“Spiders” on Mars

“Spiders” on Mars

The South Pole of Mars is a strange and wonderful place. Many of its surface features are sculpted by the never-ending cycle of freezing and thawing of exposed carbon dioxide ice and subsurface water ice. These features includes “spiders” (radially organized channels carved in the surface), pitted sheets of carbon dioxide gas trapped below the thawing ice sheet, and by the freezing and thawing of water ice permafrost.

New location on Mars identified by the Planet Four: Terrains project shown to have spiders. Image Credit: NASA/JPL/University of Arizona

New location on Mars identified by the Planet Four: Terrains project shown to have spiders. Image Credit: NASA/JPL/University of Arizona

In late October Meg Schwamb, an assistant scientist at Gemini North, presented the project Planet Four:Terrains at the joint American Astronomical Society’s Division For Planetary Science (DPS) and European Planetary Science Congress (EPSC) meeting. Planet Four: Terrains is a citizen science project that enlists the general public to help identify these different surfaces in orbital images from the Context Camera (CTX) aboard Mars Reconnaissance Orbiter. These areas would then be imaged with the spacecraft’s High Resolution Imaging Science Experiment (HiRISE) camera, the highest resolution camera ever sent to Mars, in order to monitor the evolution of these areas to better understand how the carbon dioxide process compares to other areas previously studied on Mars.

A primary aim of Planet Four: Terrains was to identify areas with channels and pits (dubbed spiders). These channels indicate regions where, in the summer, carbon dioxide jets send dust and dirt aloft through cracks in the thawing carbon dioxide ice sheet – then, surface winds blow the material into the hundreds of thousands of dark fans observed from orbit. The project launched in June 2015, when the South Pole of Mars was in darkness, but starting in July 2016 sunlight returned to the South Pole. Once the Sun returned, Meg and her collaborators hoped that Planet Four: Terrains would find new areas of jet activity. The success of the project is revealed by the nearly 10,000 people who helped to identify over 20 new HiRISE targets. The public effectively commandeered the Mars Reconnaissance Orbiter in order to study in further detail these interesting regions with observations from the HiRISE camera over the current Spring and Summer seasons in the Southern Hemisphere of Mars.

A different kind of spider. These pits with radiating channels spotted on the South Pole of Mars have been dubbed 'spiders' due to their appearance. These channels are thought to be carved into the surface by the repeated cycle of deposition and sublimation of a seasonal carbon dioxide ice cap each Mars year (which is just under two Earth years). Image Credit: NASA/JPL/University of Arizona

A different kind of spider. These pits with radiating channels spotted on the South Pole of Mars have been dubbed ‘spiders’ due to their appearance. These channels are thought to be carved into the surface by the repeated cycle of deposition and sublimation of a seasonal carbon dioxide ice cap each Mars year (which is just under two Earth years). Image Credit: NASA/JPL/University of Arizona

The Planet Four: Terrains project isn’t finished yet. New images have been uploaded to the website covering new regions of the South Pole not part of the original search. These CTX images have never before been looked at by human eyes in such detail before. There is bound to be something interesting. You can read more about the project in the NASA press release and an article from Space.com.

Get to Know Gemini! – Chris Stark

Get to Know Gemini is a new series of blog posts aimed to highlight the different careers, backgrounds, and types of people contributing to Gemini Observatory and its science.

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Name:  Chris Stark

What is your current position and at which telescope?

Information Systems Engineer II & Gemini North ITS (Information Technology Services) Team Leader.

In four lines, explain what you do as part of the Gemini Observatory team?

My role with the observatory is two-part. On the technical side, I administer various aspects of our telescope production environment, including workstations, servers, data storage, and networking. My expertise is the Linux operating system. On the management side, I serve as the team leader for the Gemini North portion of our ITS team, helping to ensure that our observatory gets the IT support they need and that our team is working to meet our IT goals.

How long have you worked for Gemini?

Since late 2009

What drew you to this job?

I grew up with friends of our family that worked in astronomy, and during my time at UH as both a student and as an IT professional, I made a number of friends who are astronomers. I’ve also always had a bit of a guilty pleasure in watching astronomy-related television documentaries. One day while I was living on O‘ahu, my wife saw an ad in the paper for a Linux administrator, so I figured, why not give it a shot?

What is the best part of your job?

Easy question! I get to work with amazing people!

Where are you originally from/where did you grow up?

I was born on the West Coast of the US, but I grew up in North Kohala.

What skill do you think is most important to know for your job?

In IT one’s technical skills are an important foundation, but what is most important is the understanding that IT is all about serving *people* and ultimately helping one’s organization reach its goals with the right technology tools.

Why is astronomy important?

There are myriad reasons why astronomy is important, but ultimately what attracts me to this field is the spirit of exploration, the quest for discovery, and the desire to find our place in the universe.

What is your favorite movie?

Bladerunner

What is the latest book you have read?

“Strange Beautiful Music: A Musical Memoir” by Joe Satriani.

What three albums would you bring with you to a desert island?

1. Pink Floyd “The Dark Side Of The Moon”
2. Joe Satriani “Shockwave Supernova”
3. Jimi Hendrix “Electric Ladyland”

What is one hobby of yours?

I write and record instrumental guitar rock music.

Favorite beverage?

It’s really hard to beat an ice cold beer!

Check back next month to learn more about the staff that help Gemini to explore the Universe and share its wonders!

Journey Through the Universe 2017 Greatest Hits

Journey Through the Universe 2017 Greatest Hits!

On Wednesday, October 19th, Gemini held a workshop called “Journey Through the Universe 2017 Greatest Hits!” Five observatory STEM (Science, Technology, Engineering, and Mathematics) professionals with great K-12 classroom presentations demonstrated the activities they present to students during the week of Journey Through the Universe classroom visits in Hawai‘i.

The Zipline Ping Pong Ball Challenge

Gemini North Software Engineer Angelic Ebbers demonstrated an activity to spark students’ thinking about engineers and how they solve many types of problems. Angelic then split the audience into groups and gave each a set of materials and set up a small zipline. The group’s task was to design and build a mechanism that could carry a ping-pong ball from the top of a zipline to the bottom in four seconds. Some groups used all of their materials, including (but not limited to): paper cups, tongue depressors, rubber bands, washers, and pipe cleaners, while other groups produced minimalist designs, using as few materials as possible. By changing materials, and conditions, groups went through the engineering process by building, testing, and rebuilding their designs.

Working with Young Minds

Sherry Yeh, a Subaru Telescope astronomer shared tips and approaches on presenting astronomy to young (preschool and kindergarten) students. Sherry revealed her mantra, “less is more!” If the students walk away remembering one concept, such as “the Earth moves around the Sun,” then you have accomplished your goal. She also demonstrated ways to keep young students’ interest by singing songs and using kinesthetic activities.

Computer Science without Computers

Gemini Information Systems Engineer Jerry Brower demonstrated how to teach computer science without computers. His activities included topics like counting in binary, bubble sorting, how computers send and receive data, and how the internet keeps your data safe (or not). All of his activities transformed otherwise abstract computer science concepts into concrete, digestible, and interactive fun.

3-D Star Constellations

Gemini astronomer André-Nicholas Chené walked the group through the trials and errors he faced while creating 3-D models of recognizable constellations. While many students know how the stars look when they all appear on the same plane, like in the sky from Earth, but by making their own 3-dimensional models, showing distance, students can better appreciate depth in space. André-Nicolas also included how we modified existing instructions to make this activity easier and effective in a shorter period of time.

Light is All Around Us

Finally, Subaru Telescope Outreach Specialist Yuko Kakazu revealed how she presents the concept of light to younger students. Using models and props, she demonstrated the properties of light, different wavelengths/colors, light sources, and the how we have day and night due to the Earth’s rotation.

Celebrate the Large and Long Program!

Celebrate the Large and Long Program!

Celebrate the Large and Long Program! is a series of blog posts which showcase the high-impact science under the Large and Long Program of Gemini Observatory.  

What is the Large and Long Program?
The Large and Long Program (LLP) is one of five observing modes Gemini offers to users of our telescopes. These five modes categorize projects based on length and weather conditions required for the observations. Classically, Gemini accepts proposals on a six month basis and awarded recipients complete their observations within that given semester. Large and Long Programs, on the other hand, provide more flexibility for long term research and last anywhere from one to three years. This extended time frame promotes collaboration across communities and produces significant and high-impact science. Here, we ask current Large and Long Programs to share a little about their research and experience with Gemini Observatory.

Detecting and Characterizing Clouds in Exoplanet Atmospheres at Gemini North

 

Caption Credit: ESA / David Sing

Schematic showing how a transmission spectrum is observed when a planet passes between its host star and the observer. Credit: ESA / David Sing.

1. Principal Investigator: Name and Affiliation?
Catherine Huitson, University of Colorado Boulder

2. How would you describe your Large and Long Program?
Our long program is designed to study the composition of planetary atmospheres outside of the Solar system. We do this by observing with Gemini during ‘transits’, when a planet orbiting its star passes in between the star and the observer. At the time of transit, the planetary atmosphere acts like a filter for the starlight and the light that reaches us from the system contains an imprint of the planet’s atmosphere (its ‘transmission spectrum’). We can then compare the observed transmission spectrum with models and determine which atomic and molecular species are present in the atmosphere. Our program focuses specifically on searching for atmospheric species responsible for cloud formation.

3. Why is Gemini best suited for this research?
Gemini is particularly well-suited to our program because the transit events occur once every couple of weeks and we need to be able to point the telescope at the system during the transit. Most large telescopes require you to travel to the telescope to observe, which would be impractical for us. Gemini has the advantage of having a ‘queue’ mode, in which we can submit a list of dates and times, and which stars to look at, and the operators at Gemini will observe for us.

4. What has been the best part of your experience with the Large and Long Program?
These observations are very difficult because the signal from the planet is very small and can often be drowned out by other sources of noise, such as the Earth’s atmosphere, which can leave its own imprint on top of the signal that we are looking at. The majority of studies such as ours have therefore been conducted with space-based telescopes, and best part of our experience has been discovering that these observations are possible from the ground. It means that many more telescopes can now be used for such studies, increasing the number of planets observed.

Take a closer look at the work of Catherine Huitson and her group hereand visit us next month to Celebrate the Gemini Large and Long Program!  

Get to Know Gemini! – Nancy Levenson

Get to Know Gemini is a new series of blog posts aimed to highlight the different careers, backgrounds, and types of people contributing to Gemini Observatory and its science.

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Name: Nancy Levenson

What is your current position and at which telescope?

Deputy Director and Head of Science, based at Gemini South.

In four lines or less, explain what you do as part of the Gemini Observatory team?

A little of everything! As Deputy Director I partner with Markus and the Directorate in the overall leadership of Gemini, especially considering interactions with our governance bodies and external stakeholders and setting strategic directions. As Head of Science, I work to maximize the scientific productivity of the observatory, supporting both external users in the international community and Gemini staff.

How long have you worked for Gemini?

A little over 7 years, since mid-2009.

What drew you to this job?

I wanted to have a bigger impact on science, more than I could achieve in a regular academic role working with my own research group. I also happen to like the variety of tasks and interactions with lots of different people from around the world.

What is the best part of your job?

Solving problems. There are lots of situations where people run into an obstacle, and often by identifying the problem and being creative we can find a solution.

Where are you originally from/where did you grow up?

Tucson, Arizona.

What skill do you think is most important to know for your job?

How to work with people.

Why is astronomy important?

The opportunity for discovery, to understand the Universe around us.

In three lines, explain your PhD thesis.

I studied the mutual interactions of a supernova remnant (the remains from an exploded star) and the surrounding material, the interstellar medium.  I used a range of observations, from X-ray energies to the infrared, to reveal what the environment had been like earlier, and I showed how existing features like large clouds affect the subsequent motion of the supernova remnant’s shock wave.

What are your current research interests?

Now I mostly study active galactic nuclei (the supermassive black holes at the centers of galaxies that are actively taking on new material). I am interested in the material close to these central engines that hides their emission, and its relationship with star formation.

What is your favorite movie?

Raiders of the Lost Ark.

What is the latest book you have read?

The Paying Guests, by Sarah Waters.

What three albums would you bring with you to a desert island?

Back to Basics, Billy Bragg
Imperial Bedroom, Elvis Costello
Something classical – either Schubert string quartets or Marriage of Figaro, depending on my mood as I am packing.

What is one hobby of yours?

Travel. I have really enjoyed the opportunity to travel around Chile and South America while living here.

Favorite beverage?

Chilean wine.

Check back next month to learn more about the staff that help Gemini to explore the Universe and share its wonders!