Transit of Venus on June 5th, 2012

If you visit the Public Observatory during its daytime hours in May (1–3pm on Wednesday through Saturday, weather permitting), you can use the 16” telescope to observe an object which looks a lot like the Moon.  Hanging in a blue sky, it shines with yellowish reflected sunlight.  We can currently only see part of its illuminated side, giving it a crescent shape.  You won’t spot any craters, though, and it looks a little fuzzy.  It’s not the Moon, but the Earth’s twin, Venus — the planet which is most similar in orbit and size to the Earth.  All eyes are on Venus now as it prepares for the show of the century: a transit across the face of the Sun.

 

Venus

Venus as seen through telescopes at the Public Observatory on April 25, 2012.

Venus and Mercury,  the only two planets which orbit closer to the Sun than the Earth, can be seen in crescent phase when they start to pass between the Sun and the Earth.  The only source of illumination is the Sun, so when Venus is between the Sun and the Earth, we see mostly the dark night side and only a sliver of the daylit side.

 

phases of venus

Phases of Venus. Image Credit: NASA

When Venus passes between the Earth and the Sun (its new phase), it is invisible because we are looking at its nighttime side.  Venus is no more than a few degrees away from the Sun at this point, so anyone attempting to observe Venus when it is new or a slim crescent should be careful to not point their telescope at the Sun, even for an instant.  Permanent eye damage could result from such an accident.

Does Venus go directly between the Earth and the Sun and cast its shadow on the Earth?  Usually not.  The orbit of Venus is tipped 3.3° with respect to Earth’s, so when Venus passes through its new phase, it usually goes above or below the Sun.  Sometimes, however, the orbits line up.  When Venus crosses directly between the Sun and the Earth, it blocks only 0.1% of the Sun’s light. The drop in overall sunlight is not noticeable, but when viewed through a telescope (safely!), the silhouette of Venus appears as a dark dot in front of the bright Sun.  This event is called a transit.

 

Venus Transit

The 2004 transit of Venus, observed by NASA's TRACE satellite. The faint halo on the lower left edge of Venus is sunlight shining through its atmosphere.

Transits of Venus occur at regular intervals, but they are rare.  They come in pairs eight years apart, and more than a century passes between pairs of transits.  There was a transit in 2004, and the second one in that pair occurs on June 5-6, 2012.  The next transit will not happen until 2117.  For nearly all of us, this is our last chance to see this event.

The transit can only be viewed by safely observing the Sun.  During the 6-hour transit, Venus will be silhouetted against the disk of the Sun.  Looking at the Sun with the naked eye can hurt the eyes, and pointing a telescope without a safe solar filter at the Sun will cause immediate telescope damage or permanent eye damage.

Here at the Public Observatory in Washington, DC, the transit will start shortly after 6 pm on June 5, 2012. The dome of the Observatory will already be in the shadow of the National Air and Space Museum building, so if the weather is clear, we will set up safe solar telescopes just outside the Museum’s entrance facing the National Mall.  We will follow the transit until the Sun gets too low in the sky to observe.  Sunset is at 8:31 PM that day, and we will see less than half of the transit from Washington, DC.  We will also stream a live image to the Web, and tweet updates at @SIObservatory. The event is paired with a free presentation by Museum staff about the history and science of transits of Venus, a free lecture inside the Museum on detecting the transits of planets in front of other stars and, later, nighttime observing in and around the Observatory.

 

solar telescope

Visitors using a safe solar telescope outside the Museum in Washington, DC.

Check with your local observatory or astronomy club for a public transit viewing event near you (whether it is visible depends on your location in the world), or check the Solar Dynamics Observatory’s map.  There are ways to observe the Sun safely at home if using proper equipment.  You can use eclipse glasses to safely observe the Sun, though the dot of Venus against the unmagnified Sun is at the limit of the eye’s resolution.  Finally, NASA is planning to stream the event live from the summit of Mauna Kea in Hawai’i, which is very likely to have good weather.  The entire transit will be visible from that location.

On June 5, 2012, solar telescopes around the world and in space will point to the Sun, marking another beat in the centuries-long dance of the planets.  Wherever you are in the world, whether your skies are clear or cloudy, it’s not an event to miss!

