Juno's first in-orbit picture of Jupiter and Galilean Moons is awesome

NASA's Juno spacecraft, now in orbit of Jupiter, has taken its first in-orbit image of the Jovian system. This incredible image was taken by the instrument JunoCam from ~2.7 million miles away from Jupiter.

Here's the information about the image from NASA (taken from the page where you can download the full-size image):

"This color view from NASA's Juno spacecraft is made from some of the first images taken by JunoCam after the spacecraft entered orbit around Jupiter on July 5th (UTC). The view shows that JunoCam survived its first pass through Jupiter's extreme radiation environment, and is ready to collect images of the giant planet as Juno begins its mission.

The image was taken on July 10, 2016 at 5:30 UTC, when the spacecraft was 2.7 million miles (4.3 million kilometers) from Jupiter on the outbound leg of its initial 53.5-day capture orbit. The image shows atmospheric features on Jupiter, including the Great Red Spot, and three of Jupiter's four largest moons.

JunoCam will continue to image Jupiter during Juno's capture orbits. The first high-resolution images of the planet will be taken on August 27 when the Juno spacecraft makes its next close pass to Jupiter.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems, Denver, built the spacecraft. JPL is a division of the California Institute of Technology in Pasadena."

This picture shows the relative size and structure of Juno and offers information about the instruments. You can find more info on the NASA page for Juno.

Jupiter, King of Worlds

Jupiter is the king of the planets of our solar system. Jupiter is almost 26,000 times more massive than the Moon and 318 times more massive than Earth! Even though Jupiter is still less than one tenth of one percent as massive as the Sun, the king of our worlds is over 2.5 times greater in mass than the rest of all of the planets in the solar system combined (unless there really is a Planet IX out there, which would only change that number a little bit; a quick back-of-the-envelope calculation tells me that if Planet IX is there and is 10 times the mass of the Earth, then Jupiter would be about 2.3 times more massive than all the other planets combined)!

Jupiter is a behemoth of planetary mass in our solar system. Here you can see the relative masses of the 8 planets. (image from Das steinerne Herz on Wikipedia)

Jupiter was one of the five planets beyond Earth known by many ancient peoples. Jupiter's apparent point of light in the night's sky was associated with the god Marduk by the ancient Babylonians, while ancient Chinese beliefs personified Jupiter as the Fu Star (Fuxing), association the bright light of Jupiter with prosperity. It was from the ancient Romans that Jupiter gained the name we use for it. Jupiter in Roman mythology is the king of the gods, just as Zeus was the king of the gods in Greek mythology. We even came to name one of the days of our weeks after Jupiter (though in English, our word for that day (Thursday) has derived from the Germanic mythologies and the god Thor).

It was Galileo's discovery of four of the moons of Jupiter in 1610 and his writing of them that nearly caused the Catholic Church to murder Galileo (the idea that there could be moons orbiting other planets was certainly considered blasphemy against the church at that time). Below you can see a page from the Sidereus Nuncius ("Starry Messenger"; Galileo's 1610 book on his astronomical observations), where Galileo drew Jupiter and the moons he had discovered:

Although Galileo's discoveries of Jupiter's moons propelled astronomy and our understanding of the universe forward, it was Giovanni Cassini who first drew pictures of the features on Jupiter that he could observe with his telescope. For instance, below are some images from Cassini where he first shows what we believe was the discovery of the Great Red Spot (or, at least, discovery of a spot which may have preceded the Great Red Spot by over a century).

Perhaps one of the coolest of the earliest drawings of Jupiter came in 1880, and can be found in the collections of astronomer and artist E.L. Trouvelot. His drawing of Jupiter was created during an observation on November 1st of 1880, and clearly shows the Great Red Spot:

These early observations and drawings must have sent people's minds racing with wonderment at what those features on the king of worlds could be. However, once we started incorporating photographic imaging with observational astronomy and, especially, started sending spacecraft to explore the other worlds we started constraining what it was we were seeing on Jupiter (while also raising lots of more questions!). 

