Friday, December 21, 2012

APOD 2.7: Spiral Planetary Nebula



The mind-blowing picture of nebula NGC 5189, also known as the Spiral Planetary Nebula (and recently called the Christmas Ornament Nebula), was recently taken by the Hubble Heritage Team. To me, this nebula resembles an approaching celestial lion, stepping forward, his tail curled up and around.

NGC 5189 is a highly complex nebula observed by the Hubble Space Telescope; it is a dying star that is part of a binary star system with a slowly-moving symmetry axis. The nebula spans about three light years and is 3,000 light years away from Earth, near the southern Fly constellation. Previous research done on NGC 5189 showed that the nebula is descended from epochs of "material outflow," lik a bright torus running across.


Friday, December 7, 2012

APOD 2.6: Lunar Halo Over Spain x4

The beautiful image, photographed by Dani Caxete, depicts a beautiful moon near Madrid, Spain, whose appearance was crystallized into having a quadruple halo due to falling ice crystals. Such a view, with a 22 degree halo, is very rare. The 22 degree arc is elongated by "column ice crystals" then also further refracted through more distant ice crystals to give the semblance of a 46 degree, rainbow-like halo. The lovely scene, as though it had been taken from a Christmas storybook, is set also by the Sierra de Guadarrama mountain range. The winter night sky scape includes many of the classic winter constellations with such stars as Sirius in Canis Major, Orion's Belt stars, and Betelgeuse within the arcs.

When the arcs and halos around the moon occur, they can be visible anywhere between a few minutes to a few hours.

Tuesday, December 4, 2012

Nathaniel Bowditch- Bibliography Listings

Taylor, W. Leonard, M.D. "America's First Mathematician, Astronomer and Philosopher: Nathaniel Bowditch." Fortnightly Club of Redlands. N.p., 9 Mar. 2001. Web. 04 Dec. 2012. <http://www.redlandsfortnightly.org/papers/Taylor01.htm>.

Berry, Robert Elton. "The Life of Nathaniel Bowditch." The Scientific Monthly 56.3 (1943): 277-78. JSTOR. Web. 4 Dec. 2012.

O'Connor, J. J., and E. F. Robertson. "Nathaniel Bowditch." Bowditch Biography. N.p., July 2000. Web. 04 Dec. 2012. <http://www-history.mcs.st-andrews.ac.uk/Biographies/Bowditch.html>.

Bowditch, Harold. "Nathaniel Bowditch." The William and Mary Quarterly 3rd ser. 3.2 (1946): 306
07. JSTOR. Web. 4 Dec. 2012. 

10 Skythings I'd like to see on 12/9 Stargaze

1. One of brightest, largest asteroids of the Asteroid Belt - Vesta, among Taurus' stars. It will be at opposition and peak visibility, at magnitude 6.4.
2. The Geminid Meteor Shower should be partially underway this week.
3. Pisces- My sun sign! I always have difficulty in making out this faint, ancient constellation.
4. Jupiter should still be highly visible.
5. Neptune, through binoculars, might be able to be seen although its magnitude will be highest after the 10th.
6. Right before dawn actually, a crescent moon, Venus, Saturn, and Mercury will be visible in the sky.
7. Pleiades please!
8. Orion shall be quite magnificent.
9. The Demon Star, Algol, in the constellation Perseus (HD19356) will be lovely and bright and having just undergone some peculiar processes.
10. Maybe I ought to get a better look at M57, the Ring Nebula, through a telescope.

Saturday, December 1, 2012

Astro-Observation Log 2.2 (12.1.12)

Today the fall sky seemed to be nearly at its zenith, because as I used my Star Walk application (which I have actually come to depend upon a little too much) the main constellations were those of the fall night sky rather than those of the summer. Stars were especially bright in my backyard, but the moon was obscured. However, a few day ago, I was taken aback by the brightness of the yellow full moon- known by Native Americans as the Beaver Moon.

