It’s been a busy spring for the RECON Network. Following a highly productive science team meeting in Boulder City, Nevada in early March, the network has collected data for two campaigns: one involving Centaur 16FH13 on April 23 and the second involving Centaur 98BU48 on May 1 (both UT dates). The May 1 campaign was particularly challenging for our RECON teams due to twilight sky conditions during this early evening event. Only teams to the south of Reno were able to participate in this campaign given sky conditions. Meanwhile, RECON leadership from Boulder Colorado deployed three telescopes in northern New Mexico, where the sun had set an hour earlier, to support the campaign.
Below are some photos taken on May 1 from Mills Canyon Rim Campground by RECON Co-PI John Keller. The “occulting” moth shown below was attracted to the visible and thermal IR given off by the laptop screen!
Congratulations to all of you that have been a part of RECON. It’s been six years since we began the pilot project and four years since the start of the full project. We’ve all learned a lot together and it’s been an amazing project throughout. We are known in the scientific community throughout the world for our work on the Kuiper Belt.
While we’ve been hard at work, the rest of our colleagues have also been probing the boundaries of knowledge of the outer solar system. Rings around tiny Centaur objects! Maybe a Planet X out there (or maybe not). Binary objects remain an important component of these objects and it’s widely recognized that RECON is the perfect tool to expand that study.
The Gaia mission from the European Space Agency has delivered on its promise to pin down where a huge number of stars are. As I’ve talked about many times, this is essential to the long-term success and productivity of RECON and any other occultation-based study of objects in our solar system. It took a couple of extra years to get to this point but we are now starting to see the benefits enabled by Gaia. In the early days of the project we were limited a bit by having to work with a much less accurate star catalog and also much poorer knowledge of the positions of the TNOs. The explosion of occultation opportunities is now upon us.
Within the project we have continued to work on measuring where candidate TNOs are to help increase the number of good events to observe. That work continues but we are now working closely with the PanStarrs survey in Hawaii. Their dataset is an amazing resource that has, in the past few months, provided thousands of observations of more than a hundred objects. With the telescopes we have available ourselves, this contribution would take us 300 nights of observing on giant telescopes to equal.
A good example of this is our campaign observation for RECON of the TNO 2014TA86. This object was discovered in 2014 by PanStarrs and the recent effort located nearly 10 years of data that had already been collected on this object by PanStarrs but not yet processed. As a result we know where this object is with much more precision that is usual for something discovered in 2014. Without the support from PanStarrs, we wouldn’t even know this object existed and now we are poised to make critical measurements of its size and position. If it turns out to be binary (which is quite likely), we’ll be adding more to our understanding of these distant worlds. Note that the shorter than usual notification of the impending campaign was a result of this recent data dump from PanStarrs coming in. This event popped up in our scans, and it was just too good to pass up, so we made an exception to our normal procedure of providing a month’s notice.
The context of our efforts is greatly expanded with the historic event to come on Jan 1, 2019. New Horizons will have a close flyby of (486958) 2014MU69, a TNO that I discovered by in 2014. It’s a neighbor of this month’s campaign target and whatever we learn from New Horizons will provide a broader understanding of our RECON target. What’s even more exciting is that our observations will provide a broader understanding of the New Horizons data as well.
I’m very excited to see what we will learn from New Horizons. I’ve been unbelievably busy this year and last organizing and chasing occultations by MU69. Many of the lessons learned with RECON were a key to the success of those occultation expeditions. I sent 25 teams of astronomers out on three separate occasions. South Africa, Argentina, Senegal, and Colombia were all visited by these dedicated teams of astronomers, braving clouds, storms, high winds, mosquitoes, insane urban traffic, and more. It was an exhausting, yet fulfilling effort, and the team work was truly amazing. All of you that have been a part of RECON can take pride in knowing that you helped make these other efforts a success.
Now it’s our turn. Early in the morning, on Friday, October 12, we will have a shot at our own historic observation of this distant TNO. What will we find? Should we let a minor inconvenience like having to get up in the middle of the night, during the week, to get in our way of learning more about our solar system? I’ve said all along in this project that astronomy isn’t always at a convenient time. We’ll continue the fine tradition of making a special effort to learn more about the universe around us. I’ll be observing from home along with all of you to add my own efforts but you are all truly the stars of the project. I should also warn you that we’re looking at a lot of very nice opportunities in the coming six months during our peak season. It will be RECON like never before. How exciting!
Our campaign tonight, August 14th, involves Pluto, a dwarf planet with an atmosphere. The nature of the experiment is a bit different from what RECON is mainly designed for.
