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Skywatch February 2008 Skywatch line for Wed. and Thurs., February 27 & 28, 2008
by Ray Bogucki The weather cooperated with observers for the total lunar eclipse
last Wednesday. The sky was clear and transparent. Just before the
Full Moon began to enter the Earth's shadow, its brightness had
lightened the sky so that only the brightest stars were visible, and
the fresh snow cover on the ground, reflecting the moonlight, made
it seem almost as bright as day. As the Moon began to enter the
Earth's shadow, the sky slowly darkened until, at full eclipse,
faint stars and even the Milky Way became visible, while neighbors
standing around the telescope became spectral shadows. Then, just
as the Moon's limb began to emerge from Earth's shadow and brighten
as it reentered the sunlight, clouds moved in to obscure the view.
Nevertheless, observing the first half of the eclipse was a splendid
success.
Now that the Moon is nearing last quarter, and not rising until
midnight, the early evening is very dark for observing the bright
constellations in the south. The familiar form of Orion, described
in our February 13 Skywatch line, is especially inviting. The stars
in Orion appear bright, not because they are close, but because they
are so large and luminous. For example, the three belt stars, all
about magnitude 2, range in distance from 800 to l,000 light years
away. Rigel, the blue-white star in Orion's foot, lies 820 light
years away and shines at a dazzling zero magnitude. Betelgeuse, the
brilliant ruby-tinged star in Orion's shoulder, is 520 light years
away and is so large that if placed at the center of our Solar
System, it would occupy the space almost out to the orbit of
Jupiter. The orbits of Mars, Earth, Venus and Mercury would all
be inside the star.
Probably the most stunning sight lies in Orion's sword, the three
fainter stars that hang down in a line below the three brighter belt
stars. Careful observation by eye suggests that the middle star in
the sword is rather fuzzy. The view opens up in binoculars or a
small telescope to reveal that the three stars are actually
groupings of stars, with the central star appearing as a cloud that
appears to be swirling around in some interstellar wind. This
object, known as the Great Orion Nebula and designated as M42, is
indeed a gargantuan cloud of gas and dust which is in the process of
gravitationally collapsing to form brand new stars -- a stellar
nursery. At the core of the cloud is a tight cluster of newly
formed stars known as the "trapezium". These stars are very hot and
emit powerful ultraviolet radiation which causes the surrounding
gases to glow with a faint green light. The radiation has
also blown a hole in the cloud so that large telescopes, such as the
Hubble, can peer deep into the cloud and see new stars in the
process of being born -- a remarkable sight!
This is the Skywatch Line for Monday and Tuesday,
February 25th and 26th. Skywatch line for Wed. and Thurs., February 20 and 21, 2008:
by Ray Bogucki As the Earth sails serenely along its orbital path around the Sun,
the Sun casts a dark umbral shadow of Earth that extends for almost
a million miles into space. For the billions of people who inhabit
the Earth, passing through this shadow is no challenge at all. Once
each day, the rotation of the Earth carries our western horizon
relentlessly upward until it overtakes and finally obscures the Sun
in an event that we call sunset. As soon as the last bit of the Sun
drops below the horizon, we enter the Earth's shadow.
Interestingly, the sky does not become dark instantly because our
atmosphere of gas, moisture, dust particles, etc., extends several
hundred miles above us and continues to reflect sunlight down to us
for a short, slowly darkening period known as twilight. Within a
couple of hours, twilight ends and we enter the fully dark, umbral shadow
of the Earth for a period which we call the night.
For our companion, the Moon, passing through Earth's shadow is a
much more difficult challenge. Because the Moon's orbital plane
around Earth is tilted 5 degrees to Earth's orbital plane around the
Sun, the three objects; Sun, Earth and Moon, don't usually line up
exactly, so the Full Moon usually passes well above or below the
Earth's shadow.
We are currently in one of the two eclipse periods which occur
each year when the alignment is close enough for the Full Moon to
pass straight through the Earth's shadow. It will do just that
tonight, Wednesday. After rising in the east at sunset, the Moon
will first enter the Earth's faint penumbral shadow at 7:36 p.m.
This is not usually noticeable. An hour later, at 8:43, the Moon
will encounter the edge of Earth's much darker umbral shadow. As
the Moon slowly proceeds into the shadow, notice that the edge of
the Earth's shadow is round. 2,500 years ago, Greek astronomers
noted this, and declared that the Earth must be a sphere because it
casts a round shadow from any direction. At 10:00 p.m., the Moon
will be fully engulfed by the Earth's shadow, but it will not be
completely dark. A pale, coppery-red light seems to illuminate it.
In 1618, Johannes Kepler, in his treatise "Epitome", explained that
an observer on the Moon would see the large disk of the Earth
covering the Sun, but the Earth's atmosphere would act as a lens to
refract the red rays of the Sun onto the Moon's surface. The Earth
would appear as a black disk with a bright reddish ring of light
around it.
In binoculars, the Moon, at full eclipse, loses its usual "bright
disk" appearance and is revealed, in a startling 3-dimensional
aspect, as an obvious sphere. By 10:50 the Moon will begin to
emerge into the brighter penumbral shadow and resume its familiar
bright Full Moon aspect. Now we only need to figure out how to keep
the clouds away.
This is the Skywatch Line for
Monday and Tuesday, February 18th and 19th. The Sun sets at 5:30 PM, with night falling at 7:05. Dawn
breaks at 5:12 AM and ends with sunrise at 6:47. This is Dudley Observatory's Skywatch Line for Friday,
February 15, through Sunday, February 17, written by Alan French. Skywatch line for Wed. and Thurs., February 13 and 14, 2008:
by Ray Bogucki We have reached midwinter and the glittering spectacle of the
bright winter constellations are fully displayed high in the
southern sky at nightfall. To appreciate this marvelous display,
dress in many layers of warm clothes. Don a warm hat, insulated
gloves and boots, and sit in a comfortable lawn chair, facing
south. For the first few minutes, allow your sight and mind to be
overwhelmed by simply sweeping your unaided eyes back and forth
across the field of bright objects. While the summer skies are
distinguished by having three bright stars to form the "summer
triangle", the winter skies boast seven stars to enclose the
brightest collection of stars in such a small area anywhere in the
skies visible from the Earth. These seven stars describe what is
often called the "winter oval" or the "winter hexagon". Why refer
to a loop of seven stars as a hexagon? Because two of the stars,
Castor and Pollux, representing the heads of the Gemini twins, are
close enough together to be considered as marking one corner of the
hexagon. To pick out the hexagon, first locate Orion, the Hunter,
one of the most familiar of all constellations. It is marked by a
straight line of three evenly spaced bright stars that form the belt
of the hunter. Two bright stars above the belt mark Orion's
shoulders, and two more bright stars below the line mark the
hunter's feet. Three fainter stars in a vertical line mark the
sword hanging from Orion's belt.
The hexagon begins just below, and a little to the left, or east,
of Orion at Sirius, the brightest star anywhere in the sky, in the
constellation Canis Major (the Big Dog). Sirius is famous for its
frenetic twinkling and seems to split off in tiny shards of various
colors in the turbulent air close to the horizon.
From Sirius, move northeastward until you encounter another very bright white star named Procyon, in the constellation Canis Minor (the Little Dog). Moving northward toward Polaris the North Star, you'll run into the close twins, Castor and Pollux, mentioned above. From Pollux, the brighter of the two, move directly overhead to the brilliant yellow star Capella, part of the pentagon asterism that identifies the constellation, Auriga, the Charioteer. From Capella, proceed downward, or south, to the bright reddish star, Aldebaran, the eye of Taurus, the Bull. Continue downward and a bit left to the brilliant blue-white star Rigel in the foot of Orion and thence back to Sirius. Betelgeuse, the supergiant reddish star in Orion's shoulder, is near the center of the just-traced hexagon. This winter, the hexagon includes a bright guest object, the Red Planet Mars, located on a line halfway between Betelgeuse and Capella. Mars forms an almost perfect equilateral triangle with Betelgeuse and Aldebaran to produce the closest gathering of three bright reddish objects anywhere in the night sky. In a future Skywatch line, we will discuss some of the striking binocular sights to be found within the winter hexagon. This is the Skywatch Line for Monday and Tuesday,
February Eleventh and Twelfth. Skywatch line for Wednesday, Feb. 6 through Sunday, Feb. 10,
2008:
by Ray Bogucki The Sun is just 400 times larger in diameter than the Moon and
just about 400 times farther away. This interesting coincidence
assures that the Sun and the Moon will appear about the same size in
our sky. We might also note that the plane defined by the Earth's
orbit around the Sun, and the plane defined by the Moon's orbit
around the Earth, do not coincide. They are tilted about five
degrees to each other.
The New Moon is defined as that point in the Moon's orbital travel
when it passes between the Earth and the Sun. Likewise, the Full
Moon occurs when the Earth passes between the Sun and the Moon, and
the Sun and Moon are opposite each other in the sky. An eclipse of
the Sun can occur only at New Moon as the Moon passes between the
Earth and the Sun, blocking out the Sun, and an eclipse of the Moon
can occur only at Full Moon as the Earth passes between the Sun and
the Moon, and casts its shadow on the Moon. Because of the tilt of
the two orbital planes relative to each other, the Moon will spend
half of its time above the Earth's orbital plane and the other half
below. Thus, most of the time, the alignment of the three bodies
will be imperfect, so the New Moon will appear to pass a little
above or below the Sun, while the Full Moon will pass a little above
or below the Earth's shadow and there will be no eclipse or other
visual effect in either case.
There are, however, two points on opposite sides of the Earth's
orbit which we can call nodes. When the Earth is at or close to one
of the nodes, we have an eclipse season. That is the only time that
the alignment of the three bodies, Sun, Moon and Earth, is precise
enough for the New Moon to pass directly across the face of the
Sun to produce a total eclipse of the Sun. Likewise, the Full
Moon can pass through the Earth's dark, umbral shadow to produce a
lunar eclipse.
In 2008, the two eclipse seasons are in the months of February and
August, and true to form, the first solar eclipse of the year occurs
tonight (Wednesday) with maximum eclipse at about 10:55 p.m. The
time tells us that the eclipse occurs on the other side of the
Earth. It will be maximum over the far southern Pacific Ocean,
close to the Antarctic continent. We will not see it, but observers
in New Zealand and southeastern Australia will see a partial
eclipse.
Still, observers in this area should take heart. In two weeks, on
Feb. 20 and still within the eclipse season, we will see the Full
Moon rise in the east at sunset, close to the bright star Regulus,
and begin to enter the Earth's faint penumbral shadow. By 9 p.m.,
high up in the southeast, it will be entering the Earth's darker
umbra and it will be fully eclipsed by 10 p.m. Throughout the
eclipse, the bright, ringed planet Saturn will be close by, adding
to the visual spectacle.
This is the Skywatch Line for Monday and Tuesday,
February Fourth and Fifth. The Sun sets at 5:12 PM, with night falling at 6:45. Dawn
breaks at 5:29 AM; the Sun rises at 7:06.
Dudley Observatory's Skywatch Line for Friday, February 1,
through Sunday, February 3, written by Alan French.
Just over one-half degree separated Venus and Jupiter on Friday morning. Although they are now moving apart as Venus moves eastward toward the Sun, the will remain a pretty pair for a while. On Sunday and Monday mornings they will be joined by the thin crescent old Moon, and form a beautiful trio in the predawn skies. Look for Jupiter and Venus any morning this weekend toward the southeast one hour before sunrise. The Sun now rises at 7:08 AM, so look just after 6:00. On Saturday morning Venus and Jupiter will be just over one degree apart, with Venus to the left of Jupiter. A pretty crescent Moon will be well to their right and higher. By Sunday morning Venus and Jupiter will be two degrees apart, and Venus will have moved lower in the sky and will be to the left of and below Jupiter. The Moon's eastward motion among the stars will have brought it closer to our planetary duo. Monday morning at 6:00 AM will find a close trio of Venus, Jupiter, and a very slender old Moon. Venus and Jupiter will be three degrees apart, and the Moon will be below the pair. The Moon will be just above the horizon, so you'll need a good view to the southeast, unhindered by trees or buildings. If wait too long after 6:00, the Moon will have set. The International Space Station, or ISS for short, will pass right over the Capital District early Sunday evening. With its large area, the ISS is the brightest satellite in the night sky, outshining all the stars. We will be giving some of the times for Sunday night's appearance in hours, minutes, and seconds. On Sunday evening, look for the ISS, appearing as a bright star, moving up from the southwestern horizon at 5:16 PM. It will be highest at 5:18:39. After reaching its highest point it will move through the constellation Perseus, and then pass close to Capella, the brightest star in Auriga. The ISS will vanish below the east-northeastern horizon at 5:21:29.
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