I had difficulty making out many of the constellations, but on the ecliptic, I managed most successfully in discerning Aquarius. The circlet and lines of Pisces were rather faint, and I barely cut put the stars together for it. Pisces, I learned, however, is one of the more ancient constellations. There was an extremely bright spot in the sky which surprised me because Star Walk made it seem like it was Jupiter, but it was most likely Algol, a huge star in Perseus. Both Andromeda, the princess, and Cassiopeia, the queen, were also quite visible. The planets are... scattered about.

Friday, November 30, 2012

APOD 2.5: Sand Cascades on Mars

The photo, courtesy of NASA (taken by the Mars Reconnaissance Orbiter in 2008) displays odd, pinkish brown chasms, dunes and streaks. The lighter, blueish areas show frost on the dark sand. The spring Sun melted most of the carbon dioxide ice, but some remains at the top of these Mars hills. When dark sand cascades down the dune, it leaves the dark streaks, and it looks like patches of trees growing. The objects are only about 25 centimeters across in reality. The billowy plumes show that the sand was sliding even as the picture was taken. The picture was taken near Mars' north pole!

Friday, November 16, 2012

APOD 2.4: Polar Ring Galaxy NGC 660


The photo, taken by Travis Rector at the Gemini Observatory using the Gemini North telescope on Mauna Kea, features Polar Ring Galaxy NGC 660. It is very bizarre but smooth image of a cosmic entity that is 20 million light-years away and within the Pisces constellation. Polar Ring galaxies are rare, and  consist of a lot of stars, gas, and dust that orbits in rings that are perpendicular to the galactic disk plane (the plane at which all the spirals and bars and galaxies exist). The configuration is shaped in this odd way as it could have picked up material from disk galaxy on a rotating ring, thus creating the pink star regions. NGC 660 spans over 50,000 light years.

Friday, November 9, 2012

APOD 2.3- Hunter's Moon Over Alps


The image depicts a beautiful "Hunter's Moon," which contracts in the dark sky with the illuminated pink mountain peak in the Italian Alps known as Rochemelon. While this peak catches the first light of the rising sun, the moon is still very prominent, being the second full moon after the northern hemisphere autumnal equinox, happening during the last week of October. Full Moonsets have many epithets, including, besides the Hunter's Moon, the Wolf Moon, the Snow Moon, Milk Moon, Harvest Moon, and Oak Moon.

Monday, November 5, 2012

Astro-Observation Log 2.1 (11.3.12)

Last Saturday night, I went to a stargazing session out in a rather secluded part of the city, and saw more stars in the night sky than I have ever seen in my life. The Milky Way Galaxy was curving above us all, and the teacher used a fancy laser gadget to point out the boundaries of the constellations and other features of space.

Sadly, I forgot the name/type of the exact telescope that was used. But it could be programmed to focus on anything that the teacher specified. Such sights through the telescope included M13 and M57.

There were many satellites that could be seen floating above us. How adorable!

Apparently, there were also many meteors and shooting stars. Yet I, being a true space cadet (ironically in this context), happened to be looking down as they flashed away.

My favorite sight was one I viewed through a pair of binoculars- the twinkling Pleiades. I saw them form various geometric shapes. Or perhaps my hand was just shaky. Taurus be flashy.

Friday, November 2, 2012

APOD 2.2: Mammatus Clouds Over Saskatchewan


I have never seen such bizarre looking clouds in a picture that has not been photoshopped- the clouds look like balloons/bags of air or jellyfish, or a woman's breasts, for which they are named after. They are called Mammatus clouds.

These cloud pockets occur when water and ice falls into clear air during evaporation. They are usually a precursor to extreme weather, and are accordingly perceived as an ominous sign- although they are beautiful and unique. They tend to appear in "turbulent air" if there is a thunderstorm nearby. They can extend for hundreds on miles.

The picture was photographed in Regina, Saskatchewan, Canada during the summer. The Mammatus clouds look especially dramatic because of the sunlight appearing on the side.


Monday, October 29, 2012

APOD 2.1- "Merging NGC 2623"

NASA's astronomy picture of the day from October 19 is an elegant sort of shape, and mixes the orange sorbet color scheme of a conch shell.