The Pioneer 10 spacecraft was the first extension of humanity to fly by Jupiter back in 1973. Here's one of the images taken during that encounter with the giant world. Pioneer 10 was the first spacecraft to measure the radiation and magnetic fields surrounding Jupiter. It was also the first to take images of the moons of Jupiter up-close. Pioneer 10 passed within 81,000 miles of the cloudtops of Jupiter on it's flyby over 40 years ago.

Jupiter has since had several other spacecraft go zooming by, most of which at least took pictures if not full-on collecting data and targeting Jupiter and its moons for observation; for instance, check out this table I stole from Wikipedia on spacecraft that have flown by along with the dates of closest approach and the minimum distance from Jupiter at that time:

-----Spacecraft-----	Closest -----Approach------	-----Distance-----
Pioneer 10	December 3, 1973	130,000 km
Pioneer 11	December 4, 1974	34,000 km
Voyager 1	March 5, 1979	349,000 km
Voyager 2	July 9, 1979	570,000 km
Ulysses	February 8, 1992	408,894 km
	February 4, 2004	120,000,000 km
Cassini	December 30, 2000	10,000,000 km
New Horizons	February 28, 2007	2,304,535 km

The only spacecraft so far to be sent into orbit of Jupiter was the Galileo Spacecraft, which operated in the Jovian system for over 8 years (from its arrival in December of 1995 until we crashed it into Jupiter (something we like to call "de-orbiting") in September of 2003). Galileo was used to study Jupiter's atmosphere and rings and to image and study the volcanoes on Io. Galileo discovered that Ganymede has its own, very strong magnetic field and really gave us most of the best data from which we have concluded that there is likely a deep subsurface ocean on Europa. The Galileo spacecraft really unlocked Jupiter and set the grounds for future spacecraft to visit that giant world.

An artist's concept of the Galileo spacecraft at Jupiter, with Io's volcanoes erupting nearby

Of the upcoming missions to Jupiter, one of them is actually going to get there very soon. The Juno spacecraft (see image to the left for a digital image of the spacecraft) is a NASA mission to Jupiter which was launched in August of 2011 and will arrive at Jupiter on July 4th of this year. Juno, named after the wife of Jupiter who was able to see through his clouds, will study Jupiter's composition, magnetic and gravitational fields, and will study the various processes within the Jovian atmosphere.

Following Juno, there are two missions in the works for studying the icy moons of Jupiter. JUICE (the Jupiter Icy Moon Explorer) is an ESA mission slated for launch in 2022. JUICE is designed to study primarily Ganymede and Callisto, though it should also fly by Europa a couple of times as well. A NASA mission set for launch on the early 2020s (likely 2022, as of now) is also in the works. The mission is currently called the Europa Multiple-Flyby Mission, though that name will surely change when the mission is more fully developed. This mission will focus on studying Europa. It will tell us about the surface processes and composition of Europa, will tell us a bit about the internal geology and composition of this moon, and, most importantly for astrobiology, will seek to determine the existence of Europa's ocean and determine what it can about the composition and possible surface-interactions of this ocean. 

Though JUICE and the Europa Multiple-Flyby Mission will target the icy moons of Jupiter, they will teach us a lot about the Jovian system in general (like how Jupiter's magnetic field and the chaotic whipping of particles through that field effect the moons of Jupiter). Taken along with Juno, the next couple of decades of research on Jupiter should be highly revealing, telling us a lot about the king of the planets but also helping us to uncover new mysteries and new questions about this behemoth in our solar system. 

In closing out this post, here is a quote about Jupiter, the god, from Ovid:

"Jupiter, from on high, smiles at the perjuries of lovers."

When it comes to the "perjuries of lovers" on Earth, Jupiter the planet, just as Jupiter the god, most certainly has no interest in our shortcomings. Though there is a beautiful history to consider in astrology, and Jupiter most certainly has played a prominent role there, the real test of time for Jupiter has revealed this king of our planets to be a massive and active monster of nature, though also beautiful in its presentation of itself to the universe.

Jupiter Drawing, from Kelvin Ma at Wikipedia

NASA and University Researchers Discuss the Search for Life in the Solar System & Beyond at AbSciCon 2015

Image taken from the NASA Astrobiology Roadmap

Last week, at the Astrobiology Science Conference (AbSciCon) in Chicago, NASA convened a press briefing to feature some of the lead figures within the realm of astrobiology and to promote discussion of what we're doing right now in astrobiology as well as what will be coming next. You can find the video of that briefing at the bottom of this post!