Rodrigo Leiva, a RECON Postdoctoral researcher at Southwest Research Institute has explained the science of this Occultation:
For an opaque object, a positive detection will look like a sudden dimming of the star, followed by a sudden back-to-normal brightness. If you put an atmosphere around an object, then part of the light is refracted away from us by the atmosphere (because its refraction index is different than 1), and some light is also refracted toward us.
If an observer is close to the central line, the atmosphere acts as a magnifying glass and the refracted light is concentrated. This is called the central flash. For a brief time, the star will look even brighter than when not occulted, i.e. you see a ‘flash’. The central flash allows us to study the lower atmosphere of Pluto, a few kilometers above the surface.
Is Pluto’s atmosphere finally collapsing? Did you know that the atmosphere has been expanding and this could be the first time we detect a change in that trend?
Our role is to give a correct interpretation of the central flash. It is necessary to know where the central line is very precisely – down to single kilometers. This is possible if we have a good sampling for the whole atmosphere. And we have the right network for that, RECON! According to the prediction, we could sample a big portion of the north half of the occultation, which will give a good constraint for the atmosphere modeling and also in determining if the atmosphere is finally contracting.
It is possible that some stations will detect gravity waves, small variations of density in the atmosphere. These waves are visible as short changes in brightness in the light curve during the occultation. It is a very exciting experiment!
Here is the sky coverage map for around 2AM EDT.
Good luck to everyone! Go RECON!
On Saturday morning, August 4, Marc and John were in Senegal with roughly 60 other observers from the US, France, and Senegal and Rodrigo was in Columbia with a dozen astronomers. Both groups were pursuing the shadow track of 2014MU69, the ~30km Kuiper Belt Object that New Horizons will fly be on New Years Day, January 1, 2019. Rodrigo’s teams in South America were rained out, and Senegal teams faced cloudy conditions. However, all teams persevered and several Senegal sites were clear enough to collect useable data. These data are currently being analyzed and synthesized with last summer’s campaigns to inform the New Horizons team as they plan for the upcoming flyby. We will provide updates as added details are made available.
In addition to collecting useful data, the expedition was a valuable opportunity for US and French observers to work with researchers from Senegal and to build international ties. The link above points to a New York Times article featuring the occultation expedition in Senegal.
Updated RECON coverage for our next official campaign: 2018 July 8 UT – Quaoar.
Over the course of four nights in April and May, the RECON team was able to use Apache Point Observatory’s Astrophysical Research Consortium Telescope Imaging Camera (ARCTIC) on the 3.5-meter ARC telescope to more accurately determine the positions of 31 trans-Neptunian Objects (TNOs). The objects that were observed had high uncertainties in their known orbits that limited our ability to predict occultations. By taking three separate exposures spread out over multiple hours, each object can be seen moving across the sky relative to the stars. By then measuring the object’s position as it moves through the night, a more accurate orbit for the object can be defined, resulting in more accurate occultation predictions. This is an important step in the occultation prediction process. The goal of these measurements is to identify the occultation events with a nominal 30% probability of success.
Drs. Rodrigo Leiva (RECON Postdoctoral Researcher) and John Keller (RECON Co-PI) observed at Apache Point Observatory on April 16-18, 2018. During the first night, they were trained on the APO 3.5-meter telescope by New Mexico State University astronomer Dr. Candace Gray. They then collected astrometry data for 14 out of 21 during the morning hours of the subsequent two nights.
For May 18th and 19th, Rodrigo remotely observed from Boulder with help from new RECON student research assistants Sean Haley, Lizzie Wilde, and Ryder Strauss while John was in Washington DC remotely controlling the telescope. After taking flats, darks, and bias frames, science images started to roll in. The objects observed were between magnitude 20-23 and were observed 3 times over the course of both nights. Each exposure of the same object was taken long enough apart so that the object had moved at least three arcseconds across the sky from the previous exposure. Sean, Lizzie, and Ryder looked through all the science images as they came in to make sure they were good to use (no weird light artifacts) and to confirm that the object was in the frame. Each object was found by assigning a pixel color (red, green, and blue) to the three images taken of each object and combined to make a color image that is useful to find moving targets – can you guess why? An example of what is seen with this method is shown below. 17 out of 18 objects were successfully recovered and put into the RECON occultation prediction system.
The occultation prediction system has also now been updated with the new, much more accurate, Gaia DR2 (Data Release 2) data, shown here. With an incredible increase in positional accuracy (three orders of magnitude more accurate than previously measured!) provided by Gaia, the uncertainty of star locations is no longer a significant factor in our occultation predictions. This means there are more accurate occultation predictions than ever before, which is great news for the future of RECON! Overall, 31 TNO positions were improved to bring the uncertainty in their orbits down to ~0.1 arcseconds. All of these objects are now updated in the system with the new more accurate orbit information gained in these observing runs. They are now accurate enough to potentially provide us with some great occultation opportunities in the future.