Monday, October 29, 2012

APOD 2.1 The Medusa Nebula

APOD 2.1 The Medusa Nebula


    The Medusa Nebula is in the constellation Gemini and is named after Medusa because of the lines which resemble braids glowing in the center of the image.  Spanning about 4 million light years and located about 1,500 light years away from us, this nebula is also known as Abell 21.  Medusa is a character from Greek mythology who is a monster with snakes for hair.  When someone looked her in the eye, they would turn to stone.  This nebula is an example of a planetary nebula which is formed when the center of a star heats excessively and the outer portion of the star is "blown away" in a stellar wind.  The glowing effect we see is a result of the heat generated by the star and the ultraviolet radiation it is emitting.  This star is transforming from a red giant, a star in a fairly late stage of its life, into a hot white dwarf star.     

Thursday, October 18, 2012

APOD 1.8 A Spiral Nebula Surrounding Star R Sculptoris

APOD 1.7 A Spiral Nebula Star Surrounding Star R Sculptoris


    
    This star, R Sculptoris, is a red giant star.  The red circles surrounding it is a very unusual spiral which was discovered with the Atacama Large Millimeter/submillimeter Array (ALMA).  This is the first time such a spiral has been observed in three-dimensions.  The ALMA telescope is the most powerful of its kind in the world.  The spiral is made up of material coming out of the star and will contribute to the dust and gas in the universe which will create future stars.  It is suspected that there is a binary star close by to R Sculptoris which it is ejecting this material towards.  Astronomers hope to discover more about how stars as large as this one evolve at the end of their lives.  Also, they think they will gain insight into how the elements making up the Earth reached our planet.  This star is in the constellation "The Sculptor," near Aquarius.  

Monday, October 15, 2012

Chapter 5 Outline

Chapter 5 Outline

  • Optical Telescopes
    • telescope: "light bucket", captures photons and concentrates them into a beam
    • Optical telescopes collect visible wavelengths
    • Refracting and Reflecting Telescopes
      • refraction: bending of a beam of light as it passes from one medium to another (straw in water looks bent)
      • refracting telescope: uses lens to concentrate beam of light and pass it through the focus (single point), distance between primary mirror and focus = focal length
      • Reflecting telescope: uses mirror (not lens) to focus light. Mirror called primary mirror, focus of primary mirror = prime focus
      • telescopes make images of their field of view, often very small
    • Comparing Refractors and Reflectors
      • reflecting better because:
        • lens focuses red and blue light differently (chromatic abberation)
        • some light absorbed by glass of lens (worse for infared)
        • large lenses heavy, lenses deform under own weight
        • lens has 2 surfaces (versus 1 of mirror) to polish and maintain
      • Largest refractor at Yerkes Obs. in Wisconsin, lens 1m diameter, relfecting have 10m
    • Types of Refracting Telescope
      • light often intercepted on path to focus so light intercepted on way to secondary mirror
      • Newtonian Telescope: light intercepted before it reaches prime focus and deflected 90 degrees to eyepiece, uncommen in large instruments
      • Cassegrain telescope: light reflected by primary mirror to prime focus, intercepted by 2ndary mirror, reflected down small hole back to primary; point behind primary mirror where light ultimately converges = Cassegrain focus
      • with more than 2 mirrors, light reflected to Nasmyth focus or into coude ("bent") room which is a separate observatory
      • Hubble Space Telescope (HST) is a Cassegrain telescope with all instruments behind primary mirror
  • Telescope Size
    • size has increased because that increases the amount of light it can collect (light-gathering power) and the detail (resolving power)
    • Light-Gathering Power
      • larger telescope = greater collecting area (total area capable of collecting radiation), have larger reflecting mirrors (refracting lens)
      • observed brightness directly proportional to area of telescope's mirror (square of mirror diameter) (5m telescope 25X brighter than 1m)
      • also direct. prop. to time it takes telescope to gather light
      • Mauna Kea has small atmospheric interference, good observation point
      • largest telescope in European Southern Observatory: optical-infared Very Large Telescope (VLT) - 4 different 8.2m mirrors
    • Resolving Power
      • resolution: ability of device to form distinct images of objects close together
      • diffraction (tendency of light to bend) limits resolution, creates fuzziness
        • Circular mirror:  angular resolution (arcsec) = .25(wavelength/diameter) when 1 micron = 10^-6 m
        • diffraction increases in prop. to wavelength used (diffraction-limited resolution)
  • Images and Detectors
    • Image Acquisition
      • charge-coupled devices (CCDs): electronic detectors used to take "pictures", made up of pixels, charges build up on pixels and 2-D image results
        • advantages of photos: more efficient (90% of photons recorded), quicker, in digital format
    • Image Processing
      • computers reduce "background noise", can correct instrumental problems
    • Wide-Angle Views
      • as angle light enters increases, accuracy of focus decreases (effect = coma)
    • Photometry
      • measurement of brightness
      • add up values in CCD pixels
      • use colored filters to limit wavelengths measured
      • can determine objects temperature
      • photometer: used for high accuracy rapid measurements of light intensity
    • Spectroscopy
      • works with optical telescopes

Observation 5

I have observed over the past few weeks that every morning, the sun appears to rise further to the South.