The panel for the briefing consisted of the following four people:

-John Grunsfeld, former astronaut and now Associate Administrator for Science at NASA Headquarters

-Alexis Templeton, Principal Investigator for the NASA Astrobiology Institute's Rock-Powered Life team

-Britney Schmidt, Principal Investigator for the NASA-funded project Sub-Ice Marine and Planetary Analog Ecosystems (SIM

-Vikki Meadows, Principal Investigator at the University of Washington's Virtual Planetary Laboratory

Left to right: Vikki Meeadows, Britney Scmidt, and Alexis Templeton. Image posted to Twitter by NASA NExSS

I've never met John Grunsfeld in person, but I love the energy and enthusiasm he presents when he talks. I have met Vikki Meadows, Britney Schmidt, and Alexis Templeton. They are impressive researchers and wonderful people. 

Britney and Alexis are especially kick-ass women. Britney has quickly climbed to fame within the sciences as a lead expert on the icy worlds of our solar system. She's travelled to Antarctica to study icy analog environments and a paper that she authored in the journal Nature in 2011 rocked icy-worlds research with the conclusion that the chaos regions on Europa may be caused by shallow subsurface fluids. 

I was abundantly overjoyed to see Alexis Templeton on the panel. She's one of the most renowned researchers in the realm of geobiology, she knows more about the connections between microorganisms and the variety of environments present on the Earth than anyone else I've ever met, and she is my graduate research advisor! Here's a picture of Alexis and I taken by John Spear while we were working at our field site, Borup Fiord Pass, in the Canadian High Arctic during the summer of 2014:

Alexis has been involved in many research projects that seek to characterize the myriad ways that microorganisms interrelate with their environments. Research that has been conducted in her lab over the years has included looking at the microbial alteration of basalt on the seafloor, characterizing metal oxidation by microbes in the depths of the Earth, and working on our NASA-funded project to understand microbial sulfur cycling and the formation of sulfur biosignatures at an Arctic analog to icy extraterrestrial environments. 

Most recently, Alexis has become the Principle Investigator of a team that goes by the handle Rock-Powered Life (RPL). This team, funded by the NASA Astrobiology Institute, seeks to characterize the pathways through which water and rock can react to form the simplest ingredients for living processes on Earth. They're also considering what these reactions mean for the habitability of extraterrestrial environments, such as those in the subsurface oceans of Europa and Enceladus. 

The NASA press briefing last week went very well. All of the members of the panel gave fantastic introductions to what we're doing right now in astrobiology to better understand life on Earth and the potential for life in our solar system and beyond! I highly recommend checking out the briefing video below:

My research talk for AbSciCon 2015

I'm traveling off to Chicago tomorrow morning to attend the 2015 Astrobiology Science Conference (AbSciCon). AbSciCon is a scientific meeting for researchers, educators, and science communicators who work in the diverse realm of astrobiology, the scientific pursuit to understand the origins, evolution, and radiation of life in the universe. This is my first big science conference, so I'm pretty excited. I'll be giving a research talk this coming Tuesday, the 16th of June, to share a little bit of my graduate research. My talk will be part of a conference session titled "Habitability of Extraterrestrial Analog Environments" and it will allow me to talk about my current work on samples that I collected last summer at Borup Fiord Pass in the Canadian High Arctic. If you're interested, here's a little introduction to what I'll be talking about on Tuesday:

My field site, Borup Fiord Pass, is a valley in the Canadian High Arctic where there resides a very special glacier. Near the toe of this glacier (the glacier's edge) you can find large accumulations of yellow elemental sulfur on top of the ice. These deposits of sulfur form from sulfide-rich springs that emerge on the glacier or just at its edge. The sulfide carried by the springs is derived from the reduction (electronation) of sulfate by microorganisms that thrive in the subsurface. The yellow sulfur that appears at the surface may be partly formed through the activity of microbial life and also may feed microorganisms that are capable of oxidizing (de-electronating) elemental sulfur. This unique sulfur-dominated system may serve as an ideal analogue for icy environments in our solar system and beyond, especially those where subsurface fluids may emerge at the surface of an icy system (like maybe on Jupiter's moon Europa!).

