|
Skywatch December
2001
December 1 -
2 |
December 3 -9 |
December 10 - 16
| December
17 - 23 | December
24 - 30
| December
31
NOTE: Times given in the scripts are all local Schenectady,
New York time.
Saturday, December 1st to Sunday, December 2nd. Written by
Susan French
The moon was full this Friday at 3:49 PM Eastern Standard Time. It
was the second full moon this month, the first having occurred on
November 1. It has become traditional in recent years to call the
second full moon in a month a "Blue Moon" and the term has been
enthusiastically picked up by the popular press.
Oddly enough, this is not part of some long tradition but stems
instead from a mistake in the March 1946 issue of "Sky &
Telescope" magazine. It says "Seven times in 19 years there were -
and still are - 13 full moons in a year. This gives 11 months with
one full moon each and one with two. This second in a month, or so I
interpret it, was called a Blue Moon."
However, the author's interpretation was incorrect. He cites a
1943 "Sky & Telescope" article and a 1937 issue of the "Maine
Farmer's Almanac" as references, but neither claims that the second
full moon of the month is called a Blue Moon. Instead, the Farmer's
Almanac says there are twelve full moons in most years or three per
season. Each full moon has a name appropriate to its season, such as
the Harvest Moon, the Lenten Moon, or the Moon after Yule. When there
are 13 full moons in a year, one of the seasons has an extra full
moon for which there is no seasonal name. The Farmer's Almanac claims
that this extra full moon in a season is known as a Blue Moon. The
rules the Farmer's Almanac used to determine which of the four moons
in a season was the extra one are pretty convoluted, but paging
through old almanacs quickly shows that the full moons labeled "Blue"
were not the second full moons in a month.
But where did the Farmer's Almanac get its Blue Moon
definition? No one seems to know. Researchers have so far been unable
to find any written reference giving a calendrical meaning to the
term "Blue Moon" predating the 1937 Maine Farmer's
Almanac.
You can see the Blue Moon on Friday night very close to the bright
planet Saturn. In fact the moon will pass in front of Saturn, with
the ringed plate disappearing at 7:47:46 pm EST and reappearing at
8:46:25 pm EST. These times are for Schenectady, but will only differ
by seconds across the Capital Region.
On Saturday night, you will see that the moon has pulled quite a
distance away from Saturn, and lies almost halfway between Saturn and
the even brighter planet Jupiter. By Sunday night, the moon will be
near Jupiter.
**********************************************
Monday, December 3rd. Written by Joseph
Slomka.
The Sun sets tonight at 4:22 PM, with night falling at 6:03. Dawn
breaks at 5:29 tomorrow morning, and ends with sunrise at 7:09
AM.
As the Sun sets, two bright planet attract our attention. Mars
shines due South, while Saturn rises in the East. Mars is long past
its prime observing season, but it still holds our attention due to
its distinctive red color. As the sky darkens, Mars also points to
the distant planet Uranus only five degrees to its west. Uranus is
normally dim, about sixth magnitude, and requires help in finding it.
However, tonight, telescope users can center Mars in their finders,
and simply turn left. Uranus appears starlike, but a distinctive
blue-green color.
Saturn rises in the East, and is best observed at twilight's end.
Saturn has reached opposition, which means that it rises at sunset
and sets at sunrise - remaining up all night. Saturn is also at its
brightest in the past thirty years; its rings, tipped to about 26
degrees, are also at maximum. Even small telescopes reveal the rings
in great detail.
Jupiter rises about 6:31 PM, with the Moon rising a half hour
later. Like Saturn, it is best to view Jupiter about two hours after
planet rise, to get above the atmosphere's turbulence. Jupiter is
grand in any size telescope, but larger instruments yield greater
detail. However, lowly binoculars show four moons dancing around the
giant planet.
Brilliant Venus rises in the East just before sunrise. It is
ending is pre-dawn presentation and will not be seen after a few
days. Trees or buildings may hide this planet.
The constellation Canis Major rises tonight to Orion's lower left.
The constellation houses the brightest star visible to our skies,
Sirius, the "Dog Star". Although the word "Sirius" means "scorching,"
the ancients have connected the constellation and star with a dog.
