Exhibit & Publication Update

I have "Geysers of Light" piece part of a group exhibition "The Cosmos" which will be hosted online as well as the New York Hall of Science from August 31st to March 2nd.
www.asci.org/artikel183.html
Press Release
The Cosmos was in The New York Times and they also mentioned my artwork
http://www.nytimes.com/2013/08/27/science/science-events-quirky-prizes-and-inspired-artworks.html?ref=science&_r=0

I also have an interview with Peripheral ARTeries magazine based out of the UK. I'm on the cover as well as from pg 20-27. My interview is mostly focused around my artwork I did for the Mars and Jupiter series.
http://issuu.com/artpress/docs/peripheral_arteries_art_review_-__a

Neptune Cloud Tank

I wasn't getting the look of Neptune with previous experiments that I felt was true to the visualization. I felt the photos were looking too dense and was very reminiscent of the Jupiter series. So I decided to copy an old hollywood visual fx known as the cloud tank. Descriptions on the process and history of it can be found off of these links:
http://rhizome.org/announce/opportunities/59735/view/
http://singlemindedmovieblog.blogspot.com/2010/04/old-school-effects-cloud-tank.html
http://www.youtube.com/watch?v=-qou5sDOO8k

Basic process was to create a layer of salt and fresh water, and use evaporated milk to create the clouds. the densities kept the milk in the middle, and I bounced light around the tank using white boards and blue gels. Special thanks to Jared Wright for helping me with this process.

Neptune Studio Revamp

Imagine If Planets Were As Close As The Moon
http://media.talkingpointsmemo.com/slideshow/if-planets-were-as-close-to-earth-as-moon
Neat idea.

Currently I'm rebuilding my studio set up so I can get more even lighting. This includes building a table strong enough to hold my tank, and setting up a white box out of foam board (or science fair display boards) to help bounce light to get a more even illumination.  In the spare time I've been reading Drifting on Alien Winds which just came in a few days ago and managed to catch an interesting documentary on the weather channel about other planet's weather.

This week I'm submitting Jupiter and Mars series to IEEE VIS 2013 (July 15 http://visap2013.sista.arizona.edu/) and Science Inspires Art: The Cosmos (July 21 http://www.asci.org/artikel1187.html)

Neptune Update

I was able to get in contact with an artist and scientist at JPL, and I was able to get some feedback as well as some great resources. One resources was the book Drifting on Alien winds, fortunately the Neptune chapter was available online so I could use it in my research right now, but I did order the book. This book has been the best resources I've come across, the author is an artist that specializes in space illustrations, so his book is very descriptive on the atmospheres across different planets and moons.

I've put off shooting for two reasons, one I was waiting on a timer to come in for a better dslr (the t3i's had too much noise to my liking, so I was waiting on the 5d timer to come in) and second was to get feedback/advice from a scientist that studied the planet. I haven't had much luck getting in contact with a scientist, I imagine summer is difficult to get a hold of people. But I did design an experiment, and I will be doing Neptunes first test shoot Monday, July 1st. Right now I'm looking two methods. First is a tank full of water with a layer of oil at the top, and dropping condensed milk through that way there's more of a cloud effect. Second method is to suspend cotton using fishing line off of mesh in a water tank to get a cloud effect. That will give me more control.

In addition I've been submitting to contest, galleries, proposals etc. I did hear back from one that I did get selected for, which is Peripheral ARTeries magazine which is an art review of new artists.

Initial Neptune Research

After conducting initial research, the main question I have is what would the color of the surface (or rather inside) of Neptune would look like. I'm unsure whether the blue would carry on through to the interior of the planet, since the methane gas clouds is responsible for the blue, supposedly there's ice and an unknown substance as well that could change the color.
 

Neptune

Neptune is a gas giant planet, so it doesn’t have a solid surface. The blue-green ball that we see in photographs of Neptune is really the top of the clouds on Neptune. If you could dive down beneath the surface of Neptune, you would find an interior with increasing temperatures and pressures right down to the rocky core at the center.

So, we’re clear that the surface of Neptune isn’t solid. There’s no standing on Neptune. That said, the “surface of Neptune” that we see is one the most active and dynamic places in the Solar System. For some reason, that astronomers haven’t figured out, the interior of Neptune is unusually hot. Even though Neptune is much further from the Sun than Uranus and receives 40% less sunlight, its surface temperature is about the same. In fact, Neptune gives off 2.6 times more energy than it takes in from the Sun. Even without the Sun, Neptune glows.