I observed this because when I am driving to school, at the beginning of the year when I was at the stoplight in Venice facing the Blu Cafe, the sun was directly in my eyes.  Now, every morning at the same time (7:55 am), the sun is at the other end of the restaurant and no longer in my eyes. 

Friday, October 12, 2012

Observation 4 Star Gazing Session

    On October 9th, I went to the observation session at Casey Key Fish-house from 8-10 PM.  During this time, the sky was clear but there was some light pollution in the direction of Sarasota (North).

    My favorite observation of the night was of the Andromeda Galaxy, also known as M31.  It is the only other galaxy visible through binoculars and appeared as a fuzzy, roughly circular object.  It is in the constellation Andromeda.  I also observed several satellites during the night and 4 meteors.
    I identified many constellations including Sagittarius, Scorpius, Hercules, Ursa Minor, Lyra, Corona Borealis, Aquila, Delphinus, and many more.  In Lyra, I observed the binary star known as the Epsilon Lyrae pair.  This appears as one bright star to the naked eye but when viewed with binoculars can clearly be seen to be binary.
    I also viewed two star clusters, one that appeared to be in Sagittarius and another through the telescope.  These star clusters contain thousands of stars.  Some other stars which I identified were Antares, Altair, and Vega.
   


APOD 1.7 Pan-STARRS and Nebulae


    This image was taken using the world's most powerful sky survey instrument.  It is both a camera and telescope built and operated by Pan-STARRS, the Panoramic Survey Telescope and Rapid Response System.  It was built in order to monitor near-earth asteroids that could pose a threat.  This institution is also researching how these dangerous objects could be deflected using spacecrafts.  The camera on this telescope is 1.4 gigapixels.  This picture is of an area of the sky close to Sagittarius showing the Lagoon Nebula (M8), the Trifid Nebula (M20), and NGC 6559.  These three nebulae make up the "Sagittarius Triplet."  The color in this photo has been altered, showing normally red emission in green.  This image shows about 3 degrees of the night sky.