Geneviève de Messieres is an astronomy educator at the National Air and Space Museum.

 

Learning to Capture the Sun

The Public Observatory Project is just over a year old now, and in that time we’ve been  experimenting with the telescope to discover what is visible in the daytime sky and devise ways that our visitors can have the best experience possible.  One of our goals is to use our equipment to take images of the Sun, so that we can share our star’s day-to-day activities with the visiting public as well as those who can’t make it to the Mall to look through our telescopes.  We wanted to capture true-to-life images of the Sun as it appears through our telescope and make interesting features clearer and more apparent.

It would be dangerous to use a normal telescope to look at the Sun because the Sun’s concentrated and unfiltered light would damage your eyes.  One of the tools we use to look at the Sun safely is our Lunt Solar Systems hydrogen-alpha telescope that filters out all but one wavelength of red light. This makes it safe for viewing a part of the Sun’s atmosphere, called the chromosphere.  To take images of the Sun, I started out with this telescope, as well as a Lumenera SKYnyx 2-0 Color camera that fits where the eyepiece usually goes. We also have a laptop with software to control the camera, called Lucam Recorder.  With these in hand, I set off to take some of my first images of the Sun.

sun

This image of two prominences was taken on June 8, 2010.

Through some experimentation, I found out that different exposure settings revealed very different details on the Sun. First I cranked up the exposure to capture the faint prominences coming off the edge of the Sun and took a series of images. Next, I turned down the exposure to what I thought was an appropriate level to capture details on the Sun’s surface before taking a second series of images. I used a processing program called the GIMP to merge the two images by selecting the disk detail and moving it on top of the prominence image.  But, something wasn’t quite right. This didn’t look much like what I was seeing with my own eyes. So, I turned to a local amateur solar imaging expert and friend of the National Air and Space Museum: Greg Piepol.

Greg’s solar imaging work, which you can check out on his website sungazer.net, has been praised for its beauty and attention to detail. My colleague at the Observatory and fellow Sun imager, Katie Moore, and I were thrilled that he agreed to come into the Museum and show us how he captures such stunning images.

Greg taught us several things that improved our imaging. The first and most important was that we had been drastically overexposing the disk of the Sun, which washed out the details we were trying to capture. Greg also taught us how to better use an image stacking program called Registax, which takes individual frames from a movie file and stacks them together, thereby removing a lot of noise caused by Earth’s turbulent atmosphere. Astronomers call this “seeing,” which is what makes the stars twinkle. He also showed us other image processing techniques in the GIMP, such as levels adjustment and color correcting that brought out details on the Sun.

sun

This image was taken on July 28, 2010, the day after Greg Piepol came to visit. The small dark Sunspot near the top of the disk is about the same size as the Earth!

This was most certainly closer to what we had seen in the telescope. But of course, as they say, practice makes perfect. Over the next few months I took pictures as often as I could. I learned the extreme importance of making fine adjustments to the filters inside the telescope to get exactly the right details. I learned the advantages of using a double-stacked filter on top of our telescope to help make the darker wispy absorptive lines in the solar atmosphere, called filaments, truly pop out.  I also learned the importance of careful processing to coax the most detail possible out of the raw data.  It is interesting to compare the final product to one of the raw, unprocessed images to see what a difference it makes.

This is a single frame from the raw video before the image is processed

This is a single frame from the raw video before the image is processed

sun

This final processed image of a Sunspot was taken on July 30, 2010

A large prominence on the Sun, taken on September 15, 2010

A large prominence on the Sun, taken on September 15, 2010

This mosaic of 2 images highlights a large Sunspot group, as well as a dark filament in the Sun’s chromosphere.

This mosaic of 2 images highlights a large Sunspot group, as well as a dark filament in the Sun’s chromosphere.

And so, the journey continues! The Sun is always changing, and there are always more techniques to be learned and perfected. If you get the chance, come see the Sun for yourself at the Public Observatory, which is open Thursday through Sunday, 11 am to 3pm for the month of October, weather permitting.  We are ordering an upgraded camera and some new software to better process these images, so be on the lookout for new images online!

Erin Braswell is an Astronomy Educator at the National Air and Space Museum.