I had the wonderful opportunity to visit this remarkable site for two weeks during the summer of 2014. Here is an image taken by John Spear, of the Colorado School of Mines, while flying over the glacier in a helicopter:

The image shows the region at the toe of the glacier where yellow sulfur staining was visible. The large sulfur covered area in this shot is about 100x100 square meters (about the size of a couple of American football fields). Interestingly, during our time at the site, we did not observe an active spring. Instead, what we found was that a very thick structure of ice had formed at the edge of the glacier. This icing is not only covered in sulfur, but is loaded with sulfur in various states (sulfide, elemental sulfur, and sulfate). We took samples from various regions on the sulfur icing, on the glacier, and in the melt water streams that ran down the valley. Below is a ternary diagram showing some of the data I've now analyzed for major cations in the samples as compared to some samples from previous years:

What this figure is showing is that there is a range of cation chemistry that can be observed in samples collected at the site. There are data here for active springs from previous years, sulfur deposits from 2009 and 2014, as well as melt water and stream water from around the site from 2000 and 2014. Most importantly, these data show that the sulfur icing is really similar to the sulfide-rich springs, which is part of why we reason that the spring was flowing and then that fluid was frozen in place to make the sulfur icing.

Sulfur bubbles on a melt pool on a sulfur icing

One of the coolest things about the sulfur icing during our time at Borup Fiord Pass was the active thawing and refreezing of the ice each day within melt pools on top of the icing. Hydrogen sulfide gas that had been locked within the sulfur icing would gurgle its way up through these melt pools, forming bubbles on the surface of the fluid. In several places these bubbles became encrusted in yellow sulfur and formed sulfur bubbles, like those shown to the left here.

I was so intrigued by these sulfur bubbles that I had to know more about them. I took some of the material and ran x-ray diffraction (XRD) on it. XRD allows us to determine what minerals or other crystallized material is present within a sample. The XRD data revealed something very interesting. The data show elemental sulfur present in three different forms, known as allotropes. Usually, in nature, sulfur is most stable as eight-membered rings of sulfur atoms that are packed in a certain arrangement that is known as α-S₈. (a.k.a. alpha-cyclooctasulfur). However, there are two other mineral forms of cyclooctasulfur that can also form in nature. These are known as the beta and gamma forms. β-S₈ is a form of cyclooctasulfur that
forms when α-S₈ is heated above ~96 C. It's extremely bizarre to find this form of sulfur in a sample from Borup Fiord Pass, where the fluid forming the sulfur icing likely never reached a temperature that high. Likewise, the gamma form of cyclooctasulfur, γ-S₈ (which is also known as the mineral Rosickyite), usually only forms in high temperature environments. That said, Susanne Douglas and Heixong Yang published an article in the journal Geology in 2002 where they reported finding Rosickyite within an endoevaporitic microbial film. They hypothesized that processes of microbial sulfur metabolism that formed elemental sulfur favored the formation of γ-S₈ over α-S₈. If that's not exciting enough, Damnhait Gleeson, who was once a member of our lab at the University of Colorado Boulder, also previously reported finding rosickyite in a microbial sample, this time it was within a sample of sulfur collected at Borup Fiord Pass in 2009 by Katherine Wright (also a former member of our lab). Since rosickyite was previously detected at our site, it wasn't a huge surprise, but it's definitely exciting. 

During my talk at AbSciCon, I'll be showing some images of the sulfur bubble material that I recently collected using an electron microscope. There's some really interesting structures to be found within these samples. I'm now hot on the trail of figuring out if I'm seeing the representation of gamma and beta cyclooctasulfur or perhaps something else all together. I don't know yet if these unique forms of sulfur and strange things that I'm seeing under the electron microscope are indicative of the biological processing of sulfur or if they've formed through an abiotic process at Borup Fiord Pass (which would also be very interesting), but it's nice to find new and exciting things when doing research.

