Contreras Wildfire and Kitt Peak

Over the years working at Kitt Peak National Observatory, I’ve seen several fires from the domes at the summit. A few of these fires have even approached close enough to create nail-biting situations where we prepared to evacuate the site. However, a little over a week ago, a fire burned right up to our facility. As an operator on the Mayall 4-meter and WIYN 3.5-meter telescopes, I’m tasked with facility and personnel safety after hours. So, this means I was keeping a close eye on the fire up until the point we had to leave Kitt Peak.

While driving up to work at Kitt Peak National Observatory on Saturday night, June 11, I passed through the small town of Three Points, Arizona and noticed an orange glow on the ridge between Kitt Peak and Baboquivari Peak. I gritted my teeth, afraid I was seeing the beginnings of a fire. I hoped I was wrong. I’d hoped someone had installed a radio tower with an orange light between the town and the mountain, but soon after I started driving up the Kitt Peak road, my hopes were dashed. I soon saw a fire burning off in the distance. At that point, I wasn’t terribly worried, I’d seen fires in that part of the range before and the Tohono O’Odham fire department usually knocked them out within a couple of days. When I reached the summit, I checked in with the duty operators, let them know I’d arrived on site and confirmed they had seen the fire and that officials knew about it. Since it had been visible from a nearby town, I figured they did, but it’s always good to check. By all accounts, the fire started from a lightning strike earlier that evening.

Unfortunately, the southwest has been suffering a drought which has now lasted over 20 years and vegetation was extremely dry. However, the wind was calm and blowing away from the observatory, so when I started my shift on Sunday, June 12, we were able to work with the fire burning off in the distance and smoke blowing away from us. As it turns out, the WIYN telescope, where I was working, had a problem with its optical system. A vacuum system which keeps the heavy mirrors off the hard mounting points had failed, causing minor distortion. We were taking spectra, so this problem didn’t keep us from working, but it needed to be fixed, so on Monday, June 13, our optical engineer began the process of removing the secondary mirror from the telescope to investigate the problem. This is a big job and it couldn’t be completed in one day, so my primary job that night was to monitor the fire’s progress and make sure the wind didn’t shift to blow over the observatory. Here’s a look at the fire shortly after sunset.

View toward Baboquivari Peak on June 13, 2022

On Tuesday, while I slept, it became apparent that the fire was a big enough danger that steps should be taken to make the site as safe as possible. Engineers began shutting down less critical systems and making things as safe as possible. The wind shifted that afternoon and more smoke began coming toward the site. When many people imagine an observatory, they might imagine anywhere from one to six telescopes on a remote mountain summit. It may help to understand that Kitt Peak National Observatory is the world’s largest observatory campus with over twenty telescopes. There are, in fact at least six dormitory buildings along with several houses, kitchen facilities, a full maintenance yard including automotive shop, water treatment facility, backup generators and so forth. Like many college campuses, Kitt Peak is almost like a small town in its own right. So lots of people were at work all across the site through the day. That evening, I had a briefing from the Kitt Peak director. Because of the smoke, telescopes would be closed that night. Smoke can damage optics. As the night started, I went up to the Mayall telescope and took a photo from the visitor gallery. Only a little of the fire was visible from that vantage, looking like a string of lights on the mountain in the background, just to the right of the left-most dome. Still, this gives you an idea of how close the fire was getting.

Contreras Fire on the night of Tuesday, June 14

The wind picked up the night of June 14 and the fire seemed to pick up strength. As you can see in the first photo, there was a small ridge line between us and the fire. By the morning of June 15, the fire crested that ridge and I wondered how much longer we would remain on site. Here’s what it looked like on Wednesday morning.

Contreras Fire on the Morning of June 15.

I went to bed, knowing someone would wake me if we needed to evacuate. I woke up and attended two administrative meetings. From my room, I could already tell there was much more smoke in the air by Wednesday afternoon. As soon as the meetings were finished, I went to the WIYN telescope. From that vantage, I saw that the fire had progressed dramatically. A wall of smoke rose from just below the mountain summit and I could see flames just over a mile away. I went into the observatory and learned that a controlled shutdown of as many systems as possible was underway. I helped where I could. Among other things, I helped to carry one piece of instrumentation down to an engineer’s car so it could be transported off the mountain safely. Firefighters began arriving on the mountain. One of them warned us a plane was about to drop a load of fire retardant and we should move our vehicles so they would be damaged when that much water and retardant came down onto the mountain. We did as directed and soon afterward I was called into a meeting in the director’s office. While in that meeting, the incident commander gave us the order to evacuate. I went to my dorm room, packed up as much as I could and went to my car. I was off the mountain within about half an hour.

Because my home is in New Mexico, the observatory management put me up in a hotel room in Tucson that night. I hoped we would be evacuated, the firefighters would hold the line on the fire and I would return in a night or two. Still I had an uneasy feeling as I walked back to my hotel room after dinner that night. Here’s the view of the hotel. What looks like clouds low in the sky is smoke from the Contreras wildfire.

