The team behind the Exoplanet Explorers project has just published a Research Note of the American Astronomical Society announcing the discovery of 28 new exoplanet candidates uncovered by Zooniverse volunteers taking part in the project.
Nine of these candidates are most likely rocky planets, with the rest being gaseous. The sizes of these potential exoplanets range from two thirds the size of Earth to twice the size of Neptune!
This post is by Adina Feinstein. Adina is a graduate student at the University of Chicago. Her work focuses on detecting and characterizing exoplanets. Adina became involved with the Exoplanet Explorers project through her mentor, Joshua Schlieder, at NASA Goddard through their summer research program.
Let me tell you about the newly discovered system – K2-288 – uncovered by volunteers on Exoplanet Explorers.
K2-288 has two low-mass M dwarf stars: a primary (K2-288A) which is roughly half the size of the Sun and a secondary (K2-288B) which is roughly one-third the size of the Sun. The capital lettering denotes a star in the planet-naming world. Already this system is shaping up to be pretty cool. The one planet in this system, K2-288Bb, hosts the smaller, secondary star. K2-288Bb orbits on a 31.3 day period, which isn’t very long compared to Earth, but this period places the planet in the habitable zone of its host star. The habitable zone is defined as the region where liquid water could exist on the planet’s surface. K2-288Bb has an equilibrium temperature -47°C, colder than the equilibrium temperature of Earth. It is approximately 1.9 times the radius of Earth, which places it in a region of planet radius space where we believe planets transition to volatile-rich sub-Neptunes, rather than being potentially habitable super-Earth. Planets of this size are rare, with only about a handful known to-date.
The story of the discovery of this system is an interesting one. When two of the reaction wheels on the Kepler spacecraft failed, the mission team re-oriented the spacecraft to allow observations to continue to happen. The re-orientation caused slight variations in the shape of the telescope and temperature of the instruments on board. As a consequence, the beginning of each observing campaign experienced extreme systematic errors and initially, when searching for exoplanet transits, we “threw out” or ignored the first days of observing. Then, when we were searching the data by-eye for new planet candidates, we came across this system and only saw 2 transits. In order for follow-up observations to proceed, we need a minimum of 3 transits, so we put this system on the back-burner. The light curve (the amount of light we see from a star over time) with the transits is shown below.
Later, we learned how to model and correct for the systematic errors at the beginning of each observing run and re-processed all of the data. Instead of searching it all by-eye again, as we had done initially, we outsourced it to Exoplanet Explorers and citizen scientists, who identified this system with three transit signals. The volunteers started a discussion thread about this planet because given initial stellar parameters, this planet would be around the same size and temperature as Earth. This caught our attention. As it turns out, there was an additional transit at the beginning of the observing run that we missed when we threw out this data! Makennah Bristow, a fellow intern of mine at NASA Goddard, identified the system again independently. With now three transits and a relatively long orbital period of 31.3 days, we pushed to begin the observational follow-up needed to confirm this planet was real.
First, we obtained spectra, or a unique chemical fingerprint of the star. This allowed us to place better constraints on the parameters of the star, such as mass, radius, temperature, and brightness. While obtaining spectra from the Keck Observatory, we noticed a potential companion star. We conducted adaptive optics observations to see if the companion was bound to the star or a background source. Most stars in the Milky Way are born in pairs, so it was not too surprising that this system was no different. After identifying a fainter companion, we made extra sure the signal was due to a real planet and not the companion; we convinced ourselves this was the case.
Finally, we had to determine which star the planet was orbiting. We obtained an additional transit using the Spitzer spacecraft. Using both the Kepler and Spitzer transits, we derived planet parameters for both when the planet orbits the primary and the secondary. The planet radius derived from both light curves was most consistent when the host star was the secondary. Additionally, we derived the stellar density from the observed planet transit and this better correlated to the smaller secondary star. To round it all off, we calculated the probability of the signal being a false positive (i.e. not a planet signal) when the planet orbits the secondary and it resulted in a false positive probability of roughly 10e-9, which indicates it most likely is a real signal.
The role of citizen scientists in this discovery was critical, which is why some of the key Zooniverse volunteers are included as co-authors on this publication. K2-288 was observed in K2 Campaign 4, which ran from April to September back in 2015. We scientists initially missed this system and it’s likely that even though we learned how to better model and remove spacecraft systematics, it would have taken years for us to go back into older data and find this system. Citizen scientists have shown us that even though there is so much new data coming out, especially with the launch of the Transiting Exoplanet Survey Satellite, the older data is still a treasure trove of new discoveries. Thank you to all of the Exoplanet volunteers who made this discovery possible and continue your great work!
The paper written by the team is available here. It should be open to all very shortly.
This is the first of two guest posts from the Exoplanet Explorers research team announcing two new planets discovered by their Zooniverse volunteers. This post was written by Jessie Christiansen.
Hello citizen scientists! We are here at the 233rd meeting of the American Astronomical Society, the biggest astronomy meeting in the US of the year (around 3000 astronomers, depending on how many attendees are ultimately affected by the government shutdown). I’m excited to share that on Monday morning, we are making a couple of new exoplanet announcements as a result of your work here on Zooniverse, using the Exoplanet Explorers project!
Last year at the same meeting, we announced the discovery of K2-138. This was a system of five small planets around a K star (an orange dwarf star). The planets all have very short orbital periods (from 2.5 to 12.8 days! Recall that in our solar system the shortest period planet is Mercury, with a period of ~88 days) that form an unbroken chain of near-resonances. These resonances offer tantalizing clues as to how this system formed, a question we are still trying to answer for exoplanet systems in general. The resonances also beg the question – how far could the chain continue? This was the longest unbroken chain of near first-order resonances which had been found (by anyone, let alone citizen scientists!).
At the time, we had hints of a sixth planet in the system. In the original data analysed by citizen scientists, there were two anomalous events that could not be accounted for by the five known planets – events that must have been caused by at least one, if not more, additional planets. If they were both due to a single additional planet, then we could predict when the next event caused by that planet would happen – and we did. We were awarded time on the NASA Spitzer Space Telescope at the predicted time, and BOOM. There it was. A third event, shown below, confirming that the two previous events were indeed caused by the same planet, a planet for which we now knew the size and period.
So, without further ado, I’d like to introduce K2-138 g! It is a planet just a little bit smaller than Neptune (which means it is slightly larger than the other five planets in the system, which are all between the size of Earth and Neptune). It has a period of about 42 days, which means it’s pretty warm (400 degrees K) and therefore not habitable. Also, very interestingly, it is not on the resonant chain – it’s significantly further out than the next planet in the chain would be. In fact, it’s far enough out that there is a noticeable gap – a gap that is big enough to hide more planets on the chain. If these planets exist, they don’t seem to be transiting, but that doesn’t mean they couldn’t be detected in other ways, including by measuring the effect of their presence on the other planets that do transit. The planet is being published in a forthcoming paper that will be led by Dr Kevin Hardegree-Ullman, a postdoctoral research fellow at Caltech/IPAC.
In the meantime, astronomers are still studying the previously identified planets, in particular to try to measure their masses. Having tightly packed systems that are near resonance like K2-138 provides a fantastic test-bed for examining all sorts of planet formation and migration theories, so we are excited to see what will come from this amazing system discovered by citizen scientists on Zooniverse in years to come!
We are also announcing a second new exoplanet system discovered by Exoplanet Explorers, but I will let Adina Feinstein, the lead author of that paper, introduce you to that exciting discovery.
We recently uncovered a couple of bugs in the Zooniverse code which meant that the wrong question text may have been shown to some volunteers on Zooniverse projects while they were classifying. They were caught and a fix was released the same day on 29th November 2018.
The bugs only affected some projects with multiple live workflows from 6th-12th and 20th-29th November.
One of the bugs was difficult to recreate and relied on a complex timing of events, therefore we think it was rare and probably did not affect a significant fraction of classifications, so it hopefully will not have caused major issues with the general consensus on the data. However, it is not possible for us to say exactly which classifications were affected in the timeframe the bug was active.
We have apologised to the relevant science teams for the issues this may cause with their data analysis, but we would also like to extend our apologies to all volunteers who have taken part in these projects during the time the bugs were in effect. It is of the utmost importance to us that no effort is wasted on our projects and when something like this happens it is taken very seriously by the Zooniverse team. Since we discovered these bugs we worked tirelessly to fix them, and we have taken actions to make sure nothing like this will happen in the future.
We hope that you accept our most sincere apologies and continue the amazing work you do on the Zooniverse. If you have any questions please don’t hesitate to contact us at firstname.lastname@example.org.
Hi all, I am Coleman Krawczyk and for the past year I have been working on tools to help Zooniverse research teams work with their data exports. The current version of the code (v1.3.0) supports data aggregation for nearly all the project builder task types, and support will be added for the remaining task types in the coming months.
What does this code do?
This code provides tools to allow research teams to process and aggregate classifications made on their project, or in other words, this code calculates the consensus answer for a given subject based on the volunteer classifications.
The code is written in python, but it can be run completely using three command line scripts (no python knowledge needed) and a project’s data exports.
The first script is the uses a project’s workflow data export to auto-configure what extractors and reducers (see below) should be run for each task in the workflow. This produces a series of `yaml` configuration files with reasonable default values selected.
Next the extraction script takes the classification data export and flattens it into a series of `csv` files, one for each unique task type, that only contain the data needed for the reduction process. Although the code tries its best to produce completely “flat” data tables, this is not always possible, so more complex tasks (e.g. drawing tasks) have structured data for some columns.
The final script takes the results of the data extraction and combine them into a single consensus result for each subject and each task (e.g. vote counts, clustered shapes, etc…). For more complex tasks (e.g. drawing tasks) the reducer’s configuration file accepts parameters to help tune the aggregation algorithms to best work with the data at hand.
At the moment this code is provided in its “offline” form, but we testing ways for this aggregation to be run “live” on a Zooniverse project. When that system is finished a research team will be able to enter their configuration parameters directly in the project builder, a server will run the aggregation code, and the extracted or reduced `csv` files will be made available for download.
Occasionally we run studies in collaboration with external researchers in order to better understand our community and improve our platform. These can involve methods such as A/B splits, where we show a slightly different version of the site to one group of volunteers and measure how it affects their participation, e.g. does it influence how many classifications they make or their likelihood to return to the project for subsequent sessions?
One example of such a study was the messaging experiment we ran on Galaxy Zoo. We worked with researchers from Ben Gurion University and Microsoft research to test if the specific content and timing of messages presented in the classification interface could help alleviate the issue of volunteers disengaging from the project. You can read more about that experiment and its results in this Galaxy Zoo blog post https://blog.galaxyzoo.org/2018/07/12/galaxy-zoo-messaging-experiment-results/.
As the Zooniverse has different teams based at different institutions in the UK and the USA, the procedures for ethics approval differ depending on who is leading the study. After recent discussions with staff at the University of Oxford ethics board, to check our procedure was up to date, our Oxford-based team will be changing the way in which we gain approval for, and report the completion of these types of studies. All future study designs which feature Oxford staff taking part in the analysis will be submitted to CUREC, something we’ve been doing for the last few years. From now on, once the data gathering stage of the study has been run we will provide all volunteers involved with a debrief message.
The debrief will explain to our volunteers that they have been involved in a study, along with providing information about the exact set-up of the study and what the research goals were. The most significant change is that, before the data analysis is conducted, we will contact all volunteers involved in the study allow a period of time for them to state that they would like to withdraw their consent to the use of their data. We will then remove all data associated with any volunteer who would not like to be involved before the data is analysed and the findings are presented. The debrief will also contain contact details for the researchers in the event of any concerns and complaints. You can see an example of such a debrief in our original post about the Galaxy Zoo messaging experiment here https://blog.galaxyzoo.org/2015/08/10/messaging-test/.
As always, our primary focus is the research being enabled by our volunteer community on our individual projects. We run experiments like these in order to better understand how to create a more efficient and productive platform that benefits both our volunteers and the researchers we support. All clicks that are made by our volunteers are used in the science outcomes from our projects no matter whether they are part of an A/B split experiment or not. We still strive never to waste any volunteer time or effort.
We thank you for all that you do, and for helping us learn how to build a better Zooniverse.
Irma has brought widespread devastation to many islands in the Caribbean over the last few days, and now Hurricane Jose is a growing threat in the same region.
By analysing images of the stricken areas captured by ESA’s Sentinel-2 satellites, Zooniverse volunteers can provide invaluable assistance to rescue workers. Rescue Global are a UK-based disaster risk reduction and response charity who are deploying a team to the Caribbean and will use the information you provide to help them assess the situation on the ground.
Breaking news… Zooniverse volunteers on Exoplanet Explorers have discovered a new 4-planet system!
Congratulations to all* who directly classified the light curves for this system, bringing it to the attention of the research team. And an enormous *thank you* to the 14,000+ volunteers who provided over 2 million classifications in just three days to make this discovery possible. This is equivalent to 3.4 years of full time effort. I *heart* people-powered research! It’s also amazing how quickly we were able to get these data to the eyes of the public — the Kepler Space Satellite observed this star between December 15 and March 4, 2017. Data arrived on Earth on March 7th and Zooniverse volunteers classified it April 3-5, 2017. I *heart* Zooniverse.
ExoplanetExplorers.org was the featured project for our inaugural ABC Australia Stargazing Live 3-day, prime-time TV event, which just ended yesterday and through which this discovery was made. Over the years, we’ve partnered with the BBC as part of their Stargazing Live event in the UK. On night 1, Chris Lintott, our intrepid leader, invites the million+ viewers to participate in that year’s featured Zooniverse project, on night 2 he highlights interesting potential results coming through the pipeline, and on night 3, if science nods in our favor, he has the pleasure of announcing exciting discoveries you all, our volunteers, have made (for example, last year’s pulsar discovery and the supernova discovery from a couple years back).
This year we partnered with both the UK’s BBC and Australia’s ABC TV networks to run two Stargazing Live series in two weeks. We’re exhausted and exhilarated from the experience! We can imagine you all are as well (hats off to one of our volunteers who provided over 15,000 classifications in the first two days)!
Stargazing Live epitomizes many of our favorite aspects of being a member of the Zooniverse team – it’s a huge rush, filled with the highs and lows of keeping a site up when thousands of people are suddenly providing ~7000 classifications a minute at peak. We’re so proud of our web development team and their amazing effort; their smart solutions, quick thinking, and teamwork. The best part is that we collectively get to experience the joy, wonder, and discovery of the process of science right alongside the researchers. Each year the research teams leading each project have what is likely among the most inspiring (and intense) 3-days of their careers, carrying out the detective work of following up each potential discovery at breakneck speed.
Brad Tucker and his team leading PlanetNineSearch.org featured in the BBC Stargazing Live event this year checked and rechecked dozens of Planet 9 candidates orbital parameters and against known object catalogs, making sure no stone was left unturned. We were bolstered throughout with re-discoveries of known objects, including many known asteroids and Chiron, a minor planet in the outer Solar System, orbiting the Sun between Saturn and Uranus.
Even though Planet 9 hasn’t been discovered yet, it’s huge progress for that field of research to have completed a thorough search through this Skymapper dataset, which allows us to probe out to certain distances and sizes of objects across a huge swath of the sky. Stay tuned for progress at planetninesearch.org and through the related BackyardWorlds.org project, searching a different parameter space for Planet 9 in WISE data.
Also, and very importantly, the BBC Stargazing Live shows gave the world an essential new member of the Twitterverse:
The Exoplanet Explorers team, led by Ian Crossfield, Jessie Christiansen, Geert Barentsen, Tom Barclay, and more were also up through much of each night of the event this week, churning through the results. Because the Kepler Space Telescope K2 dataset is so rich, there were dozens of potential candidates to triple check in just 3 days. Not only did our volunteers discover the 4-planet system shown above, but 90 new and true candidate exoplanets! That’s truly an amazing start to a project.
Once you all, our amazing community, have classified all the images in this project and the related PlanetHunters.org, the researchers will be able to measure the occurrence rates of different types of planets orbiting different types of stars. They’ll use this information to answer questions like — Are small planets (like Venus) more common than big ones (like Saturn)? Are short-period planets (like Mercury) more common than those on long orbits (like Mars)? Do planets more commonly occur around stars like the Sun, or around the more numerous, cooler, smaller “red dwarfs”?
There’s also so much to learn about the 4-planet system itself. It’s particularly interesting because it’s such a compact system (all orbits are well within Mercury’s distance to our Sun) of potentially rocky planets. If these characteristics hold true, we expect they will put planet formation theories to the test.
A fun part of our effort for the show was to create visualizations for this newly discovered system. Simone, one of our developers, used http://codepen.io/anon/pen/RpOYRw to create the simulation shown above. We welcome all to try their hand using this tool or others to create their favorite visualization of the system. Do post your effort in the comments below. To set you on the right path, here are our best estimates for the system so far:
The star is in the constellation of Aquarius (see if can get the WWT), with ra, dec = 23:15:47.77, -10:50:58.91.
Host star (V=12): 0.8 Rsol, 0.9 Msol. Late G or early K.
We predict there may be more planets further out, with similar resonances as the inner planets. The predictions for outer planets are 20d, 30.7d, 47d, etc. (assuming Per_x = 3.56 * 1.538^x.). Planet number 11 would be ~264d, planet 12 ~405d.
There are 73 other previously discovered exoplanet systems with 4 or more planets known.
In 2372 years, on July 9, 4388AD, all four planets will transit at the same time.
If you’re standing on planet e, the nearest planet would appear bigger than the full moon on the sky. Apparent size of other planets while standing on e = 10 arcmin, 16 arcmin, 32 arcmin.
If you’re on planet e, the star barely appears to rotate: you see the same side of it for many “years,” because the star rotates just as quickly as planet “e” goes around it.
This post wouldn’t be complete without a thank you to Edward Gomez for following up candidates with the Los Cumbres Observatory Robotic Telescope Network. Not only is LCO a great research tool, but it provides amazing access to telescopes and quality curricular materials for students around the world.
*And a special thanks to the following volunteers who correctly identified at least one the planets in the newly discovered 4-planet system:
Alan Patricio Zetina Floresmarhx
Anastasios D. Papanastasiou
We’re testing out a new feature of our interface, which means if you’re classifying images on Comet Hunters you may see occasional pop-up messages like the one pictured above.
The messages are designed to give you more information about the project. If you do not want to see them, you have the option to opt-out of seeing any future messages. Just click the link at the bottom of the pop-up.
You can have a look at this new feature by contributing some classifications today at www.comethunters.org.
We’re cleaning up our email list to make sure that we do not email anyone who does not want to hear from us. You will have got an email last week asking you if you want to stay subscribed. If you did not click the link in that email, then you will have received one today saying you have been unsubscribed from our main mailing list. Don’t worry! If you still want to receive notifications from us regarding things like new projects, please go to www.zooniverse.org/settings/email and make sure you’re subscribed to general Zooniverse email updates.
NOTE: This has not affected emails you get from individual Zooniverse projects.
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