There's a bit more that I'll be presenting at my talk at AbSciCon, however the talk is only supposed to be 10 minutes in length (which is a very short time for a talk). Fortunately, for the stuff that I don't get to cover in my talk, my colleague Chris Trivedi of the Colorado School of Mines will be presenting a poster with information about his work on our samples from Borup Fiord Pass. Hopefully, if people find our work interesting and want to know more following my talk, they'll then have a chance to check out Chris' poster as well.

This is me saluting the sulfur stained glacier and the valley that holds it

I'm definitely looking forward to the experiences I'll be having in the coming week at AbSciCon 2015. There's going to be a lot of great science to hear about and to talk about. I'm going to serve as a judge for student posters at the conference and I'll also be serving as a Meeting Mentor, spending half of one conference day with a high school student shadowing me at the conference. On top of all of this great stuff, on Monday evening there will be the final preliminary heat of the 3rd season of the NASA Famelab science communication competition. In case you don't know, I won the first preliminary heat of the competition in August of 2014, when I shared a story about my first day in the field at Borup Fiord Pass. I'm looking forward to watching a new line-up of scientists and science communicators as they compete in this final heat for Famelab. I have a feeling there are going to be some awesome talks and a lot of great stories.

I'll be adding more posts in the coming weeks that detail my experiences at AbSciCon, so look forward to those. I think I'll wrap this post up right now by sharing the video of the talk I gave when I competed in NASA Famelab in 2014. Here's looking forward to great science and good times at AbSciCon 2015!

Borup Fiord Pass: video from the 2011 expedition to this unique Arctic environment

Science on the ice at Borup Fiord Pass in summer, 2014 (Photo: John Spear)

Borup Fiord Pass is a truly unique and intriguing field site. The deposition of elemental sulfur and microbial processes at the surface of a glacier at Borup Fiord Pass may provide clues we need in our search for life on icy worlds like Jupiter's moon Europa, and strange circular structures in the valley near the glacier may be the remnants of past springs which could inform our future exploration of Mars. I got to travel to Borup Fiord Pass in the summer of 2014 and it was an incredible experience.

My current graduate research is focused on characterizing the materials that form at the surface of this Arctic glacier. Much of that material is rich with sulfur in various chemical forms. I'm now using various instruments to perform my characterizations of the sulfur-rich materials from the site. For instance, I get to use a particle accelerator to conduct x-ray spectroscopy to look at the sulfur!

In 2011, Bob Pappalardo, of the Jet Propulsion Laboratory, and Steve Grasby, of the Geological Survey of Canada, made the trek north to visit Borup Fiord Pass. They took some samples that we've now been using to better understand the geochemical and biological processes that have occurred at the glacier. They also recorded a lot of video. Some of that video was recently edited into B-roll by JPL. The video shows Bob and Steve collecting sulfur on the ice beside a sulfide-rich spring. Take a look and see what you think about the sulfur that forms on the ice at this strange Arctic site:

B-roll: Astrobiology Field Research on Ellesmere Island, Canadian Arctic from JPLraw on Vimeo.

For more information about this strange glacial environment in the Arctic, check out an earlier post on this blog titled "Borup Fiord Pass: An introduction to how an Arctic glacier may aid in our search for life on Jupiter's moon Europa". You can also find articles about Borup Fiord Pass science that have been posted by sites like Space.com and Popular Science.

We'll soon be putting together videos that show our work during the more recent field expedition in 2014. Stay tuned to this blog for those videos and for more of the science and awesomeness of Borup Fiord Pass!

Borup Fiord Pass: An introduction to how an Arctic glacier may aid in our search for life on Jupiter's moon Europa

Standing on the glacier at Borup Fiord Pass and looking down-valley (Photo: John Spear)

Borup Fiord Pass. I've said that name so many times that it almost feels like the name of a good friend. Last summer I had the opportunity to visit this remote place on the planet, far north of the northernmost cities of North America. The experience was incredible and something that I will cherish forever. My research team and I spent two weeks at Borup Fiord Pass, and when we left we brought back the samples that I'm now studying to better understand the relationships between living organisms and the chemical element sulfur.

