Transit of Venus (June 2012)

A Rare But Familiar Sight

Venus transits are the rarest type of solar eclipse with over a hundred years elapsing between occurrences.  They occur when the planet Venus passes directly in front of the Sun.  A Venus transit occurred in 2004, and we traveled to South Africa to witness it.

   Because of the peculiar celestial geometry involved, Venus transits happen in pairs, with a second one occurring 8 years after the first one.  Thinking about the Venus transit brought back good memories, so John planned a day off for the possibility of seeing a second one, a portion of which was to be visible from Baltimore.  However, seeing a second one would require more luck than the first one because clear skies are much less likely in Maryland than in South Africa.

   On the night before the event, the prospects for clear weather in Maryland were dismal.  However, we have found Clear Sky Charts to be a reliable predictor of clear skies in North America, and this web site predicted clear skies over Ocean City, Maryland.  So, we hastily assembled our astrophotographic and toddler care gear for a last-minute road trip (Figs. 1 and 2).

   With the help of Google Maps, we chose a waterfront picnic area on Assateague Island as our observation site.  The waterfront location would give us a clear view of the western horizon, an important consideration because the transit was to begin only a couple hours before sunset, when the Sun is relatively close to the horizon.  The drive to Ocean City was completely surrounded by a sense of uncertainty because the sky was filled with large clouds.  But when we arrived at our destination, the skies cleared almost miraculously, and we were able to observe and photograph most of the event (Figs. 3 and 4).  The next Venus transit will occur in the year 2117 and will not be visible from most of the US.

(back to home page back to home page)
      Image
Fig. 1.  Our observation site was Assateague Island National Seashore, located just south of Ocean City, Maryland.

Image
Fig. 2.  We cast long shadows because the Venus transit occurred in the hours before sunset.
 
Image
Fig. 3.  Silhouette of Venus near the beginning of its crossing in front of the Sun, as photographed by us from Assateague Island National Seashore on 2012 Jun 5 at 22:47 UT (6:47 pm EDT, local time).  Venus is the black disc near the upper left edge of the Sun.  Also visible are small sunspots, representing temporary cold spots on the Sun's surface. The grainy appearance of the Sun's surface is caused by convection currents.  The Sun's natural color is white, as shown in this photograph.  IMPORTANT: safe observation and photography of the Sun require special filters.
 
 
Play
Fig. 4.  Time-lapse movie (0.6 Mb) covering the beginning of the Venus transit.  In this time-lapse sequence, time has been sped up by a factor of approximately 225.  Clouds obscured the beginning of the transit.  The sequence ends just before sunset, when the Sun becomes reddish and drops behind some distant clouds.  The clouds are at an angle because the telescope is tracking along the celestial equator rather than Earth's equator.  Playing this movie requires web browser support of HTML5 video.

Image
Fig. 5.  Mark inspected our astrophotography setup.

Image
Fig. 6.  Sunset view of western horizon from our observation site.
     
Equipment Details (optional reading, as usual)

This was the first major trial of a new telescope for us, an Astro-Physics 5-inch apochromatic refractor (Fig. 5).  Astro-Physics manufactures some of the best telescopes designed for amateur astronomers.  These telescopes are in high demand because they are competitively priced but not mass-produced.  On a whim, we got on the Astro-Physics waiting list back in 2003 when we first became serious about astrophotography, and our name came up 8 years later in 2011!  Fig. 3 is the highest resolution solar image we have obtained so far, an example of the telescope's capabilities.  The complete technical details of our outing appear below.
  • GPS location:  N 38.209500°, W 75.168298°, altitude 0.5 ft (Fig. 6) (show Google map)
  • Solar filter:  full-aperture Baader Planetarium AstroSolar safety film
  • Telescope:  Astro-Physics "Gran Turismo" apochromatic refractor (130 mm aperture, 820 mm focal length)
  • Camera:  Canon EOS 5D Mark III digital SLR (22-megapixel resolution, full frame 35 mm format) mounted at telescope's prime focus
  • Telescope mount:  telescope and camera placed on Losmandy GM-8 equatorial mount with digital clock drive to compensate for Earth's rotation
  • Polar alignment:  performed in daylight, based on site latitude, longitude, and UTC (according to Garmin eTrex Venture HC GPS receiver) and hour angle of Sun (according to Starry Night Pro software)
  • Power:  automotive battery booster pack with 12V low-dropout voltage regulator
  • Image acquisition:  camera shutter manually set to 1/1600 s (ISO 200), automatically released at 15-second intervals by a Canon TC-80N3 timer remote control, images in RAW and JPEG format
  • Image processing:  aligned each image based on centroid calculation or visual adjustment in Photoshop; custom Photoshop scripts for alignment, resizing, and cropping; assembled final time-lapse frames with Apple's QuickTime Pro 7 software; RAW conversion and contrast enhancement of Fig. 3 in Photoshop


back to home page back to home page

Apple   BBEdit
(Main content: 6/9/2012)