This high amount of interior heat matched with the coldness of space creates a huge temperature difference. And this sets the winds blasting around Neptune. Maximum wind speeds on Jupiter can be more than 500 km/hour. That’s twice the speed of the strongest hurricanes on Earth. But that’s nothing compared to Neptune. Astronomers have calculated winds blasting across the surface of Neptune at 2,100 km/hour.

When NASA’s Voyager 2 spacecraft visited Neptune in 1989, it also discovered the planet’s Great Dark Spot, a huge storm like Jupiter’s Great Red Spot. But unlike Jupiter, the Dark Spot didn’t seem to be very stable, and had already disappeared by 1994 when the Hubble Space Telescope tried to locate it.

Deep down inside Neptune, the planet might have a solid surface. At the very core of Neptune is thought to be a region of rock with roughly the mass of the Earth. But temperatures at this region would be thousands of degrees; hot enough to melt rock. And the pressure from the weight of all the atmosphere would be crushing. There would be no way to walk around on the “surface of Neptune”.

Source: NASA
http://www.universetoday.com/22070/surface-of-neptune/

The interior is presumed to contain a rocky core with an icy mantle topped by a deep layer of liquid hydrogen. Voyager 2's instruments detected a complex magnetic field. Like Uranus, the field is tipped with respect to the axis of rotation and offset from the center (the tilt is 50 degrees for Neptune, compared with 60 degrees for Uranus). However, the field is somewhat weaker than for Uranus.
As for Uranus, it is speculated that this magnetic field my originate in a conducting shell not far below the clouds, rather than deep in the interior as for Jupiter or the Earth. In that case, the conducting material would not be metallic hydrogen, as for Jupiter, or iron and nickel, as for the Earth. As noted earlier for Uranus, a mixture of water, methane, and ammonia under the right pressure could be responsible.

http://csep10.phys.utk.edu/astr161/lect/neptune/surface.html

Neptune's blue appearance comes from the layer of methane gas that sits above the clouds. Methane absorbs red light, so only the bluish colors show up when viewing the planet.


Much is still unknown about Neptune, because the strong pressure makes it impossible for us to land on the planet. It is thought that there is an ocean of really hot water on Neptune's surface. The planet's pressure makes it impossible for the water to boil away.

The only spacecraft to visit Neptune was the Voyager 2 in 1989. Voyager confirmed that Neptune's atmosphere was very cold and very windy. In fact, the surface of Neptune reaches 200 degrees below zero! Regardless of the frigid temperatures, Neptune's core remains very warm. Neptune actually gives off more heat than it receives from the Sun.

Yahoo Answers

Chemistry

• According to the Smithsonian Museum, hydrogen, helium and methane dominate Neptune's ambiguous surface. At near-surface conditions, these chemicals exist as gases. Frozen methane forms clouds that are visible from space, just like frozen water does on Earth. The Great Dark Spot storm system is a distinguishing surface feature on Neptune. The storm was a hurricane-like feature similar to Jupiter's Great Red Spot. The storm's dark feature offers a glimpse into the deeper layers of Neptune's atmosphere. As one travels down into the giant planet, pressure and internal heat transform the hydrogen and methane gases into a compressed fluid.

  http://www.ehow.com/about_6325426_surface-neptune-like_.html#ixzz2WWvMmDfe

Planets get their color from what they are made of -- their composition. Both Uranus and Neptune get their blue-green color from methane, but Neptune is a more vivid and brighter blue, which points to Neptune having an unknown component.

Neptune does not have a solid surface, but its atmosphere (made up mostly of hydrogen, helium and methane) extends to great depths, gradually merging into water and other melted ices over a heavier, approximately Earth-size solid core.

Neptune's atmosphere extends to great depths, gradually merging into water and other melted ices over a heavier, approximately Earth-size solid core. Neptune's blue color is the result of methane in the atmosphere. Uranus' blue-green color is also the result of atmospheric methane, but Neptune is a more vivid, brighter blue, so there must be an unknown component that causes the more intense color.

Summer 2013 Schedule Plan of Action

Jupiter Series: Final Images