Borup Fiord Pass is a valley in the Canadian High Arctic where yellow staining of the surface of a glacier is caused by large deposits of sulfur in its elemental form. This site gives us the opportunity to study the chemical and biological cycling of sulfur through various forms in a unique icy environment. Borup Fiord Pass also gives us a chance to study some of the biological processes we might expect to find on icy worlds with subsurface oceans, such as Jupiter's moon Europa, if life ever came to exist there.  

Europa, one of the most intriguing places in the solar system (NASA)

Watch out where those huskies go...

Borup Fiord Pass is located on Ellesmere Island, very near the North Pole, at the northern extreme of the Canadian territory of Nunavut. To get an idea of where this is, if you hold up a globe and point the North Pole directly toward yourself, then Borup Fiord Pass will be within the first 10 degrees of latitude from the center:

Looking at the world with the North Pole at the center

Benoit Beauchamp, of the University of Calgary, was the first person to see the yellow staining on the glacier at Borup.  At least, that's what I've been told. There are military flights that pass overhead quite often. I wouldn't be too surprised if one of the pilots of a military plane was flying low and happened to see some large yellow patch on the white of the ice. Maybe that pilot thought, "huh, that's interesting." Or maybe some explorer decades ago chanced upon a glacier with a yellow icing that smelled of hydrogen sulfide, but the same explorer didn't see need to note the occurrence. 

We really don't know how long this yellow staining has been happening, though we know it's been active since Benoit first noticed it during a helicopter fly-over in 1988. Once Steve Grasby, a geochemist with the Geological Survey of Canada and my collaborator, learned from Benoit about the yellow coloration on top of the glacier, he knew something special was happening and had to check it out.  

Steve Grasby sampling a sulfur deposit on one his earliest trips to Borup Fiord Pass

Steve Grasby and his earliest collaborators on the Borup Fiord Pass project published the results of their initial findings after multiple visits to the site in an article published in the journal Astrobiology in 2003. In this article they detailed some of the basic characteristics of the yellow sulfur materials and the processes causing their existence on the glacier.  

The sulfur is deposited by springs that emerge on the glacier and which carry high levels of sulfide, the most electron-rich (reduced) form of sulfur, with a formal oxidation state of -2. In considering the chemical composition of the spring fluids and the isotopes of sulfur at the site, Steve Grasby and his colleagues determined that the sulfide is likely derived from sedimentary sulfate deep in the subsurface. Sulfate is the most electron-poor (oxidized) form of sulfur (since the sulfur atom in a sulfate molecule shares it's electrons with four oxygen atoms, giving the sulfur a formal oxidation state of +6). The transition from sulfate to sulfide implies that there must be microorganisms somewhere below the glacier which are using sulfate reduction (making sulfur more electron-rich) for their metabolisms.  

After sulfur in groundwater has been processed by organisms in the subsurface, it then flows up through the glacier or along its base and emerges as springs at the surface. Many years, the springs are still quite active when researchers have arrived to investigate. Last summer, in 2014, there was no apparent spring activity, but rather an earlier spring had deposited a large sheet of sulfide-rich ice. 

Where this icing dropped over the sides of a small canyon, we called the deposit "Sulfur Falls" (see image below). Near the glacier, in the middle of the icing, was a large circular structure that we called "The Blister". This structure may be the remnant of a sulfur-rich plume which had burst its way out from the subsurface and could possibly have formed the icing.

This is me kneeling on a pile of glacial till in front of the toe of the glacier at Borup Fiord Pass.  The yellow coloration of the ice behind me is caused by the deposition of elemental sulfur at this site. (Photo: John Spear)

The sulfide-rich water and ice that forms at the surface then provides the material for the oxidation of sulfide (stripping of electrons from sulfur) to form elemental sulfur (sulfur with a formal oxidation state of 0 and which only forms bonds with other sulfur atoms).  Elemental sulfur forms one of the most beautiful minerals on Earth:

Elemental sulfur: the mineral is yellow in solid state,
turns blood red when melted, and burns a bright blue (Image: Volty)

There are a lot of scientifically intriguing questions that remain with regard to Borup Fiord Pass. For one thing, cells of a certain type of microorganism that our lab has isolated from the field site have the strange capability of forming unique biominerals when grown in gradient cultures of sulfide and oxygen. This was first reported in a paper by Damnhait Gleeson and our colleagues in the journal Geobiology in 2011. We've learned a good deal about these biominerals since that time. Specifically, Julie Cosmidis, a postdoc in our lab, is now working on characterizing these unique structures. I'm also now in the process of looking at the samples from the field to see if any of these unique structures can be found there.

