NASA and university scientists release space sequencing data to the public


As part of the Biomolecule Sequencer project, our team just wrapped up the first of what we hope are many rounds of sequencing in space. For this first set of experiments, our goal was to determine whether the MinION and associated flow cells could survive launch to the International Space Station (ISS) and be loaded in microgravity conditions. We analyzed four samples in flight and performed four synchronous ground controls, and benchmarked the flight sequence data against the Illumina and PacBio platforms on the ground; all samples were prepared on the ground and stored on Earth or sent to the ISS frozen, where they were thawed just prior to loading. The big take home message is that there was no decrease in MinION performance between the flight and ground samples.

The data from our flight and ground sequencing runs, along with orthogonal data from other sequencing platforms, are now available in NASA’s GeneLab Database. We’ve also released a pre-print of our analysis of the data, and before we sent the sequencer to the ISS, we tested it aboard a parabolic flight.



Schematic of sequencing experiments performed on the International Space Station and on the ground. The image is from our bioRxiv preprint.

 Why on Earth would anyone want to sequence DNA in space?

Currently, we’re working on demonstrating that all of the steps necessary for sequencing can be performed on the ISS. The culmination of this would be and end-to-end, sample-to-sequence analysis of a sample collected aboard the ISS. Our ultimate goal is to have a functioning sequencing platform aboard the ISS. Some people we’ve talked to have been skeptical about the need for sequencing in space, and wonder whether this is just a gimmick. However, there are a number of applications for sequencing for space exploration:

  • Microbial monitoring. Microbes in the air, water and surfaces of the ISS are currently cultured to get microbial counts and samples are returned to Earth for identification (see here and here). Having in-flight identification capability would enable targeted remediation, and, as exploration moves beyond low-Earth orbit (i.e., towards Mars), it will not be feasible to return samples to Earth for identification.
  • Crew health. It has been observed that the human immune system becomes dysregulated in response to spaceflight, and that microbes can become more virulent. This means that even without new pathogens being introduced to the environment, it is possible that crew members could develop infections. One example of this is viral reactivation, which happens on Earth (i.e., getting shingles virus after you’ve had chicken pox). Sequencing in-flight would allow you diagnose the infectious agent and choose the appropriate antimicrobial treatment.
  • Microbiome studies. The ISS is a unique environment for microbes. It has been continuously inhabited by humans and microbes in constant microgravity with increased space radiation for over 15 years. These conditions place a different set of evolutionary pressures on microbial populations in the ISS, and within the humans that occupy it (see also here). Having a sequencer facility aboard the ISS would enable you to sample regions of interest on demand, and you could even track the accumulation of genetic mutations over time, without having to return samples to Earth coincident with the return of cargo re-supply ships.
  • Gene expression changes. Analysis of mutations at the DNA level allows you to see the permanent effects of spaceflight on organisms. Equally important is understanding how organisms themselves are responding to life on the ISS, and one powerful way of understanding how organisms are responding is by looking for changes in their gene expression (i.e., determining which genes are being upregulated and which are being downregulated). A particular challenge for measuring changes in gene expression is that they can occur on the timescale of minutes to hours, so bringing organisms back to Earth means that they may have re-acclimated. It is possible to extract the RNA and then return the samples to Earth, but there are risks with this method as well, because RNA is susceptible to degradation even when it is stored in a freezer. Having a sequencer aboard the ISS would allow you to perform these analyses in situ, without risk of re-acclimation or sample degradation during storage.
  • Search for extraterrestrial life elsewhere in the solar system. We know that the DNA/RNA/protein paradigm for life on Earth is capable of supporting life in environments ranging from below-freezing polar oceans to above-boiling hot springs, in the presence or absence of oxygen, using an incredible range of energy sources. This includes single-celled bacteria and archaea, to plants, and animals ranging from tardigrades to dinosaurs. At least in principle, then, the molecular basis for life as we know it is a reasonable starting point in the search for life elsewhere. Nanopore-based sensors that perform direct molecular analysis have been used to analyze RNA and even proteins, highlighting their potential to analyze a range of DNA-like molecules that could potentially support life.

Roger Harrington works on making a thin section in our @NASA_ARES Thin Section Lab

Roger Harrington, one of our @NASA_ARES Curation staff, is seen here as he works on polishing a sample in our Thin Section Lab.  To the left of Roger is a picture of Antarctic meteorite sample LAR 12011 and a petrographic thin section of this meteorite taken under polarized light. So what is a thin section?  A thin section is an extremely thin slice or sliver of a rock mounted onto a glass slide with epoxy.  They are prepared in order to help scientists investigate the textures and mineralogy of the rock using tools such as a polarizing petrographic microscope, scanning electron microscope, or an electron microprobe. This work is a part of petrology and helps to reveal the origin and evolution of the parent rock.  A thin section sample is approximately 30 micrometers (0.03 mm) thick – which is a little less than half the thickness of a human hair!  Petrographic thin section samples are available for check out by college and university professors.  For more information go to:



NASA Administrator discusses #StateofNASA. ARES honored to be part of current/future endeavors

In his “State of NASA” address, NASA Administrator Charles Bolden spoke about NASA’s scientific and technological achievements as well as cutting-edge future. He highlighted key work and advancements by the agency during the last few years and discussed many of the future goals NASA continues to work toward. This includes the exploration of Mars and elsewhere in our solar system and beyond, aeronautics research, development of technology to enable humans to explore deep space, and research aboard the International Space Station for the benefit of life on Earth and for astronauts on long duration space missions.

Staff @NASA_ARES are involved in many aspects of the work discussed – but one upcoming highlight worth mentioning is the DNA sequencing in space experiment led by @NASA_ARES Principal Investigator Aaron Burton and Deputy Project Manager/Project Engineer Kristen John (inset image). As mentioned by Administrator Bolden, in May, astronaut Kate Rubins will launch to the International Space Station (ISS) and plans to become the first person to perform DNA sequencing in space after she arrives at the ISS.

View a video of the “State of NASA” address at:


#ANSMET expedition complete! Team spent 5 weeks in #Antarctica searching for #meteorites!

#ANSMET 2015/2016 expedition complete! This amazing team, like so many others before them, spent five weeks in Antarctica (Miller Range) searching for meteorites in what most would consider bitter cold conditions. Think these team members would want to do this again next year?? Ask any one of them the next time you see them and see what they say! How about you – would you want to search for meteorites in Antarctica?

Now that this year’s mission is complete, the collected samples will be transported to our #NASA_Curation Meteorite Laboratory in Building 31 at the NASA Johnson Space Center in Houston, TX. We can’t wait to receive this year’s fabulous finds that through research and analysis, will help scientists better understand the history of our solar system! #RocksFromSpace

To read about this year’s 2015/16 Field Season, go to:

(Images courtesy of Case Western Reserve University and the 2015/16 Field team)