Venus
Venus and the Moon Will "Snuggle Up" on Feb. 27
To date it has been a superb winter for viewing the queen of the planets, Venus. February marks the pinnacle of its evening visibility as it stands like a sequined showgirl nearly halfway up in the western sky at sunset. Currently shining at its greatest brilliance for this apparition, this dazzling evening star
appears as a distinct crescent shape in small telescopes, which is growing progressively larger in size as it approaches our Earth.
And be sure to get out your calendar and put a big circle around Friday, February 27, 2009, for that evening a lovely crescent Moon will appear to snuggle up close to Venus, particularly for skywatchers across the Western Hemisphere. It will make for an eye-catching scene as the two brightest sky objects of the night dominate the early evening scene for about three hours after sundown; even those who do not normally look up will likely have their attention drawn to this dynamic duo
during their normal commute home from work or school. What will make this array especially attractive is the fact that it will look almost three-dimensional; the Moon will look almost like an eerily illuminated blue and yellow Christmas ball hovering next to the brilliant-white diamond that is Venus.
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The crescent Moon and Venus. (Image courtesy Bob King/News Tribune)
Sadly, this will be the last in the current series of evening get-togethers between the Moon and Venus, for during March Venus will slide rapidly down into the sunset glow and by month's end will disappear from our evening sky until the spring of 2010.
But again . . . Friday night, February 27 will be the night when the Americas will be greeted with one of the most beautiful Venus-crescent Moon conjunctions possible. The pairing will persist from before sunset on into the depths of darkness. The time when Moon and planet will appear closest will be around 8:30 p.m. Eastern time (7:30 p.m. Central, 6:30 p.m. Mountain, and 5:30 p.m. Pacific). Venus will appear to hover approximately 1.5-degrees above and to the right of the 10-percent illuminated Moon (the Moon itself appears one-half degree in diameter). For cities situated in the Mountain time zone, the time of closest approach will come during evening twilight, while for those in the Pacific time zone it takes place around, or just prior to sunset.
From other places around the world, the pairing will appear a bit different primarily because the Moon appears to move much more rapidly against the background stars than Venus, and also because of the effect of parallax: different viewing angles from different points on our planet.
From Europe, for instance, Venus will appear to hover majestically about 4-degrees directly above the Moon at sunset. South Americans will see the Moon with Venus to its right; the pair low in the west-northwest at dusk and appearing to set side-by-side. From Australia, the Moon will be positioned far to the lower left of Venus on the evening of Feb. 27 and a somewhat similar distance to its upper right the following evening.
Finally, if you're watching with some friends, here's a trivia question you might want to pose to them: Of the two which do they believe is the brighter: Venus now at its peak brilliance or the three-day old Moon? The almanacs say that the Moon is 8.5 times (2.3 magnitudes) brighter, but because its light is not concentrated into a point like Venus, they may have a difficult time believing this!
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A "Celestial Summit Meeting" Set For December 1st
Without a question of doubt, the most spectacular celestial sight during these final days of November is reserved for the early evening sky. One of my astronomy mentors, Dr. Ken Franklin (1923-2007), a former Chairman and Chief Astronomer here at the Hayden Planetarium often made reference to our dynamic and ever-changing night sky.
Such an eloquent description certainly fits our current evening sky, as we now have a celestial summit meeting in the making in the western evening twilight.
The highlight will be the gradual approach relative to each other of the two brightest planets—Venus and Jupiter—with the waxing crescent Moon joining them on the first evening of December. For the remainder of November, skywatchers will observe Jupiter and Venus slowly converge on each other in the southwestern sky, right after sunset. Venus and Jupiter will appear a similar distance apart on both the evenings of November 30 and December 1. The moment of closest approach will actually come during the early morning hours of December 1, unfortunately when this dynamic duo
is below the horizon for North America. They'll be separated by just over 2°, which corresponds to roughly one-half the distance that separates Pollux from Castor, the Twin Stars
of Gemini (The width of your fist, held at arm’s length roughly corresponds to 10°).
The pinnacle, however, will come on early on Monday evening, December 1.
Every once in a while, something will appear in the night sky that will attract the attention of even those who normally don't bother looking up. It's likely to be that way on that Monday evening when a slender crescent Moon, just 15% illuminated, will appear in very close proximity to Venus and Jupiter.

Venus and Jupiter is joined by the waxing crescent Moon after sunset. This diagram is drawn for North America and the Moon's size is exaggerated for clarity. Image courtesy Sky & Telescope.
People who are unaware, or have no advance notice, will almost certainly wonder, as they cast a casual glance toward the Moon on that night, what those two large, silvery stars
happen to be? Sometimes, such an occasion brings with it a sudden spike of phone calls to local planetariums, weather offices, and even police precincts. Not a few of these calls excitedly inquire about the UFOs
that are hovering closely in the vicinity of our natural satellite.
A very close conjunction of the crescent Moon and a bright star or planet can be an awe-inspiring naked-eye spectacle. Those involving Venus, Jupiter and the Moon—the three brightest objects in the night sky—always attract the greatest attention of all. Ken would have called it, A beautiful celestial tableau!

Jupiter, Venus, and the Moon photographed on April 23, 1998. Image courtesy Steve Irvine.
The English poet, critic, and philosopher, Samuel Taylor Coleridge (1772-1834) used just such a celestial sight as an ominous portent in his epic, The Rime of the Ancient Mariner. In addition, there are juxtaposed crescent Moon and star symbols that have appeared on the flags of many nations, including Turkey, Pakistan, Malaysia, Algeria, Mauritania, and Tunisia.
Earthshine
Also on Monday evening, you may be able to see the full globe of the Moon, its darkened portion glowing with a bluish-gray hue interposed between the sunlit crescent and not much darker sky. This vision is sometimes called the old Moon in the young Moon's arms.
Leonardo da Vinci (1452-1519) was the first to recognize it as what we now call Earthshine.
As seen from the Moon, the Earth would loom in the sky nearly 3.7 times larger than the Moon does for us. In addition, the land masses, the oceans, and clouds make the Earth a much better reflector of sunlight as compared to the Moon. In fact, the Earth's reflectivity varies as clouds, which appear far more brilliant than the land and seas, cover greater or lesser parts of the visible hemisphere. The result is that the Earth shines between 45 and 100 times more brightly than the Moon. The Earth also goes through phases, just as the Moon does for us, although they are opposite from what we see from Earth. The term for this is called complementary phases.

Earthshine on the young, crescent Moon always appear after sunset or before sunrise, when the Moon is a thin crescent. Image courtesy Dan Bush www.missouriskies.org
On Thanksgiving Day, for example, when the Moon is New for us, as seen from the surface of the Moon, the Earth appears Full. A few nights later, as the sliver of a crescent Moon begins to appear in our western twilight sky, its entire globe may be glimpsed. Sunlight is responsible for the slender crescent, yet the remainder of the Moon appears to shine with a dim blush-gray tone. That part is not receiving sunlight, but shines by virtue of Earthlight: the nearly full Earth illuminating the otherwise dark lunar landscape. So Earthshine is really sunlight which is reflected off Earth to the Moon and then reflected back to Earth.
Venus and Jupiter
Those using binoculars or a small telescope will certainly enjoy the almost three-dimensional aspect of the Moon, but Venus will be rather disappointing appearing only as a brilliant blob of light, for right now, it's a small, featureless gibbous disk. That will change in the coming weeks, however, as Venus approaches Earth and the angle it makes between us and the Sun allows it to evolve into a half-Moon
phase in mid January, and a lovely crescent phase of its own during the latter part of February and March. Jupiter on the other hand is a far more pleasing sight with its relatively large disk, cloud bands and its retinue of bright Galilean satellites.

Jupiter and its four largest Moons, as seen through a telescope. Image courtesy Michael Stegina/Adam Block/NOAO/AURA/NSF
No question about it. It will hardly be an evening spending time watching TV! If the weather is clear between about 5 and 7 p.m. next Monday, be sure to get out and take a look.
Look. . . up in the sky. . . It's the International Space Station
When I was a youngster growing up in the Throggs Neck section of The Bronx, the Hayden Planetarium had a service called Dial-a-Satellite.
When you called a special phone number, you could hear a recorded message telling you when and where to look for the brightest naked-eye satellites that occasionally tracked across our local New York skies. Back then (and I'm speaking now about the mid-1960s) the only really bright satellites readily visible were actually two giant Mylar balloons... measuring about 100-feet in diameter which orbited Earth at altitudes of about 1000 miles.

The 135-foot rigidized inflatable balloon Echo I satellite undergoing tensile stress test in a dirigible hanger at Weekesville, North Carolina in the early 1960s.
These were the Echo
passive communications satellites: they actually functioned as reflectors, not transmitters. After being placed in orbit around the Earth, a signal would be relayed to one of the two Echo satellites, which were reflected or bounced off its surface, then returned to Earth. The Echo satellites were easily visible to the eye because of their highly reflective surface, but also because of their low orbits; they would appear from below one side of the horizon, cross the sky, then disappear below the opposite horizon after crossing the sky, as happens with all low Earth orbiting satellites. These spacecraft were nicknamed satelloons
by those involved in the project. Today, those two Echo satellites are long-gone, but there are now literally thousands of satellites orbiting our Earth.
By far and away, the biggest object now orbiting our Earth is the International Space Station. And if our skies are reasonably clear on Saturday, November 22, we here in the Tri-State Area will have a great opportunity to see the ISS make a long, high pass across the evening twilight sky.
It will be moving along a track that will take it roughly from Washington to just north of New York and then on toward Boston and the Gulf of Maine; it will briefly overfly our region about an hour after sundown.
It always amazes people when they are told that they can actually see the Space Station—now orbiting 218 miles above Earth—with their own two eyes; no optical aid is needed. As big as a football field, the ISS is visible by virtue of sunlight shining on its metallic skin and large solar panels. To the unaided eye it appears as a very bright star that does not twinkle and shines with a slight yellowish-white tinge. Check out this short video of it when it passed over Gloucester, Massachusetts back on Christmas Eve, 2006.
What to expect when looking for the International Space Station in the night sky.
Some assiduous astronomers have even been able to photograph the actual structure of the Space Station by tracking it with their telescope:

A composite of images of the International Space Station from a ground-based telescope. © Dirk Ewers, 2008
On Saturday, the ISS will emerge from above the southwest horizon at 5:32 p.m. Prepare yourself for this ISS pass by getting outside some minutes before it's due to appear and getting yourself acclimated to the sky and the surrounding stars. Certainly, you will immediately notice two very bright, non-twinkling silvery stars
low in the southwest. They are not stars, but planets; the brighter and lower of the two is Venus, the other will be Jupiter. Make a fist and hold it out at arm's length. When the ISS first appears, it should be roughly "two fists" to the right of Jupiter and Venus. It will appear to move straight up to a point almost directly overhead. It will then drop down toward the northeast, disappearing about 3-minutes after it first appeared, near to the northeast horizon. It actually will seem to rapidly fade out toward the end of its track as it moves into the Earth's shadow.

Path of the International Space Station on November 22, 2008 between 5:32 and 5:35 p.m. Image © Heavens-Above GmbH.
As to just how bright it should get, it should be plainly visible even from brightly lit cities; only Venus and perhaps Jupiter will be brighter. So during it's 3-minutes of visibility, the Space Station will be one of the three brightest objects in the sky!
And keep in mind that as you look at it, there are ten people who are currently onboard. Three are semi-permanent residents, staying for upwards of six months on the ISS. The other seven just recently arrived on the Space Shuttle Endeavour which was launched from Florida on November 14. The Shuttle is currently docked to the ISS and is scheduled to return to Earth on November 29.
Pretty neat, huh? Tell all your neighbors... and take the kids out for a look.
I'll be interested to see how many plan to check it out, so drop me a line if you see it.