The image displays what is known as NGC 2623, which is actually two galaxies becoming one some 300 million light-years away towards the zodiacal constellation Cancer. Such a uniting is likely similar to the one that happened with the Milky Way Galaxy with its combining nucleus. Star formation ensued around the newly-forming nucleus, for many, many miles, part of tidal tails, with luminous stellar dust and gas.

Friday, October 19, 2012

APOD 1.8 - The Hubble Extreme Deep Field

I remember the day this photo came out; my family was genuinely excited about it, as it is the farthest-shot image from space ever taken. Something so beautiful and helter-skelter is ineffable to me, though deep space seems to bear a remarkable resemblance to the final unexplored frontier of Earth, which is the deep sea. Pitch blackness with unusual sources of wild color.

Anyhow, the image reveals some of the most ancient galaxies ever seen by man- by ancient, we are talking billions and billions of years. All that time is difficult to comprehend.

The infrared channel of a Hubble camera took the shot. It is considered an eXtreme Deep Field (XDF) shot. The XDF will continue to be heavily studied and utilized by astronomers.

Wednesday, October 17, 2012

Astronomy Observation Log 4 (Astronomy Cast - The Hubble Space Telescope)

Managing to get a telescope above the atmosphere is a tremendous feat for mankind, benefiting our knowledge of space in an incredible amount of ways and also illuminating the beauty of distant celestial objects. 

As the podcast makes an important point of, the atmosphere has been "astronomers' worst enemy."

The concept for the Hubble Telescope, an extraterrestrial tool, arose in the 1940s. The materialization of the actual instrument came about by the 60s. Many great astronomical affairs take part through committees- the funding for the Hubble Telescope was no exception, although even Congress lent money to the affair. The Hubble Space Telescope was carried into orbit in 1990. 

Originally, there were major issues with the curvature of the telescope's mirror- the outside was not sufficiently polished, and the first pictures taken by it were hideous. Once the astronomers in charge figured out this error with the outer edges of the mirror, they could fix the failing facets and install new detectors. Astronauts, interestingly, are excellent construction workers for these instruments in space...

Corrective optics were incorporated directly into the instrument. Improvements are consistently being made upon the Hubble.

I learned from the podcast that infrared is one of the most important parts of the spectrum for astronomers, because it allows them to see the most distant parts of the galaxy. The Hubble Space Telescope was the first to allow us to pick up on those incredibly long wavelengths.

The Hubble Space Telescope has been serviced many times. 

Monday, October 15, 2012

Ch. 5 Sections 1-3

5.1- Optical Telescopes


  • Telescope = A "light bucket" whose primary function is to capture as many photons as possible from a given region of the sky and concentrate them into a focused beam for analysis.
    • Optical telescopes are designed to collect wavelengths visible to the human eye.
    • History since Galileo in 17th centuries.
  • Refracting telescopes use lenses to gather and concentrate a beam of light. 
    • Lens thought of as series of prisms combined in a way so that all light rays arriving parallel to its axis (imaginary line through center of lens) are refracted to pass through a single point called the focus. Distance between primary mirror and focus is focal length. 
  • Reflecting telescopes use curved mirrors instead of lenses to focus the incoming light.
    • The mirror that collects the incoming light is called the primary mirror, as telescopes often have more than one mirror. Focus of the primary mirror is called prime focus.
  • Prime-focus images are often magnified with a lens called eyepiece before being observed by eye, or recorded as a photograph/digital image. 
  • Reflecting telescopes tend to be favored over refracting ones:
    • The fact that light must pass through the lens is a disadvantage of refracting telescopes. Tends to focus red and blue light differently.
    • When light passes through lens, glass absorbs some of it. This is a problem for infrared and ultraviolet observations because glass blocks most of the radiation in those regions.
    • Large lenses are heavy, so they deform under own weight. Meanwhile, a mirror doesn't have this problem because it is supported over it's entire back surface.
    • A lens has two surfaces that must be accurately machined and polished, while a mirror only has one. 
  • Types of reflecting telescopes:
    • In Newtonian telescope, the light is intercepted before it reaches the prime focus and then is deflected by 90 degrees, usually to an eyepiece at the side of the instrument. Uncommon in larger instruments but popular for smaller more common ones.
    • In Cassegrain telescope, incoming light hits the primary mirror and then is reflected upward toward the prime focus, where a secondary mirror reflects the light back down through a small hole in the main mirror into a detector or eyepiece. Has rear platform. 
    • In Nasmyth/coudé focus, starlight is reflected by several mirrors- by primary mirror toward prime focus, down the tube by a secondary mirror, and then a third, smaller mirror reflects light out of the telescope where the beam may be analyzed by a detector mounted alongside, at the Nasmyth focus, or via a series of further mirrors into an environmentally controlled laboratory "coudé" room. This lab room is separate from the telescope itself, allowing astronomers to use heavy and finely tuned equipment that cannot be placed at any other foci.
5.2- Telescope Size

  • Development of astronomical instruments has led to an increase in size for 2 reasons: The amount of light a telescope can collect- light-gathering power.Amount of detail to be seen- resolving power.
  • Light-gathering power
    • Larger telescopes have greater collecting area- total area capable of gathering radiation.
    • Observed brightness of an astronomical object is directly proportional to the area of our telescope's mirror and therefore to the square  of the mirror diameter. (eg. a 5-m telescope will produce an image 25 times as bright as a 1-m instrument.) Relationship also in terms of time required for a telescope to collect enough energy to create a recognizable image on a photographic plate.
  • Resolving power
    • Larger telescopes have finer angular resolution- Ability of a telescope to distinguish between adjacent objects in the sky.
    • Diffraction and light bending around corners limits resolution. When rays spread out and are not focused to a sharp point, fuzziness ensues. 
    • The amount of diffraction is proportional to the wavelength of the radiation and inversely proportional to the diameter of the telescope mirror. 
    • For a circular mirror and "perfect" optics we can write: angular resolution (arcsec) = 0.25(wavelength(in micrometers)/diameter(m)) when one micron is 10(^-6) m
    • Diffraction-limited resolution- Theoretical resolution that a telescope can have to to diffraction of light at the telescope's aperture. Depends on the wavelength of radiation and the diameter of the telescope's mirror.
    • Larger telescopes produce less diffraction than small ones.
5.3- Images and Detectors

  • Many different detectors and devices to study radiation are placed at various points along light path outside the telescope.
  • Computers play a vital role in observational astronomy.
    • Electronic detectors called charge-coupled devices (CCDs) send output directly to a computer. Composed of many tiny pixels, each of which records a buildup of charge to measure the amount of light striking it.
    • The amount of charge is directly proportional to the number of photos striking each pixel, or the intensity of the light at that point. Buildup of charge is monitored electronically.
    • Advantages of CCDs include: 
      • they are more efficient than photographic plates, recording as many as 90 percent of the photons striking them, compared with less than 5 percent for photographic methods. thus shows objects 10 to 20 times fainter. does this in less than a tenth of the time of photographic techniques.
      • CCDs produce a faithful representation of an image in digital format that can be placed directly on magnetic tape or disk or across a computer network to an observer's home institution.
  • Computers used to reduce background noise of astronomical images. Noise corrupts integrity of messages
  • Large reflectors are good at forming images of narrow fields of view, wherein all the light that strikes the mirror surface moves almost parallel to the axis of the instrument. 
  • As angle at which light enters increases, accuracy of the focus decreases. Effect is called coma, which worsens as we move farther from the center of the field of view. 
  • Photometry- Measurement of brightness of star. Astronomers often combine photometric measurements using colored filters to limit the wavelengths they measure.
  • When highly accurate and rapid measurements of light intensity are required, a specialized device known as a photometer is used, to measure the total amount of light received in all or part of the field of view.
  • When astronomers want to study the spectrum of incoming light, large spectrometers work in tandem with optical telescopes. 

Sunday, October 14, 2012

Astronomy Observation (Log 3) 10.14.12

As I have not yet attempted to use my telescope yet, I again analyzed the sky with the help of the Star Walk application. Clouds were covering some areas of the sky, but especially along the ecliptic, I was able to make out clear distinctions between constellations. From my front yard, I saw the individual stars that made up both my zodiac sign Pisces, and also Aries. I could see Ursa Minor, with the north star Polaris standing out very clearly. There was a new moon, and I saw what I thought might have been Jupiter, but it was near the constellation Perseus. I also saw the set of constellations that include Vulpecula and Delphinus.

Friday, October 12, 2012

APOD 1.7- Color Illusion

When you see the image from the NASA APOD website without rolling your mouse over the image, the line connecting A and B is not there, which makes the illusion much trickier. With the two squares connected, it is easier to see that the colors of A and B are actually the same! This does not seem like something that is directly connected to astronomy, but it is meant to be a testament to the fact that human observations, especially those based on celestial objects, are certainly are not always reliable- as the majority of people are likely to be quick to think that the squares are different colors. Even with using measuring devices, people cannot always escape the illusions perceived by the brains and eyes of humans.

Thursday, October 11, 2012

Grimaldi Biography


Letts 1
Olivia Letts
Mr. Percival
Astronomy, Per. 3
12 Oct. 2012
Francesco Grimaldi – A Life
            Francesco Maria Grimaldi had the opportunity to become highly educated, being born into a well-respected and well-to-do family in 1618 in Bologna, Italy.  The seventeenth century, generally considered to be the final century of the Italian Renaissance, was a time marked by both great religiosity and fervent intellectuality.  Grimaldi’s life reflected this – by 1632, he and his brother Vincenzo had joined the Society of Jesus (for Jesuits).  He studied philosophy in Parma, Ferrara, and Bologna.  One of his teachers, Giovanni Riccioli, would later assist and be assisted by Grimaldi during some important experiments.  From 1638 to 1642 he taught rhetoric and humanities at the College of  Santa Lucia at Bologna, where he also studied theology after 1642.  By 1647, he was qualified to teach philosophy, but this was a time-consuming course to teach and thus, suffering from tuberculosis, he had to teach something that he found “less strenuous.” He began to teach mathematics and physics, being skilled in all branches. Full vows for priesthood were taken by Grimaldi in 1651. 
From the 1640s until his death in 1663, he focused heavily on his chief interests, astronomy and optics.  He was the first to observe and record the optical diffraction phenomenon; he was also the one to name it (diffractio).  This was discovered after during a specific experiment in which he introduced sunlight into a darkened room through a tiny hole, projecting it only a white surface.  Between 10 and 20 feet from the slit, Grimaldi put a thin, opaque rod into the cone of light so as to cast a shadow on this white surface.  He was surprised to note that the shadow of this cone was far wider than how it was geometrically predicted, and
Letts 2
also, there were external diffraction bands of different colors bordering the shadow.  The brightness of these colors was more intense near the shadow, in fact.  In 1665 he published these findings.  Grimaldi had conducted other experiments for diffraction, where he discovered internal paired tracks of light and “fringing.”  His findings further proved the fluid nature of light as opposed to rectilinear passage. Grimaldi’s Physico-mathesis de lumine, published in 1666, the geometrical foundations for the wave theory of light were laid.  Later, Isaac Newton would create a set of careful measurements that made it clear that the phenomenon was of a periodic nature.  Yet this great figure himself did not accurately reflect upon Grimaldi’s experiment, as he treated the concept of diffraction like a mode of refraction, and he could not explain the fringes of color that occurred around the shadow.  Grimaldi as well was never able to properly explain why diffraction occurred – his death was sudden and interrupted further experiments with light - this was not accomplished by anyone until Joseph von Fraunhofer could in the 1800s.
            With former teacher Riccioli, Grimaldi carried out another important experiment, in which the two Jesuits dropped weights from a tower and timed the occurrences with a pendulum. They discovered the time of the fall squared was proportional to the distance of free fall source to rest.  Grimaldi was considered vital to Riccioli’s completion of his Almagestum novum, a major work which actually made Riccioli an incredibly important contributor to astronomy and falling bodies.  Riccioli noted Grimaldi’s great skill in devising and building telescopes and other observational instruments, through which the two frequently observed celestial bodies.  Grimaldi is well-known for his lunar measurements, and his famous selenograph of the moon.  There is a copy of this lunar map in the entrance to the National Space Museum in Washington, D.C.  He began a trend of describing lunar regions by naming them after famous astronomers and physicists.  Grimaldi often did not receive proper credit for his findings, and during his lifetime, his works were not published by his name.  