Thursday, October 11, 2012

Johannes Hevelius Biography



Johannes Hevelius
    Johannes Hevelius was born to Abraham Howelcke and Cordelia Hecker on the 28th of January, 1611.  He was born in Danzig Poland which is located on the Baltic Sea.  Hevelius is of German and Czech descent and grew up speaking mostly German but also learning a bit of Polish in his community.  His name is often disputed as it has many pronunciations and spellings including Hevel, Hewel, Hofelius, Hovelius, and many more.  Hevelius is the most commonly used today.  He had three brothers and six sisters although he was the only son in the family to survive to adulthood.
            Growing up, Johannes was well off because his father was a wealthy brewer.  When Johannes was six, his parents sent him to a school named Gymnasium near his hometown.  He attended Gymnasium for six years until the school was closed because the Thirty Years War was going on at the time.  Next, Hevelius was sent to a school in Bromberg.  This was challenging for Hevelius because they spoke Polish there but he quickly picked up the language.  During his years of education, Hevelius was particularly drawn towards math, always having a passion for the subject.  He was greatly influenced and inspired by a math teacher, Peter Kruger, who taught him to make his own observational instruments.  At the age of nineteen, Hevelius moved to Holland where he began studying law but still found time to pursue optics and mechanics.  After receiving his law education, he travelled and lived for a short time in London until 1634 when he was called back to continue the family brewery which his father could no longer operate due to illness.
            Once he returned to Danzig, Hevelius married a woman named Katharina in 1635 and maintained the brewery.  After a few years, he was once again inspired to pursue astronomy by two successive events.  First, he went to visit his dying math teacher, who had initially instilled in him his love of astronomy, who once again urged the bright Hevelius to study his passion.  Shortly after this, Hevelius witnessed a solar eclipse on June 1st, 1639.  His dreams of studying astronomy were rejuvenated and his wife Katharina assisted him in his studies by practically taking over the brewery to give him time to study and make observations.   In 1662, however, his wife Katharina died.  Within a year he married a sixteen year old, Elizabetha.  Elizabetha shared a passion for astronomy and   assisted him more directly than Katharina in his studies.  Hevelius and Elizabetha had three children together, two sons and a daughter.  Only their daughters survived. 
            Johannes Hevelius had always hoped to be able to create a star catalog but found his efforts hindered by the fact that he was lacking instruments.  He began building his own instruments, most notably his long telescopes utilizing the technology of refraction.  The longest telescope he created was about 150 feet long.  His self-created observatory was named Sternenburg and was above other people’s houses.  His observations include the phases of Mercury.  He was eventually successful in creating a star catalog, as he had hoped, including in it 1,564 stars and their positions.  The catalog was named Prodomus Astronomiae.  He discovered and named a star of his own, Mira, located in Cetus.  In addition, he discovered Nova 1670 Cygni.  He also discovered and ovserved comets from his observatory.  He used the positions of sunspots throughout a four year period to almost accurately calculate the solar rotational period.  Although all of these are notable accomplishments, Hevelius’ most well-known feat was his publication of Selenographia.  This is a book of observations spanning ten years detailing maps of the Moon.  It included both the Moon’s phases and estimates of Lunar mountain heights.  Hevelius was the first individual to calculate the heights of Lunar mountains.  The book included 60 pictures of the Moon containing much detail. 
            Unfortunately, in 1679 a fire destroyed Hevelius’ observatory.  All of his instruments, printings, and records were lost.  The only thing saved was his star catalog.  Even though Hevelius was 68 at the time of the fire, he rebuilt his observatory to continue making observations.  Throughout his life, Hevelius made money from both his father’s passed down brewery and from a pension which he received for his work in astronomy.  He was a member of the Royal Society, a scientific association, during his lifetime. He died on his birthday in 1686.  After his death, his wife Elizabetha made sure that his star catalog, nova observations, and constellation charts were published. 

Hevelius' 140 Foot Telescope



A Detailed Drawing of the Moon by Hevelius





Formal Education Group of the Space Telescope Science Institute's Office of Public Outreach.     "Johannes Hevelius." Amazing Space: Telescopes from the Ground Up. NASA, n.d. Web.      06 Oct. 2012.

O'Connor, J J, and E F Robertson. "Johannes Hevelius." History.mcs.st-and.ac.uk. School of         Mathematics and Statistics: University of St Andrews, Scotland, 2008. Web. 06 Oct.            2012. 

Kenneth Glyn Jones, 1968. The Search for the Nebulae -- II. Journal of the British Astronomical Association, Vol. 78, No. 5 (1968), p. 360-368. Section on Hevelius: p. 366. Reprinted          in: The Search for the Nebulae. Chalfont St. Giles, 1975.

Asimov, Isaac. "[171] Hevelius, Johannes." Isaac Asimov's Biographical Encyclopedia of   Science and Technology. New Revised Edition ed. N.p.: n.p., n.d. 114-15. Print.

"Hevelius, Johannes." Complete Dictionary of Scientific Biography. Vol. 6. Detroit: Charles           Scribner's Sons, 2008. 360-364. Gale Virtual Reference Library. Web.

Thursday, October 4, 2012

Observation 3 Blue Moon Aug 31 2012

    Although I never posted my observation until now, on August 31st I observed the blue moon from the Island of Venice.  I actually observed it twice throughout the night from two separate locations.  First, I observed it at about 8:30 from the beach and then again at about 9:30 from my house.

    From the beach, the blue moon appeared bright and there was little light pollution around so it was very clearly visible along with a few stars.  There were not very many clouds so my view of the moon was unobstructed. 

    From my house, the moon seemed even brighter because it was later at night.  There was more light pollution around my house though so no stars were visible due to the increased brighness of both the moon and streetlights.  Also, there were a few more clouds so at times the moon was behind them although it was still visible because of its brightness. 

APOD 1.6 Stars In a Dusty Sky

Stars In a Dusty Sky: 28 September 2012

    The bright star in the upper right corner of this image is Markab, otherwise known as Alpha Pegasi.  This means "the horse's sholder" in Arabic and is part of the Great Square in Pegasus.  According to myth, Pegasus was born from Medusa when she was decapitated.  Blue reflection nebulae are also visible in the image.  Blue reflection nebulae are clouds of interstellar dust; visible because of their reflection of nearby stars's light.  Near the center of this picture, the distant edge-on spiral NGC 7497 can be seen.  This is a spiral galaxy.  I found this photo interesting because of the blue reflection nebulae and the extremely bright star in the upper right (Markab).