Another interesting question comes from the presence of the yellow sulfur itself.  Given the chemistry of the fluid at the ice surface and the presence of oxygen from the atmosphere, the sulfur should be oxidized the whole way to sulfate, yet the yellow staining persists throughout the summer (at least until the snow begins to fall at this site). Much of my work is now focused on quantifying the different chemical forms of sulfur at Borup Fiord Pass. Expect more posts from me in the near future that details some of the various types of instruments and methods that I'm using in this endeavor.

Using the Field Microsensor Multimeter from Unisense to measure sulfide (Image: Alexis Templeton)

The Connection to Europa

There's been a lot of buzz in the press and social media lately regarding Europa. Europa is one of the four Galilean Moons of Jupiter and is definitely one of the more intriguing places in our solar system for astrobiologists. Europa bears a deep subsurface ocean, and that ocean might have been in recent communication with the surface. If life ever came about in the ocean of Europa, we might have the potential to find signs of such life near the surface of that moon. We're now working on the next spacecraft that will explore Europa.  

Europa's awesome surface textures and deep subsurface ocean are enough to scientifically justify a mission to that moon, but the possibility for life detection in materials at Europa have bolstered scientific and public support together and now it looks like we might soon see a Europa mission on its way to Jupiter. For us to better understand what signs of life we may find on Europa, it's a good idea to study life in icy environments here on Earth. Places like Lake Vostok and Blood Falls in Antarctica and Borup Fiord Pass, my field site, in the Arctic can aide in this type of research. Indeed, Borup Fiord Pass has gotten its fair share of press as a Europa analogue site. Here are articles from Wired, Space.com, Popular Science, and CBC News that report on the importance of Borup Fiord Pass in our search for life on Europa.

With Lake Vostok and other ice-covered Antarctic lakes, as well as some recent research on a drilling project to study the organisms living under the Ross Ice Shelf, we can explore ecosystems in lakes and oceans deep below icy environments. Research in these areas may highlight the techniques we'll need if we ever want to get through the ice on Europa and explore the ocean below.  However, that ice is very thick (probably at least 1 km but maybe more than 10 km in thickness), and it will take us a long time to build a spacecraft with the right technology to get down there. In the meantime, there's a lot that we have to learn about Europa's ocean and the possibility for signs of life to be found in the near-surface of the ice through an orbiter mission and our first lander mission. That's where our work at Borup Fiord Pass comes in. By studying the connection of subsurface microbial processes to the chemical and biology processes that occur where fluids make their way through the ice and to the surface, we might be able to highlight some key signs of life to look for near the Europan surface.  

I was recently at NASA's Ames Research Center for the Workshop on the Potential for Finding Life in a Europa Plume. There are a lot of us who are now trying to figure out what the best instrumentation is to send to Europa to capture signs of life.  You might have read recently about the potential discovery of water plumes coming out of Europa.  Although some of us are highly skeptical of the data in that study, if there are water plumes at Europa, they may offer even more insight into the processes that are occurring in the subsurface ocean.  Even if the plumes are not there, we still have a lot to learn with the mission that we'll be sending to Europa. If we can get data about the chemistry of the surface or, better yet, the near subsurface, then we may be able to find signs of life from the subsurface ocean.  This of course requires that fluid from the ocean has made its way through the ice and to the near surface. There's a lot of "ifs" involved, but that's part of the fun of science.

In the coming months, I'll be writing up posts that detail the importance of sulfur for astrobiology as well as the importance of Borup Fiord Pass in our exploration of Europa (and other worlds). These are important topics for me, especially since they'll be included in my Ph.D. dissertation.  Before I leave you, though, here's a sweet infographic from NASA regarding Europa, one of the most intriguing worlds in our solar system: