and highest, at 7 PM. Mars shines near
the foot of Gemini. It is less than three degrees from the star cluster
M-35. Both objects easily fit in your binocular or telescope field. Mars
is too small and dim for detailed observation. Mars sets before 3 AM.
Saturn remains beneath Leo. Saturn is about midway between Regulus, the
constellation's brightest star, and a cluster of three galaxies. The
Saturn-Regulus pair can be seen in binoculars; a telescope is required to
see the galaxy cluster-planet pair. Saturn is visible for most of the
night. The best time to observe it is about 11:30 PM, when it is highest.
Telescopes show off the rings and several of its many moons.
First Light sees Saturn ready to set in the West, and Jupiter just risen
in the East. Jupiter lies just above teapot-shaped Sagittarius.
On Tuesday, a thin crescent Moon appears between Jupiter and a
Venus-Mercury cluster; Wednesday forms a trio with the Venus-Mercury pair.
Mercury and Venus share a binocular field for most of the month. Both rise
shortly before 5:30 AM Low in the East. Venus is much brighter and
larger. Venus also appears as a fatter crescent. Horizon obstructions may
frustrate early observers.
If you live in dark rural areas, the next two weeks are special. The Solar
System is full of dust, which varies from small pebbles to smoke
particles. When the position of the Sun and ecliptic are right, a faint
glow may appear in the West, just after sunset. This phenomenon is called
Zodiacal Light. It is best seen about a half hour after twilight ends.
Sunlight is scattered by dust particles, which are positioned between the
Sun and Earth. Moonlight, atmospheric pollution or haze can erase the
effect. But, if you are lucky, you will see a pillar of light rising from
the horizon in the direction of the Sun.
This is Dudley Observatory's Skywatch Line for Friday,
February 29, through Sunday, March 2, written by Alan French.
The Moon was at last quarter late Thursday night, so the Moon will not
rise until well after midnight over the weekend and most of the night will
be dark and moonless. Early in the evening, just after the last remnants
of twilight have vanished, the constellations of winter are toward the
south. This would be a good weekend to learn your way around these
distinctive star patterns, or reacquaint yourself with old friends.
The easiest way to learn the brighter stars and constellations is with a
planisphere. A planisphere has a wheel that shows all the stars possibly
visible in our skies, with outlines of the constellations. This wheel fits
inside a sleeve, and a window shows what stars are visible at any
particular time on any night of the year. The wheel just has to be turned
so that the date on its outside matches the time on the window.
Planispheres are often available at bookstores, or perhaps you have one
sitting, forgotten, in a drawer somewhere. (Just make sure it applies to
43 degrees north latitude.) If you don't have one, a quick and easy
project is to make your own. You can download the two printed pieces you
need from the web, print them, and follow the simple instructions
included. For the planisphere “kit,” visit www.lhs.berkeley.edu/starclock/skywheel.htm <http://www.lhs.berkeley.edu/starclock/skywheel.htm> and print out the
parts and instructions for Uncle Al's Skywheel. If your family is going to
join you learning the stars, I suggest a planisphere for each person.
One problem using a planisphere is maintaining your night vision. As you
may have noticed, it takes your eye 15 to 20 minutes to get used to the
dark, and more stars are visible once you are dark adapted. If you use a
regular flashlight to look at your planisphere, you will lose your night
vision, and have to start getting used to the dark all over again. The
solution is to use a dim red flashlight. It should be just bright enough
to read the planisphere when you are dark adapted. You can cover a
flashlight with red plastic, tissue paper, thin paper, or nail polish to
make your own astronomer's flashlight.
To use your plansisphere, set it so the time and date correspond to when
you are out under the stars. Note there are compass directions – north,
west, south, and east - written around the outside of the planisphere. If
you are looking south, hold “south” at the bottom. If you decide to
explore the northern sky, hold “north” at the bottom.
Early risers on Monday will have a chance to see the International Space
Station and a pretty paring of the Moon and Jupiter.
The ISS will be moving out of the Earth's shadow, low in the southwest,
and will first appear near Spica, the brightest star in the constellation
Virgo, at 5:26:22 AM. It will be highest at 5:28:39 when it will be 64
degrees above the southeast horizon, and will vanish below the east
northeastern horizon at 5:31:31. The path of the ISS passes below Hercules
and Lyra, and then moves down through the lower part of Cygnus, the Swan.
After watching the ISS look toward the southeast. You'll see a pretty
crescent Moon with bright Jupiter about ten degrees above and somewhat to
the right of it. |