Sirius is a blue-white double star, larger and hotter than our Sun.
It is the closest star visible to northern latitudes, and the fifth
closest star to Earth.
**********************************************
Tuesday, December 4th. Written by Jonathan
Cassidy.
That "W" is back in the sky. Of the most recognizable
constellations The "W" of Cassiopeia ranks as one of the most easily
recognized. At star parties with all ages of people there are three
constellations that stand out as most easily found and recognized.
These are: The Big Dipper; Cassiopeia and Orion.
Cassiopeia is THE constellation of Autumn. I do not understood why
the Great Square of Pegasus or the line of the head, back and leg of
Andromeda are not as recognizable.
In all cases people, no matter what the age or education, pick out
Cassiopeia before Pegasus or Andromeda. The story of Queen Cassiopeia
is not flattering to the ancient figure nor is the set of stars as
large as other prominent constellations. It might be the near equal
brightness and the "W" pattern that make it so easily picked out
these nights.
Use Cassiopeia to point your way to other interesting sites in the
night sky. See if you can find these naked eye objects: Perseus
Double Cluster; M31 Andromeda Galaxy, the Milky Way Galaxy.;
Polaris.
**********************************************
Wednesday, December 5th. Written by Ray Bogucki.
Capella, one of the brightest stars after Sirius, and whose name
means "the Goat star", is now low in the east at nightfall in the
constellation Auriga (or-EYE-gah), the Charioteer. Capella is yellow,
much like our Sun, and forms the northeast corner of the well-known
pentagonal asterism of stars that helps us to locate Auriga. The
constellation, Auriga, is well-known to amateur astronomers as the
home of several bright open star clusters, three of which are Messier
objects. Auriga also contains a number of eclipsing binary stars.
These are variable star systems in which two stars orbit each other
in a plane that is edge on to our line of sight. Thus, as each star
passes in front of and eclipses the other, the combined light of the
system decreases during the eclipse in a regular, predictable manner.
The nearby eclipsing binary, Algol, in Perseus, is a famous example,
well known to the ancients.
A few degrees southwest of Capella, the Goat star, lies a small,
obvious triangle of stars known as "the Kids". Epsilon, the star in
the triangle nearest to Capella is a mysterious eclipsing binary very
different from Algol. First, whereas Algol is 100 light-years away,
Epsilon lies at a staggering distance, estimated at from 4000 to 8000
light-years. To be visible from Earth as a third magnitude star from
that distance, Epsilon must be one of the most luminous stars ever
discovered. Second, while Algol's orbital period is 2.9 days and the
drop in magnitude lasts a few hours, Epsilon's period is 27 years and
the drop in magnitude caused by the eclipse of the bright primary by
the secondary object lasts for 2 years. In addition, the eclipsing
object is invisible. If it is a star, it must be so cool and diffuse
that it emits no visible light. Also, in order to require 2 years to
pass in front of the primary star, the secondary object must be a
billion or more miles in diameter, which would make it the largest
star known. Another explanation for Epsilon's unusual behavior
suggests that the eclipsing object is an ordinary star hidden inside
a huge cloud of obscuring dust and gas, perhaps in the planet-forming
stage. Still another group suggests that the secondary object is a
black hole. To date, none of the explanations are fully satisfactory
and the deep mystery of this innocent-looking star remains.
**********************************************
Thursday, December 6th. Written by Peter Jennes.
Sunset for tonight, Thursday, December 6th will be at 4:21. This
Sunday and Monday, the Sun sets at 4:20 in the local area and it
should comfort some people that sunset on those two days are the
earliest sunsets of the year. After Monday, the Sun will slowly start
to set later each night. For other areas of the country, the earliest
sunset occurs on different dates. However, for all northern
locations, the actual length of daylight continues to get shorter for
fifteen more days.
The mechanism governing the date of earliest sunset is the
latitude of the observer. The further north an observer is, the later
will be the date of the earliest sunset. For instance, an observer in
Fairbanks, Alaska at 65 degrees north latitude doesn't see the
earliest sunset until around 2:30 PM on December 18th. However, an
observer in Miami, Florida, located at 25 degrees north latitude,
sees the earliest sunset around December 2nd at 5 PM.
Although the date of earliest sunset occurs on different dates for
different locations, they all have one thing in common. That
commonalty is the fact that all of them occur before the Winter
Solstice, the shortest day of the year. Logically, it would seem that
the earliest sunset of the year should occur on the shortest day of
the year but this is not the case. The reason these two dates are
separated is related to how the Earth orbits the Sun. First, because
the Earth's axis is tilted with respect to the plane of our orbit,
the date of the earliest sunset varies from location to location.
Then there are the laws of orbital motion first described by Kepler.
These laws state that because the Earth's orbit around the sun is an
ellipse, our orbital speed will vary as the Earth proceeds in its
orbit. When these variations in orbital speed are combined the
Earth's tilted axis, the net result is a lag between the earliest
sunset and the shortest day of the year.
Despite the declining nighttime hours, remember to mark your
calendar for next Thursday, Friday, and Saturday. Those nights mark
the peak of the Geminid meteor shower. With up to 95 meteors per hour
visible from a dark site, the Geminid shower is one of the best shows
of the year.
**********************************************
Friday, December 7th to Sunday, December 9th. Written by
Susan French
This weekend there will be free public observing sessions hosted
by the Albany Area Amateur Astronomers. A variety of telescopes will
be set up for viewing the wonders of the December sky, including the
Andromeda Galaxy, the Seven Sisters, the Great Nebula in Orion, and
the planets Saturn and Jupiter.
On Friday, observing will be held at the George Landis Arboretum
in Esperance and on Saturday at Sanders Preserve in West Glenville.
Both events start at 8 PM, and guests of all ages are welcome. The
telescopes are set up outside, so dress warmly. Observing is
cancelled if the sky is mostly cloudy, and may be cancelled if heavy
snowfall blocks the observing area. For further information call Sue
or Alan French at 374-8460.
This weekend also marks the beginning of the Geminid meteor
shower. The number of meteors will increase over the week reaching a
peak of about 100 per hour on Thursday night. Geminids can be seen
any time after about 8 PM with the best views probably around 1:30
AM. After Thursday, the rate will drop with few Geminids being
visible after the 17th.
Early evening meteors will favor the eastern half of the sky, but
late at night they are likely to be seen almost anywhere. Near
maximum, there are many bright fireballs with vivid colors. Geminids
travel across the sky more slowly than the Leonid meteors we saw last
month.
Most meteor showers are caused by debris left behind by comets.
Geminid meteor particles are denser than those from cometary meteor
showers. The parent object of the Geminids was unknown until
recently. However, the asteroid 3200 Phaethon, discovered by IRAS
(the Infrared Astronomical Satellite) in 1983, is now known to be the
source of the Geminid meteors. It is the only non-cometary object
associated with the evolution of a major annual meteor stream.
**********************************************
Monday, December 10th. Written by Joseph
Slomka.
The Sun sets tonight at 4:21, with night falling at 6:03 PM. Dawn
breaks at 5:34 tomorrow morning, and ends with sunrise at 7:16.
As the Sun sets, Mars is the brightest object in the southern sky.
Mars remains relatively bright, but is so small that amateur
telescopes no longer yield useful images.
By twilight's end, Saturn rises in the constellation Taurus. The
creamy white planet lies three and a half degrees above the red star
Aldebaran.
Jupiter rises about two hours after Saturn, in the middle of
Gemini. Jupiter is an interesting object for two reasons. First of
all, Jupiter's atmosphere appears as a seething cauldron of various
colors. This is evidence of titanic storms, many of which have lasted
for decades; the Great Red Spot has been observed continually for
about three hundred years. In fact it is possible to hear the storms.
If you have access to a shortwave radio and directional antenna, you
can hear the static these storms generate. A complex satellite system
is Jupiter's other attraction. There are sixteen moons, of which four
are visible to small telescopes and binoculars. If you observe
Jupiter about 1 AM, you will see Ganymede and Io aligned together
Jupiter's moons could not be more different. For example, Io is a
forbidding place where volcanoes spew sulphur and the surface is
stained various colors. While Europa is a frozen wasteland; ice, many
feet thick, covers most of the planet.
By 7:00 PM, the constellation Gemini, The Twins, rises in the
east. Simply follow the distinctive "V" of Taurus and locate two
stars that seem equally bright. The constellation indeed resembles
stick drawings of men. Castor is the northern and slightly dimmer
star; Pollux is his brother. Castor was an expert horseman, while
Pollux was a boxer. Their names reflect these occupations. They were
sons of the Greek god Zeus, and Helen of Troy's brothers. Greek
sailors revered them as protectors. The phrase "by jimminy" is a
variation of "by Gemini," an ancient oath.
**********************************************
Tuesday, December 11th. Written by Jonathan
Cassidy.
Tonight the slim crescent moon is just one day from new and does
not add any light to the night sky. The new moon is in conjunction
with the sun and does not appear at night.
So tonight is a dark night. A good night to see things not
normally visible when the moon is up. So what is up there to see? How
about star clusters? Directly overhead tonight is the "W" of the
constellation Cassiopeia. To the east is Alpha Persei. Half way
between is a dim smudge of stars. This is the Perseus Double Cluster.
It can be found naked eye on dark sky nights like tonight.
Further to the north east after 8 PM you will see the bright star
Capella in the constellation Auriga. This constellation looks like a
lop-sided pentagon.
Notice that the Milky Way Galaxy goes through Cassiopeia, Perseus
and Auriga. Star clusters found in these constellations reside in our
home galaxy.
With binoculars, on a dark night, you will find several star
clusters in the area of Auriga. Just cruise around the area with any
power or size binoculars and you will be rewarded.
**********************************************
Wednesday, December 12th. Written by Ray
Bogucki.
This Friday, Dec. 14, will see a special New Moon when the center
of the Moon passes directly in front of the center of the Sun,
producing a solar eclipse. Because the Earth is near perihelion, its
closest approach to the Sun, the solar disk is larger than usual, and
because the Moon is receding from the Earth at this point, its disk
is diminishing. The result is that, at the moment of eclipse, the
Moon's disk will be almost 2 arc-minutes smaller in diameter than the
Sun's, and thus unable to cover it completely. This type of eclipse
is called annular, and at mid-eclipse a razor-thin ring of sunlight
will remain around the black disk of the Moon. While this apparition
may not be as dramatic as a total solar eclipse, the sight of the Sun
with 97% of its center punched out by what appears as a large, black
hole is startling in its own right. The Moon's shadow will trace a
path across the open Pacific Ocean with the only landfall occurring
just before the end of the eclipse in Costa Rica and Nicaragua in
Central America. At Albany, viewers will see the first intrusion of
the Moon's disk into the limb of the Sun at 4:13 Friday afternoon,
unfortunately just a few minutes before sunset.
Tomorrow night the Earth will pass through the orbiting debris
that generates the Geminid meteor shower. It is unusual that this
stream of debris has no known comet as a parent, but rather, it
follows, almost exactly, the orbit of the asteroid, Phaeton. This 4
-mile wide, silicate rock orbits the Sun with a period of 1.43 years,
its highly elliptical, cigar-shaped orbit bringing it within 13
million miles of the Sun and then far out beyond the orbit of Mars.
Phaeton has no known history of cometary activity and it is not clear
by what mechanism it could have generated a stream of orbital
debris.
The Geminids are relatively slow-moving, about half the speed of
the recent Leonids, and often feature bright fireballs. Because
tomorrow night's forecast is for clouds and rain, it would be
worthwhile to spend some time tonight watching for early arrivals of
this unusual meteor shower.
**********************************************
Thursday, December 13th. Written by Peter
Jennes.
Tonight and tomorrow night marks the peak of the Geminid meteor
shower. Since the Moon is less than one day from new, it will not
interfere with meteor observations. Unlike the recent Leonids, the
Geminids are more predictable but also more mysterious. The Geminids
were unknown until 1862 when observers began to notice a minor meteor
shower with a radiant in the constellation Gemini. Since then, the
Geminids have intensified to the point of becoming one of the best
annual meteor showers, comparing with the summer's Perseid meteor
shower.
The biggest difference between the Geminid and Perseid meteors
comes from parent body of the two showers. The Perseids are born from
Comet Swift-Tuttle while the Geminids are remnants of a mysterious
object called 3200 Phaethon. It took 120 years of searching and a
modern astronomical satellite to find this object. In 1982, NASA's
Infrared Astronomical Satellite discovered a curious object moving in
the same orbit as the Geminid meteoroid stream. The orbital match was
so good that it had to be the source of the debris, but to the
surprise of many, it wasn't a comet. Instead, Phaethon looks like an
asteroid and has an asteroid's spectrum. However, Phaethon has the
orbit of a comet.
Several theories have been proposed as to how an asteroid could
create a meteor shower. At this time, the most widely accepted theory
is that 3200 Phaethon has accumulated a crust making it appear like
an asteroid. However, underneath this crust lies a comets
burned out nucleus. Astronomers propose that when Phaethon passes the
sun, pieces of the nucleus break off to form the Geminid meteoroids.
Studies of Geminid fireballs support this theory. By observing these
fireballs, scientists have estimated that Geminid meteoroids are less
dense than a typical asteroid but denser than a comet.
The Geminid Meteor Shower radiant places meteors in the sky all
night. Early in the evening, the Geminid shower tends to produce
earth-grazing meteors that make long trails arcing up from the
eastern horizon. Later in the evening, the trails get shorter but
from a dark site, the hourly count jumps up to an average rate of 100
meteors per hour. From urban areas however, this number drops off to
about 4 meteors per hour.
**********************************************
Friday, December 14th to Sunday, December 16th. Written by
Greg Nowell
As you look into the eastern sky at about 9 p.m. tonight you will
see two constellations, Taurus and Auriga. Taurus is a compact
V-shaped constellation that points south. Just above it is a small
cluster of stars known as the seven sisters, or the Pleiades. Taurus
represents a mythological bull. A fairly bright reddish star, called
Aldebaran, was thought to be the eye of the bull. Taurus' horns
actually extend further north than the highly defined V-shape that
follows the Pleiades through the winter sky.
The tip of one of Taurus' horns is of particular interest. This
star is called Al-Nath. It is on the exact boundary between the
constellations of Taurus and Auriga, and is in fact counted as the
second brightest star in Auriga as well as the second brightest star
in Taurus. Al-Nath lies below Capella, which with the exception of
the planet Jupiter is one of the brightest objects to be seen in the
sky at this time. Al-Nath, sometimes also transcribed from Arabic as
El-Nath (with an "E"), is itself the 25th brightest star visible to
the unaided eye. Since the human eye can pick out thousands of stars
on a clear night, ranking 25th in brightness is no small achievement.
But Al-Nath has another claim to fame. It is the closest of the naked
eye stars to a part of the sky astronomers call the
"anti-center."
Standing under the starry sky, it is hard to imagine that the
stars we see have any relation to the dazzling photographs of
galaxies and deep space that we see occasionally in magazines. But
this little planet of ours is in a galaxy, and as it spins around we
see different parts of that galaxy. When you look at Al-Nath, you are
looking almost exactly in the direction of the edge of the galaxy
that is closest to Earth. If you could draw a line from Al-Nath
through your eyes, out the back of your head, through the Earth
itself, and out deep into space again, that line would take you
straight to the heart of our own galaxy, the galactic center. The
anti-center is the extreme edge of our galaxy, and lies at the very
end of a straight line that starts in the galactic center, passes
through Earth, and ends at the galactic rim.
The famous eighteenth French astronomer Charles Messier did not
know that Al-Nath was near the galactic center, because in his day
galaxies were not understood as vast collections of stars. That
knowledge came over a century after his death. But it is a curious
coincidence that Messier began his famous list of deep sky objects
with the gaseous remnants of an exploded star that we call the Crab
Nebula. The Crab Nebula cannot be seen with the naked eye, but it is
easily viewed in small telescopes. The Crab Nebula is designated M1,
number one on Messier's list. M1 lies even closer to the galactic
anti-center than Al-Nath. It seems remarkable that the most famous of
earthly lists of sky objects should begin with the very one that lies
nearly on top of the galactic anti-center.
**********************************************
Monday, December 17th. Written by Joseph
Slomka.
The Sun sets tonight at 4:22, with night falling at 6:05. Dawn
breaks at 5:51 AM, with sunrise taking place at 7:22.
As you hear this Skywatch Line, it is most likely snowing hard.
For centuries, people thought that weather only existed on Earth. Now
we know that there is all kinds of weather in most of the Solar
System.
The Sun is a raging ball of hydrogen gas, which is fusing into
helium and other elements. However, the Sun's output is not steady.
The Sun goes through an eleven year period in which the number of
sunspots vary. The exact mechanism is still not thoroughly
understood, but as the number of spots increase, so do the number and
degree of solar storms. These storms spew vast quantities of
particles in all directions. If Earth gets in the way of such a
storm, its atmosphere reacts to these particles, creating beautiful
auroras, or Northern Lights. If the storm is really energetic, radio
communications may be disrupted, satellites damaged, and even power
grids disrupted. One giant eruption blacked out Canada's Quebec
providence in 1989.
Mercury and the Moon have no weather, because they have no
atmosphere. Pluto's weather is unknown, since no spacecraft has
visited the last planet of the Solar System. Most likely, Pluto's
atmosphere is so cold that no significant weather would be found.
Venus is perpetually cloudy, an example of a greenhouse effect
gone wild; in addition, its clouds rain sulfuric acid. Mars is a
planet that is well known for having weather. Clouds and dust storms
are visible in backyard telescopes, as are polar ice caps. Jupiter' s
storms are easily seen in backyard instruments. One storm, the Great
Red Spot, had been documented for three hundred years, and lesser
storms are frequently seen on the planets cloud belts. Saturn also
displays rare variations in its cloud cover, revealing possible
weather - features also available to larger backyard telescopes.
Spacecraft have found Uranus and Neptune with similar variations in
their cloud systems, again indications of atmospheric variations.
**********************************************
Tuesday, December 18th. Written by Jonathan
Cassidy.
Earth's Sun is not the only star to show an eclipse. The star
Algol, beta Persei, in the constellation Perseus is an eclipsing
binary set of stars. That is two stars orbiting the same center of
gravity locked together in space.
The plane of orbit of these two stars is in line with our planet.
Thus we can see the two stars eclipse each other. We can not see that
there are two stars there but we can see that the combined light from
the stars varies over a short period. The variation in light is
enough that naked eye observers can see it happen in just a few
days.
Algol has a maximum magnitude of 2.1 and a minimum of 3.3, but
nearly as dramatic as the long period variables. The cycle, from
brightest to dimmest, is only 2.9 days. This makes the cycle easier
to see and plot than other types of variable stars.
This means that the two stars are going around each other in less
than three days. That is quite fast. In comparison we take 365 &
1/4 days for Earth to go around our Sun. Algol's light curve shows
this quick speed the dip in magnitude is short relative to the length
of the cycle. On some nights it is possible to watch the entire dip
and return brightening in one session.
**********************************************
Wednesday, December 19th. Written by Ray
Bogucki.
The Sun is rapidly approaching two points in its orbit that mark
extremes in its orbital behavior. On Friday, Dec. 21, the Sun's
northern axis will reach its maximum tilt away from the Sun,
producing the winter solstice. This is the day with the minimum
number of sunlit hours, only 9 hours and 18 minutes at this latitude.
It is also the day when the Sun rises and sets at its most southerly
points, and stands at its lowest elevation above the horizon when it
crosses the southern meridian at noon. One might reasonably assume
that this day would mark the latest sunrise and earliest sunset, but,
in fact, the earliest sunset occurred 10 days ago. Sunrise, however,
will continue to occur later each day until about January 2, when the
daylight hours begin lengthening at both ends of the day. The
asymmetry in times of sunrise and sunset is caused by the tilt of the
Earth's axis and the variations in orbital velocity at different
times of the year. It might seem logical to describe the day when the
Sun is at its lowest as the middle of winter, but the seasonal delay
in weather gives us the coldest two months in January and February.
Thus, the solstice is usually designated as the beginning of
winter.
January 2 also marks the point in the Earth's elliptical orbit
when it reaches perihelion, its closest approach to the Sun for the
year. On this day we will be 3 million miles closer to the Sun than
when we are at our farthest point on the sixth of July. Perihelion
also marks that point in our orbit when the Earth achieves its
highest orbital velocity, almost as though the Earth was trying to
help out by speeding the residents of the northern hemisphere a
little faster through their coldest months, and the people in the
southern hemisphere a little faster through their hottest months.
**********************************************
Thursday, December 20th. Written by Peter
Jennes.
**********************************************
Friday, December 21st to Sunday, December 23rd. Written by
Susan French
This Friday is the December Solstice and marks the beginning of
winter in the Northern Hemisphere.
The Earth's North Pole points toward a spot in the
constellation Ursa Minor, the Little Bear. This spot is called the
North Celestial Pole, and it lies very close to the star we call
Polaris or the North Star. In the same way, the South Celestial Pole
indicates the spot toward which our South Pole points, but it is not
marked by any bright star. On the Earth we draw an imaginary line
halfway between the North and South Poles called the Equator, and in
the sky we draw a line halfway between the North and South Celestial
Poles called the Celestial Equator.
The Sun blots different constellations in the sky as the Earth we
live on travels around it. The Sun's apparent path through
these constellations is known as the Ecliptic, and it runs through
the familiar constellations of the Zodiac. Some of these
constellations lie above the sky's equator, and some lie below
it. Right now, the Sun is in the constellation Sagittarius, the
Archer. Sagittarius is farther below the Celestial Equator than any
of the other zodiacal (zoh DYE ah cahl) constellations, so we see the
Sun taking its lowest path across the sky for the year.
The moon is at First Quarter on Saturday at 3:56 PM EST. The term
First Quarter Moon may seem confusing since it is obvious that more
than one quarter of the moon's face is lit. Instead, First
Quarter refers to the fact that the moon is one-fourth of the way
around the Earth as seen from the sun. When the moon is at First
Quarter phase, it appears about half lit.
The Ursid meteor shower peaks this weekend. These meteors favor
the northern half of the sky, but the best place to focus your
attention may be straight up where the sky is clearest. The Ursid
shower produces many faint meteors and some fireballs. The rate
usually peaks at about 10 or meteors per hour, but there are
occasional outbursts of up to 50 per hour. Best viewing is after
moonset at about midnight. The debris that causes Ursid meteors comes
from Comet Tuttle.
**********************************************
Monday, December 24th. Written by Joseph
Slomka.
**********************************************
Tuesday, December 25th. Written by Jonathan
Cassidy.
The Sun is up latter now. Even though the Sun is still rising
later, and will continue to do so till some time in January, it is
now setting slightly later each day, thus the days are
lengthening.
In relation to its north south travel, due to Earth's tilt on it's
axis, the Sun stands nearly still twice each year. This is the time
that the tilt of the Earth related to the Sun is at the maximum or
minimum, that is winter of summer solstice.
During the second week in December, this year the Sun stood at
nearly the same place each day at noon. Now it is moving higher in
the sky each day. You can check this by noting the position of a tall
structure's shadow at the same time each day, usually noon.
If you mark the position at the same time of the day and same day
of the month you will construct a figure on the ground. If done
correctly the figure will look like the numeral "8". The figure is
called an Analema. This week is a good time to start one and is a
good activity during the dark cold months of winter.
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Wednesday, December 26th. Written by Ray
Bogucki.
Continuing in a series of occultations, the Moon will pass in
front of the planet Saturn early Friday morning. A few minutes after
4 a.m. the dark northern limb of the Moon will begin to cover the
planet. Saturn will reappear from behind the sunlit part of the
Moon's limb about a half hour later. The next occultation in this
series will occur on February 20 at the more convenient time of 7
p.m.
Even when it is not being occulted, Saturn presents an intriguing
target for observation. Earth just passed between the Sun and Saturn
earlier this month, so it is still near its closest approach for this
cycle. Although Saturn is a little smaller than Jupiter and almost
twice as far away, it nevertheless presents a sizable 20 arc-second
disk. Its extensive ring system extends its apparent diameter to
about 46 arc-seconds, the size of Jupiter. The rings are tilted about
26 degrees to our line of sight, just about the maximum possible. The
extra sunlight reflected by the rings greatly add to the brightness
of Saturn which currently shines brighter than a zero magnitude star.
The spectacular ring system is 170,000 miles in diameter but less
than one mile in thickness. It is made of chunks of rock and ice
ranging in size from that of a sand grain to large, house-sized
boulders. When the rings are edge-on to our line of sight, they
disappear in small, or medium sized telescopes and appear as a
razor-thin straight line in large telescopes. In its current
configuration, even a small telescope will show the dark, Cassini
division between the outer A and B rings and Saturn's largest moon,
Titan. Saturn is located a few degrees north of Aldebaran, the red
eye of Taurus, the Bull in the eastern sky at nightfall. It rises
before sunset and is well-placed for observation throughout the
night.
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Thursday, December 27th. Written by Peter
Jennes.
At 4 AM tomorrow morning, Saturn disappears behind the Moon's dark
limb. This event occurs 10 degrees above the horizon so if you are
hoping to see this occultation, you will need a clear western view.
As the Moon covers Saturn, it will be two days away from full.
December's Full Long Nights Moon occurs early Sunday and at that
time, it is more or less opposite the Sun. Usually, the Moon is
slightly out of line from the Sun, while at other times, the Moon is
directly opposite the Sun and a total lunar eclipse occurs. This
month the Moon is almost on a direct line with the Sun and passes
through the outer fringes of the Earth's shadow. This type of eclipse
is called a penumbral eclipse and unless you have specialized
equipment, the effects of these eclipses are barely visible.
One simple observation that is easy to overlook during the full
Moon is that the full Moon, because it is roughly opposite the Sun,
actually rides higher in the sky during the winter when the Sun is
low to the horizon. In contrast, during the summer the Sun rides high
in the sky while the full Moon hugs the horizon. In fact, if you
measure the angle between the horizon and the almost full Moon around
midnight on Saturday, you would find that it is about 70 degrees
above the horizon. In contrast, at noon on Sunday, the Sun will be a
mere 24 degrees above the horizon. Six months from now, during June's
Full Strawberry Moon, the angle between the Moon and the horizon
decreases to 20 degrees above the horizon, while the Sun will be high
overhead at 70 degrees above the horizon.
To further illustrate how the Sun and Moon change places in the
sky, on Sunday the moon will be drifting through the stars of Gemini
and the Sun will be in Capricorn. During June, you will find that the
Moon and Sun have changed places. Instead of the Sun, you will find
the full Moon sitting in Capricorn while the Sun will be in Gemini.
Simple observations like this seasonal place changing between the Sun
and Moon led to some of humankind's greatest astronomical
discoveries.
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Friday, December 38th to Sunday, December 30th. Written by
Susan French
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Monday, December 31st. Written by Joseph
Slomka.
The Sun sets tonight at 4:31, with night falling at 6:13 PM. Dawn
breaks at 5:56 AM, with sunrise taking place at 7:26.
As the Sun sets, two bright planets occupy our attention, while
two others require skill and luck. Saturn blazes moderately high in
the eastern sky in the constellation Taurus. Mars is still the
brightest object in western skies. Uranus and Neptune lie to Mar's
right, but require skill and luck to find them in the darkening
sky.
By nightfall, Jupiter occupies the constellation Gemini. One of
Jupiter's most famous features - the Great Red Spot is now in the
news. It has apparently shrunk over the past century. No one knows
why, but observers hope to clear up the mystery.
Since the nearly full Moon dominates the sky, and blots out most
galaxies and star clusters, let us concentrate on Earth's satellite.
Our Moon is very unusual. It is about one sixth the Earth's diameter,
one sixth the gravity, and one eightieth the mass. These facts amount
to a double planet system; only Pluto's satellite, Charon, is larger
in relation to the main planet. Its low gravity means that it has no
atmosphere. Despite the fact that the Moon was visited several times
by astronauts and is only two light seconds away, we know remarkably
little about its history and composition. The only certainty is that
the Moon underwent a severe history of bombardment, leaving behind
craters that binoculars can see. There are three competing theories.
One is that the Moon formed the same time as the Earth, with the two
bodies orbiting about a common axis. A second hypothesis is that the
Moon is a body that accidentally wandered into Earth's gravity field
and was captured. The most recent speculation is that Earth, very
early in its history, was hit by a very large body, and the Moon
formed from the debris of that collision. If this third option is
correct, it explains many oddities about the Earth-Moon
relationship.
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