Archive for February, 2009

Star News: When Satellites Collide

Space News | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

In an article in Spaceflight Now, it was reported that two satellites, a defunct Russian satellite and a commercial Iridium communications satellite, collided around 12:00 p.m. EST on February 10, 2009.  The collision obliterated both satellites.  Initial radar tracking has identified more than 600 pieces of debris.

Iridium Satellite model.

Iridium Satellite model.

According to Air Force Brig. Gen. Michael Carey, deputy director of global operations with U.S. Strategic Command, there are about 18,000 objects in space that they routinely track.  These include objects that they know about that are 3.9 inches across or larger.  The collision between the two satellites occurred at an altitude of 491 miles over northern Siberia.   According to a 2008 report by an international monitoring group called the Space Security Index, before the latest incident, it is estimated that there were over 300,000 orbital objects measuring between 1 and 10 centimeters in diameter and “billions” of smaller pieces.  Traveling at speeds that can reach many thousands of kilometers per hour, the tiniest debris can damage or destroy a spacecraft.

According to the article, in 1996, a French spy satellite was hit by a wheeling fragment left from an exploded Ariane rocket at 50,000 kilometers per hour. In June 1983, the windscreen of the US space shuttle Challenger had to be replaced after it was chipped by a fleck of paint measuring 0.3 millimeters, that impacted at four kilometers per second.  The latest collision added an additional 600 pieces that will need to tracked.

If it is not self evident, one might ask, “Why it is important to track the objects?”  Well, every time a rocket is sent into space, manned or unmanned, it is important that the rocket is not sent up in a collision course with something else already in orbit.  Objects traveling 20,000 miles an hour on a collision course do not fare well, this included astronauts.

We take space walks almost for granted these days.  When we ponder on the possibilities of a collision that might occur between a piece of space debris and an astronaut, the prospects of this are not good at all.

Back in school, we learned how a fusion reaction works.  An atom splits sending out particles which split other atoms and they in turn do the same thing.  The rate of atoms splitting continues to grow until the rate is enormous.  Now let us ponder space satellites and space debris.  What if satellites began to collide, producing hundreds of debris objects?  These resulting objects then would collide with other objects producing even more objects.  At what point do we reach a “critical mass” of space debris where it will be impossible to leave Earth and go into space without being struck by space debris?  Something to ponder……

For more information about these articles, go to one of these the websites: http://spaceflightnow.com/news/n0902/11iridium/ oor
http://www.dailystar.com.lb/article.asp?edition_id=10&categ_id=2&article_id=99326

Celestial Feature of the Week: Collinder 70

Celestial Feature of the Week | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

Winter is the best time of the year for many stargazers because the skies are clearer than at other times of the year and the winter constellations are the most prominent, at least to this observer.  Probably the most recognizable constellation is Orion, the Hunter.  We have discussed several deep sky objects within the boundaries of Orion in earlier editions of this journal.  This week we will introduce you to a deep sky object that few people are aware of but everyone can see: Collinder 70.

Collinder 70 is a large open cluster, located around the belt of Orion.   It includes all three belt stars: Mintaka (the Girdle), Alnilam (The string of Pearls) and Alnitak (the Belt).  This open cluster has a large diameter of almost 3 degrees and consists of 100 stars or more.  Most of them can be seen with a pair of binoculars, 10th magnitude or brighter.

A pair of binoculars gives you the best view of this object.  Binoculars have a large field of view allowing you to see the whole cluster at one time.  A telescope would reduce your field of view to just a small part of the cluster in one view.  It would be like trying to see an elephant through a straw!  When you look at the area with new eyes, eyes for looking at the cluster, you will get the same thrill that you had when you first saw the Seven Sisters (Taurus) or the Beehive Cluster (Cancer).

When you look at this cluster, look for multiple stars and star colors.  This turns out to be a rich field of view when you take time to inspect it closely.  As a reminder, you can best see star colors if while you are looking at them, you slowly “unfocus” the image.  This spreads the image out, revealing the colors much more vibrantly.  You might also take some time to try to sketch the star patterns that you see.   No matter what you do, enjoy the view; you will see this area in a way you’ve not do so in the past.

