Exoplanets and Travelling

+ Data Science and Public Engagement

A short introduction of myself

Hi! I am an astrophysicist hunting for new exoplanets. Since 2018, I am a Torres Fellow at the Massachusetts Institute of Technology (MIT), working on small exoplanets, small stars and stellar flares with the Transiting Exoplanet Survey Satellite (TESS) team. Whenever I am not searching for new worlds, I enjoy travelling, the outdoors (scuba diving, rock climbing and hiking), and exploring our own Earth.

Expertise: Exoplanets, Stellar Flares, Cool Stars, Habitability

Skills: Bayesian Statistics, Machine Learning, Time Series Analysis

My PhD was obtained at the University of Cambridge, UK, where I worked in Professor Didier Queloz's group at the Exoplanet Research Centre. My research was focused on how we can distinguish between real exoplanets and stuff that looks like exoplanets, but is not (false positives). I worked with the Next Generation Transit Survey, a ground-based array of telescopes on the hunt for Neptune-sized exoplanets.

For my Master’s Thesis, I did something completely different: research in the biophysics lab of Professor George Shubeita at the University of Austin at Texas (Hook 'em Horns). I developed a mathematical model furthering our understanding of animal models of genetic diseases like Alzheimer's and Fragile X.

My physics undergraduate education was at the University of Würzburg, where I studied AGN mega-masers in the multi-wavelength group of Professor Matthias Kadler.

(Yellowstone. Credit: M. Günther)


Credit: Tansu Daylan

Oct 19, My PhD supervisor, Prof. Didier Queloz, just won the Nobel Price in Physics!

Sep 19, Secured two grants to design and conduct two experiments on a zero gravity flight. One will be related to prebiotic chemistry in artificial gravity. Stay tuned!

Jul 19, Our TOI-270 system is published and got world-wide media attention, as we hope to understand the "missing link" between rocky Earths and puffy sub-Neptunes

Jan 19, Our first TESS study of stellar flares and how they could impact the origin of life on exoplanets

Sep 18, Started as a Torres Fellow at MIT, working closely with the TESS science team

Aug 18, Volunteered with Love The Oceans in Mozambique: marine biology field work, scuba diving, and work with the local schools

July 18, Graduated from the University of Cambridge with a PhD in (astro-)physics

Apr 18, Launch of TESS on the SpaceX Falcon 9 from Cape Canaveral

Oct 17, Meeting Nobel laureate Rainer Weiss on the day of his award

Sep 16, Advancing my Spanish for a month at Universidad de La Habana, Cuba with an A.J. Pressland Fund scholarship

Feb 16, Joined Prince Philip, Duke of Edinburgh, and Ambassador Ammon for the Kurt Hahn Dinner in the German Embassy in London

Apr 15, My first visit to Paranal: working on NGTS, and exploring the worlds driest desert, Atacama, and its unbelievable night sky

Jul 15, Discussing my research with Prince Andrew, Duke of York, during his visit to Cambridge's Astrophysics Groups

Oct 14, Started my PhD at the University of Cambridge


How do stellar flares impact habitability?

Why care about flares? Because flares can impact habitability - they may erode exoplanets' atmospheres, but might also trigger the genesis of life. And all of this is especially important around M-dwarfs! To model flares, we use our public allesfitter code (Günther&Daylan, in prep.). It not only models exoplanets&binaries and red noise (with GPs), but also robustly selects the appropriate model for potentially complex flares via Bayesian evidence. Using Nested Sampling, we can compute the Bayes factors of diffferent models - pure noise, 1 flare, 2 flares, and so on. So what do we find? From the sample of ~25,000 TESS objects we find ~760 flaring stars, ~630 of which are M-dwarfs. Especially the mid M-dwarfs are `flary'. And one of the coolest (no pun intended) things: TESS explores so many bright early to late M-dwarfs! Of course, thanks to Kepler/K2/NGTS/MEarth/EVRYSCOPE and others we already learned some things about their flares - but TESS truly opens up new avenues here. Moreover, we find that fast rotating M-dwarfs are the most likely to flare, solidifying previous findings by other studies. And one of my personal favorites: the large amplitude flare on an M4.5 dwarf, raising the stellar brightness by a factor of 15.7! This goliath is even preceeded by a series of `warm-up' flares. Finally, we link all this flaring to prebiotic chemistry, coronal mass ejections, and ozone depletion. This figure contains a lot of info, and a detailed explanation is beyond this tweet - so if all this raised your interest, have a look at the paper :)

See Günther, M.N. et al., 2019a

Small exoplanets around small stars: TOI-270

The TOI-270 system is a true Disneyland for us exoplanet scientists. With three small exoplanets orbiting a red dwarf star, TOI-270 is a prime example of the type of system the Transiting Exoplanet Survey Satellite (TESS) set out to discover, and will soon provide a lot of puzzle pieces we are currently missing. The star TOI-270, only 40% the size and mass of our Sun, has three planets in orbit: one slightly bigger than Earth and likely rocky, and two double the size of Earth and probably of a similar composition as Neptune - rocky cores covered by a thick gas atmosphere. Being one of the nearest and brightest such systems, TOI-270 is a true Disneyland for exoplanet science. It is relatively easy to observe and offers something for every research area, from formation and dynamics to atmosphere and habitability studies. The unique, open spirit of the TESS community made this discovery possible, and various follow-up efforts are already in progress. So stay tuned for more exciting TOI-270 news in the future. Go TESS!