Thursday, October 4, 2012

APOD 1.6- Goat Aurora

The picture of the "Goat Aurora" over Greenland is one that looks surrealistic, and indeed, incredibly goat-like. This aurora was very vivid, and fast-changing, so that even veteran sky-watchers were genuinely shocked by its appearance. This head of a goat apparently morphed into other forms as well, including an elephant and "fingers on a celestial hand." The Milky Way Galaxy also shone bright during that late august night spectacle, with a variety of constellations and nebulas visible to the naked eye. The farm in the picture is in Tasiusaq, Kujalleq, Greenland.

Seeing this picture reminds me how difficult it actually is to connect stars that form constellations... There are so many stars dotted around them in this rich sky that often I cannot possibly link together the groups of stars.

Sunday, September 30, 2012

Astronomy Observation Log 2 (Astronomy Podcast EP 133: Optical Astronomy)

Optical astronomy is essentially the branch of astronomy in which we use telescopes (commonly reflecting or refracting telescopes) to observe celestial bodies. It is still the most "cherished" branch of astronomy, and was essentially the only kind there was until the last century.

One of the interesting things discussed is how the eye collects photons, and can use up certain chemicals after having gazed at an overly bright object. Because optics and opthalmology fascinate me, I liked hearing from the podcast on optical astronomy all the information that related to these topics.

Everything absorbs some colors and reflects others. The color that an object glows depends on two main things. Its temperature, and the way the chemical sensitivities of our eyes take in various mixtures of photons.

A little over half the podcast was about optics, with some ties to the glow of distant planets and the color of the sun, but later on they began to bring about more discussion on these points relating to astronomy.

Oxygen is excited to a specific temperature in different areas of a nebula, which affects the color it gives off. The less collisions of the oxygen molecules that are happening the fuzzier the vision of these bodies will be. Specific elements with specific electron transmissions are also what send color. Honestly, all the different ways we receive color and the different effects of chemical happenings on our eyes confuses me very much.

The atmosphere presents the biggest challenge when we are observing bodies in space. Hot and cold pockets are like lenses changing the path of traveling temperatures which come off as light. That is only one of the ways our atmosphere poses a challenge, especially when the bulk of us use fairly amateur telescopes to capture light.

Friday, September 28, 2012

APOD 1.5- Over Corona Australis

NASA's featured astronomy picture for September 27, 2012 was a shot of giant wafts of cosmic dust, along with numerous tiny stars, over the constellation of Corona Australis. Normally I have great trouble in identifying the series of stars that compose a constellation, especially when there are so many other bright objects in the sky from the Milky Way galaxy, but I can easily distinguish those that outline the "Southern Crown." The dark, thick part of the dust cloud is presumed to stretch for about eight light-years. The stunning bright blue spots are actually reflection nebulae, the light coming from hot stars reflected onto the dust.

Thursday, September 27, 2012

Francesco Grimaldi - Bibliography Listings


Resources for Francesco Grimaldi Biography:


Hall, A. R. "Beyond the Fringe: Diffraction as Seen by Grimaldi, Fabri, Hooke and Newton." Notes 
and Records of the Royal Society 44.1 (1990): 13-23. JSTOR. Web.

"Grimaldi, Francesco Maria." Complete Dictionary of Scientific Biography. 2008. Encyclopedia.com. 27 Sep. 2012 <http://www.encyclopedia.com> Web.

"Francesco M. Grimaldi, S.J. (1613 to 1663) and His Diffraction of Light." Francesco M. Grimaldi, S.J. N.p., n.d. Web. 27 Sept. 2012. <http://www.faculty.fairfield.edu/jmac/sj/scientists/grimaldi.htm>.

O'Connor, J. J., and E. F. Robertson. "Francesco Maria Grimaldi." Grimaldi Biography. N.p., n.d. Web. 27 Sept. 2012. <http://www-groups.dcs.st-and.ac.uk/~history/Biographies/Grimaldi.html>.

Monday, September 24, 2012

APOD 1.4 - The Pencil Nebula

My favorite objects in space are nebulas, and through NASA's astronomy picture of the day I discovered yet another - the Pencil Nebula, which is included in the New General Catalogue of Nebulae and Clusters of Stars as number 2736. It is 800 light-years away and a small part of the very large Vela supernova remnant. The nebula itself is from a star that exploded presumably about 11,000 years ago. Originally these visible, billowous salmon-colored ripples moved at very high speeds, but they have come to slow considerably, sweeping up interstellar gas in the process.

Sunday, September 16, 2012

APOD 1.3- Ring Nebula

The featured picture is not actually a photograph of the Ring Nebula (found in the constellation Lyra), but a sketch done by Frédéric Burgeot. Though it was done beneath the eyepiece of an excellent 40-in. reflecting telescope.

The Ring Nebula, about one light-year across, consists of wavelike, intense ultraviolet layers radiating off of a dying star. The reddish color in the outer rings comes from the ionized hydrogen.

Astronomy Observation Log #1

Date: September 15, 2012
Time: 11:00 PM-12:00 AM
Place: Osprey, FL
Sky conditions: New moon; many scattered clouds but a fairly clear sky.

Instruments used: Naked eye, Starwalk Application

Planets: Found Venus

Bright stars noted: Formalhaut, in Piscis Austrinus. Altair of the Summer Triangle

Constellations noted: Corona Australis, Scorpius, Ophiuchus, Aquarius, Capricornus, Pisces, Piscis Austrinus, Cetus, Microscopium

Friday, September 7, 2012

Coincidence or Intention?

I had been wondering what constellation might have served as inspiration for Vincent Van Gogh's immortal painting Starry Night. I found a website, that interestingly enough, reveals the very strong similarities between the constellation of the Ram, Aries, and the placement of the bright stars of Starry Night.
http://www.vggallery.com/forum/forum_18a.htm

APOD 1.2: Perseid Meteor over Albrechtsberg Castle

The picture, taken by SebastianVoltmer, shows a bright descending meteor from the yearly perseid meteor shower. Albrechtsberg Castle in Austria, located on the northern bank of the river Peilach and near the town of Melk, is an excellent location to view these annual meteor showers from, along with other night-sky beauties. On August 12, northern summer constellations such as Aquarius, Aquila, and Delphinus could be viewed. The trail of the meteor (entering Earth's atmosphere at 60 km per second as dust grains from the tail of the Swift-Tuttle comet) gesticulates to the constellation Perseus.

Thursday, September 6, 2012

Sept. 2 2012 NASA APOD 1.1 :RBSP Night Launch

The elegant stream of incandescent light in NASA's featured picture from September 2 denotes the path taken by an Atlas V rocket (an expendable launch system) last Thursday morning over Florida's Cape Canaveral Air Force Station. The long camera exposure allows us to see this composite of two composures.

NASA's twin Radiation Belt Storm Probes (RBSPs) are currently in separate orbits within the forbidding Van Allen radiation belts, their mission being to explore the dynamic conditions of these belts. Most spacecraft vehicles avoid these fiery radiation belts.

Photo by Mike Killian

Saturday, September 1, 2012

Once in a Blue Moon

Throughout my writings and texts and diary entries, the phrase "once in a blue moon" is commonly found, as it is an expression I used to be very fond of reiterating.

Last night, there was a blue moon. Sadly, it was not actually blue. Yet its appearance marked a night of importance for some, as it was the second full moon of August.

The phenomenon of two full moons in one month occurs about every three years - while it is not as rare an occurrence as the old proverb might have denoted, it is still something that many people take note of and something that various cultures have created names for.

Neil Armstrong's family asks that you appreciate the full moon and "give him a wink" the next time you walk out on a clear night and glance up at our very own natural satellite.











The information I attained, and the wonderful pictures from around the world of last night's moon come from:

 http://photoblog.nbcnews.com/_news/2012/08/31/13595968-blue-moon-shines-around-the-world?chromedomain=cosmiclog&lite