Orions Belt

Orions Belt

Today in History: 2/22/09 – 2/28/09

Space History | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

February 22, 1978: The first Navstar (Global Positioning Satellite) was launched into space.

NavStar ready for launch.

NavStar ready for launch.

February 23, 1987: Astronomer Ian Shelton discovered the brightest supernova seen from Earth in 383 years in the Large Magellanic Cloud, seen from the Southern Hemisphere.

supernova-1987a

Supernova 1987a

February 24, 1968: Astronomers from Cambridge University announce the discovery of pulsars.  Pulsars are highly magnetized rotating neutron stars which emit a beam of radio wave radiation.  The beam can only be detected when it is pointing at the Earth and is thus called the lighthouse effect.  These stars rotate extremely quickly, once every 1.5 milliseconds to once every 8.5 seconds.  Although the announcement didn’t take place until 1968 they were actually observed in July 1967.  What they were looking at wasn’t determined until later.

Vela Pulsar

Vela Pulsar

February 26, 1842: Camille Flammarion (February 26, 1842 – June 3, 1925) was born in France at Monitgny-le-Roi.  His colorful career in astronomy included a strong belief in life on other planets including on the Moon and on Mars.  While he was somewhat eccentric in his thinking, he authored more than 70 books and did more to encourage public interest in astronomy during his day than anyone else.  It could easily be said that, “He was the Carl Sagan of his day.”  Among his contributions, with others he extensively studied double and multiple stars resulting in the publishing a catalog of 10,000 double stars in 1878.  Clearly he was very well though of in the scientific community as evidenced by the fact that there is a crater on the Moon and Mars named after him; there is even an Asteroid (1021) Flammario named after him.

The famous "Flat Earth" Flammarion woodcut originates with Flammarion's 1888 L'atmosphère : météorologie populaire (p. 163)

The famous "Flat Earth" Flammarion woodcut originates with Flammarion's 1888 L'atmosphère : météorologie populaire (p. 163)

February 28, 1990: STS-36 Atlantis launched.  This was the 6th mission for Atlantis and the first mission which was postponed due to a shuttle commander’s illness.  Once launched, it proved to be a successful mission.

STS-36 Night Launch

STS-36 Night Launch

Telescope Corner: Why do refracting scopes seem to cost more than reflecting scopes?

Telescope Corner | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

Of course, this question is based on a generalization but a useful one in any case.  Everything else being equal, a reflecting telescope uses a mirror to collect and focus the starlight to the eyepiece while a refracting telescope uses a lens.

The logistics for making a 4” mirror are much different from making a 4” lens.   First, the material that the lens must be made from is much more precise than the mirror.  One must look through the lens so there can not be any occlusions or concentration gradients within the lens.  Since we are simple looking at an image reflected from the surface of the mirror, the purity of the material is not as much a consideration.

Secondly, when making a lens, one must shape and grind and polish two surfaces.  Additionally, these two surfaces must be in proper orientation to each other for an image to be clear.  When making a mirror, one grinds and polishes only one surface.  Finally, when placing the lens in the telescope, one can only support the lens from the sides.  A mirror can be supported from its entire back.  This advantage is clearly more obvious when the telescope becomes quite large.

Everything else being the same, refracting telescopes cost more than reflecting telescopes because a lens costs more to fabricate than a mirror.

Planet Watch: 2/22/09 – 2/28/09

Planet Watch | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

For a great website to locate the planets, go to www.nightskyinfo.com.  This site will tell you about the planets and give you a good star map to locate them.

Sunset Sky: (Sunset until 11 p.m.)

Go out in the early evening and you will see the brightest planet high in the western sky.  It is Venus, the Evening Star.  It is brilliant and easy to spot.  It will be the first object that will show itself in the twilight sky,

Late Evening (11 p.m. until 4 a.m.):

Since Saturn is rising in the east around 6:30 p.m. EST, you might begin to look for it around 9:00 p.m. to the east about 45 degrees above the eastern horizon; clearly high enough to observe from most locations.

Predawn Sky:  (4 a.m. until sunrise)

Obviously, Saturn is best seen in the early predawn sky when it is highest in the sky.  Mercury is fairly high in the early morning sky as well, and if you have good low horizon and dark skies to the east, you should be able to spot it.

Mars, Jupiter, and Neptune are still too low to observe.  By the middle to the end of March, we should begin to see Jupiter low on the eastern horizon.

Moon Watch: 2/22/09 – 2/28/09

Moon Watch | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

Sunday (22nd), the Moon passes 1.1 degrees north of Mercury at 5 p.m. EST.

Sunday (22nd), the Moon passes 0.7 degrees north of Jupiter at 8 p.m. EST.

Monday (23rd), the Moon passes 1.7 degrees north of Mars at 3 a.m. EST.

Tuesday (24th), the Moon will be New at 8:35 p.m. EST.

Friday (27th), the Moon will pass 1.3 degrees south of Venus at 6 p.m. EST.

Weekly Stargazers’ Rating: 2/22/09 – 2/28/09

Stargazer Rating | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

The Moon will be New on Tuesday so the Stargaze Rating is excellent for the whole week.  Moon enthusiasts can enjoy a waning crescent Moon early in the week and a waxing crescent Moon later in the week.  This will give them the opportunity to view the craters along each limb of the Moon as the terminator crosses them.

Satellite Watch: 2/22/09 – 2/28/09

Satellite Watch: Satellites of Magnitude 3.0 and brighter | Posted by Drew on Behalf of Dr. Bob.
Feb 22 2009

Sunday, February 22, 2009:

Okean O Rocket (Tumbling Rocket Body): 06:03 Hrs., 88Âş altitude in the NW, rising from the NNE, heading to the SSW, magnitude 2.7.
Hubble Space Telescope (HST): 06:12 Hrs, 34Âş altitude in the S, rising from the WSW, heading to the ESE, magnitude 2.7.
Cosmos 1093 Rocket Body: 19:26 Hrs., 67Âş altitude in the E, rising from the S, heading to the NNE, magnitude 2.2.
Tropical Rainforest Monitoring Mission (TRMM): 20.15 Hrs, 49Âş altitude in the WSW, rising from the WSW, heading to the WSW, magnitude 2.3.

Monday, February 23, 2009:

Hubble Space Telescope (HST): 06:11 Hrs, 30Âş altitude in the S, rising from the WSW, heading to the SE, magnitude 2.9.
Lacrosse 4 Rocket Body: 06:54 Hrs, 72Âş altitude in the ESE, rising from the SSW, heading to the NNE, magnitude 2.5.
Tropical Rainforest Monitoring Mission (TRMM): 19:21 Hrs, 69Âş altitude in the SSE, rising from the WSW, heading to the E, magnitude 1.5.

Tuesday, February 24, 2009:

Cosmos 1093 Rocket Body: 06:29 Hrs., 84Âş altitude in the ESE, rising from the N, heading to the S, magnitude 2.3.
Tropical Rainforest Monitoring Mission (TRMM): 20:03 Hrs, 77Âş altitude in the N, rising from the W, heading to the NNE, magnitude 1.3.

Wednesday, February 25, 2009:

Radcat Satellite: 05:52 Hrs, 88Âş altitude in the NNE, rising from the NNE, heading to the SSW, magnitude 2.9.
Cosmos 1093 Rocket Body: 06:32 Hrs., 46Âş altitude in the W, rising from the NNW, heading to the S, magnitude 2.5.
Tropical Rainforest Monitoring Mission (TRMM): 19:07 Hrs, 84Âş altitude in the NNW, rising from the W, heading to the E, magnitude 1.4.

Thursday, February 26, 2009:

Okean O Rocket (Tumbling Rocket Body): 06:00 Hrs., 87Âş altitude in the E, rising from the NNE, heading to the SSW, magnitude 2.8.
Helios 1B Satellite: 06:25 Hrs, 68Âş altitude in the WNW, rising from the N, heading to the SSW, magnitude 2.9.
Tropical Rainforest Monitoring Mission (TRMM): 19:49 Hrs, 78Âş altitude in the NNE, rising from the W, heading to the E, magnitude 1.3.

Friday, February 27, 2009:

Lacrosse 4 Rocket Body: 06:01 Hrs, 84Âş altitude in the SSE, rising from the SSW, heading to the NNE, magnitude 2.1.
Lacrosse 3 Satellite: 06:40 Hrs, 49Âş altitude in the WSW, rising from the NW, heading to the SSE, magnitude 2.8.
Tropical Rainforest Monitoring Mission (TRMM): 18:54 Hrs, 75Âş altitude in the NNE, rising from the W, heading to the E, magnitude 1.5.

Saturday, February 28, 2009:

Lacrosse 4 Rocket Body: 06:13 Hrs, 45Âş altitude in the WNW, rising from the SW, heading to the NNE, magnitude 2.4.
Tropical Rainforest Monitoring Mission (TRMM): 19:36 Hrs, 80Âş altitude in the S, rising from the W, heading to the ESE, magnitude 1.4.
Lacrosse 5 Satellite: 19:51 Hrs, 89Âş altitude in the NW, rising from the NW, heading to the SE, magnitude 2.5.

Rome Star Party on February 21st at Stonebridge Golf Course!

Rome Star Gazers Party! | Posted by Drew on Behalf of Dr. Bob.
Feb 15 2009

For those of you who have said you do not know much about astronomy or the night sky but “prefer to stare (into the sky) in wonder and amazement – to be “star-struck” so to speak”, perhaps you might come out to one of the star parties and let me show you some of the finer details in the night sky. You might become even more “star-struck” by the additional detail and beauty that I might be able to share with you.

Celestial Feature of the Week: Winter Hexagon

Celestial Feature of the Week | Posted by Drew on Behalf of Dr. Bob.
Feb 15 2009

Perhaps you have heard of the Summer Triangle; we have spoken of it numerous times in earlier editions of this journal.  Astronomers define an “asterism” as a “distinctive pattern formed by a group of stars belonging to one or more constellations.”  There are quite a few examples that you may have heard of: Big Dipper in Ursa Major; the Sickle in Leo, the Teapot in Sagittarius, the Great Square in Pegasus, and, as mentioned, the Summer Triangle from Aquila, Lyra, and Cygnus.  These asterisms all are alike in that they are large.  There are some asterisms, which are quite small: for example, the Coathanger in Vulpecula.

I wonder if you have ever heard of the “Winter Hexagon.”  If not, this is a great time of the year to try to locate it in the night sky because it is directly overhead early in the evening.  This asterism is very large and can therefore be a difficult shape to distinguish; it includes stars from six different constellations!

winter-hexagon

I will trace the stars and constellations that make up the Winter Hexagon in clockwise order, assuming you are facing south at the time you observe.  Starting at the top of the hexagon, the northern most point, you have Capella, the brightest star in Auriga.  From there, shift your gaze south-southwest (down and to the right) to Aldebaran, in Taurus, the Bull.  Now proceed to the south-southeast (down and to the left) to Rigel, the right foot of Orion, the Hunter.  Now, shift your gaze to the east (left) to Sirius, the Dog Star – the brightest star in the heavens.  For the fifth star, move your gaze to the northeast (up and to the left) to Procyon in Canis Minor, the Little Dog.  Next, direct your gaze to the north (up) to the twins, Pollux and Castor.  Finally, shift your gaze back to the beginning point, northwest (up and to the right), to Capella, closing the Hexagon.

Take the time to pick this large asterism in the night sky and add it to your list of objects that you have positively identified.