Read more in our Nature Astronomy Blog, the New York Times, or The Economist.

See Günther, M.N. et al., 2019b,

Other research projects

Click here to read more about some of my other studies:

(Artist illustration of TOI-270. Credit: Sci-News.com)


6 first author

25 in total



Google Scholar

Peer-reviewed, lead author

  • Günther, M.N. et al., 2019b, A Super-Earth and two sub-Neptunes transiting the bright, nearby, and quiet M-dwarf TOI-270, Nature Astronomy, 409
  • Günther, M.N. et al., 2019a, Stellar Flares from the First Tess Data Release: Exploring a New Sample of M-dwarfs, in press (arXiv:1901.00443)
  • Günther, M.N. et al., 2018, Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system, MNRAS, 478 (4): 4720–4737
  • Günther, M.N. et al., 2017b, Centroid vetting of transiting planet candidates from the Next Generation Transit Survey, MNRAS, 472 (1): 295-307
  • Günther, M.N. et al., 2017a, A New Yield Simulator for Transiting Planets and False Positives: Application to the Next Generation Transit Survey, MNRAS, 465 (3): 3379-3389
  • Günther, M.N. et al., 2016, Quantifying and predicting Drosophila larvae crawling phenotypes, Nature Scientific Reports, 6: 27972

Peer-reviewed, co-lead author

Peer-reviewed, co-author


  • Günther, M.N. & Daylan, T., 2019, allesfitter: Flexible star and exoplanet inference from photometry and radial velocity, Astrophysics Source Code Library (ascl:1903.003)

PhD Thesis

(NGTS in Paranal, Chile. Credit: G. Lambert)


The Transiting Exoplanet Survey Satellite (TESS)

The Transiting Exoplanet Survey Satellite (TESS) is set to discover thousands of new exoplanets. Launched in April 2018, TESS now monitors millions of stars for temporary drops in brightness, which are caused by planetary transits. It will identify planets ranging from Earth-sized to gas giants, around a wide range of stellar types and orbital distances - and maybe even Earth 2.0.

The TESS discovery of Pi Men c (some call it the first TESS planet): video, cnet, sciencenews, dailystar, sciencealert

The TESS discover of HD 21749 b and c (TESS' first Earth-sized planet): New York Times

The Next Generation Transit Survey (NGTS)

The Next Generation Transit Survey (NGTS) is an exoplanet hunter based in Paranal, Chile. With its 12 fully robotized 20 cm telescopes, NGTS covers a total field of view of almost 100 sq. deg. on the sky at once. The main goal of NGTS is to find transiting Neptunes that will be suitable for RV follow-up and mass measurements using current and future instruments such as HARPS and ESPRESSO.

(TESS. Credit: NASA's Goddard Space Flight Center)


& more


'Ask/Tell a Scientist' at the Science Festival in Cambridge, MA, USA: Enagaged in open discussions with the public about any scientific topic, from astronomy to biology.


Volunteered for a month with marine biologists in Mozambique, studying and teaching about marine conservation - sprinkled with some astrophysics.


Hosted a public evening on exoplanets in Burgkunstadt Germany, and gave a visiting tutorial for the high school's astrophysics course. Featured in the local German news (web1, web2) and on the school's website (web1, web2).

Tutored high-performing high-school students in physics and astronomy over multiple months, as part of 'The Brilliant Club' - a charitable programme focussed on low-participation neighbourhoods (web).


Bringing exoplanet science to 8-12 year old pupils in Barton Road and Milton Road Primary Schools. Thanks to the Cambridge Science Festival Roadshow for this fantastic programme (leaflet).


Initiated a public evening on exoplanets hosted at my former high school, Gymnasium Burgkunstadt, in Germany. The evening was featured in articles in the Obermain Tagblatt (web) and on the school's website (web).

(Outreach event, Germany. Credit: OT/Adriane Lochner )


Department of Physics,

and Kavli Institute for Astrophysics and Space Research

Massachusetts Institute of Technology

Cambridge, MA 02139, USA

Email: maxgue [at] mit.edu

Twitter: @M_N_Guenther

(Sunset at Paranal, Chile. Credit: M. Günther)