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.
Fig. 1. Our observation site was Assateague Island National Seashore, located just
south of Ocean City, Maryland.
Fig. 2. We cast long shadows because the Venus transit occurred in the hours
before sunset.
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.
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.
Fig. 5. Mark inspected our astrophotography setup.
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