Smoke from the Contreras Wildfire, visible from Speedway Blvd in Tucson, Arizona

On Wednesday night, I watched the fire on the mountain webcams from my hotel room. Part of my job is accounting for the night’s use so it can be reported to the National Science Foundation. I filled out my reports. Thursday night was more of the same. On Friday morning, I filled out my report, but soon after, computers at the observatory went dark. A little while later, I learned that utility power had gone out on the mountain and we’d lost the internet connection. The fire had reached the summit.

I went home on Friday, but have continued to follow the news. The firefighters did a tremendous job. No scientific buildings were lost. As far as I’ve heard, only four support structures were consumed by the fire. It helped that almost all the buildings at Kitt Peak are constructed of concrete, steel, and brick. Since Saturday, the fire has been contained, but access to the Kitt Peak summit is still strictly regulated for safety. As soon as its safe, engineers and facility teams will begin the process of inspecting the site. They’ll see how much smoke and ash infiltrated the domes. They’ll see if there’s been heat damage. They’ll make sure we have reliable power and internet. Once that’s done, it’ll be time to see if the telescopes and instrumentation can be brought back on line and repair things as needed. It’ll be a process and it’ll take time. Still, I can’t emphasize enough how grateful I am to the firefighters who jumped in and kept the facility as safe as possible so that we actually can look forward to resuming operations. They did tremendous work and I look forward to resuming science at Kitt Peak in the not-too-distant future.

Confronting Change

In earlier posts, I’ve discussed working with the Hydra spectrograph on the WIYN Telescope at Kitt Peak National Observatory. It’s a piece of instrumentation that allows astronomers to observe up to 90 objects simultaneously during one telescope pointing. The WIYN telescope can see one square degree of the sky at a time. Hydra has a set of optical “buttons” which can be placed on a metal plate at the position where an object will be in the field of view. These buttons send data to the spectrograph two floors below via fiber optic lines. The device that places these buttons is a robot, which resembles the claw from crane machine. It picks up each button from a parked position and puts it where it belongs.

Sticker on Hydra’s side

This type of multi-object spectrograph is somewhat common now, but Hydra was one of the first of these types of spectrographs built in the early 1990s. In fact, the instrument is older than the WIYN telescope and I helped to commission the instrument in its first version at the Mayall 4-meter. Precision machines like the Hydra gripper suffer a lot of wear and tear in 30 years, so a little over a year ago, Hydra began an upgrade process. The engineers worked with Prod Design and Analysis in El Paso, Texas to upgrade the gripper with new technology. The folks at Prod were struck by how much the gripper resembled a crane machine’s claw and added the sticker you see in this first photo.

Hydra Control Rack

As you might imagine, I’ve become quite familiar with Hydra, working with it off and on for almost thirty years. However, making major changes to the instrument meant learning new procedures. The original Hydra gripper was an analog device that “knew” where buttons were by counting steps using a device called an encoder and then remembering those steps to go back and pick the button up again. If there was some electrical noise or a mechanical problem that caused the count to be less precise, it could miss picking up the button. The upgraded Hydra also uses encoder counts, but it has added new programmable logic controllers and video analysis. It goes to the button, takes a picture, analyzes that pictures and then adjusts it’s position, if needed, to get the button. All this new logic has meant that we have a new control cabinet in the telescope to house electronics. The hope is that this will make positioning more accurate. However, it has meant learning new ways to monitor the process of the gripper at work and recovering the gripper if problems occurred.

This past week was one of the first times I’ve had to use the upgraded Hydra without one of the engineers on hand in case problems occurred. I made sure to review the manual, because it had been several months since my introduction to the upgrades and I reviewed the troubleshooting procedures. The first night of observing started out quite smooth. We had four field setups without any problem whatsoever. Then on the fifth field configuration, a heart-stopping problem occurred. The Hydra control program crashed while the gripper was carrying a button to a new position. Of course, these buttons and their attached fibers are all very delicate and if Hydra forgets the button’s position, there’s a risk that the attached fibers could get tangled. This could prove to be a very expensive problem.

In the old days, a problem like this automatically meant going into the dome, which is a cold proposition on a winter night! Then with a long stick , carefully reaching into the instrument and releasing the button from the gripper jaws, which allow you to open the instrument. After that, you’d have to manually place this fragile, optically sensitive button and fiber back into its stow position. In short, it’s a delicate procedure to do when you’re cold and on a lift in a dark dome!

The new Hydra Handpaddle

Now we have a handpaddle, which lets us talk to the gripper directly. I went to the Troubleshooting guide, refreshed my memory and followed the instructions. For the most part they worked. I was able to control the gripper and set the button down in a controlled way. Unfortunately, we’re still working out some bugs, so I still had to open Hydra and check the button’s real position, but it was a much quicker, safer operation.

Confronting change in procedures that had grown familiar and routine was definitely scary and a little challenging. The things that helped me manage my discomfort were focusing on the familiar parts of the routine, reviewing the new procedures before starting work, and then when a problem did happen, I took a deep breath and used the instructions and my experience to solve the problem the best I could. This past week, the upgraded Hydra moved from a machine that presented me with a little anxiety to a machine I look forward to understanding better.

Summer Shutdown 2021

I returned to work on site at Kitt Peak National Observatory in November 2020. Social distancing regulations were put in place along with several other protocols to minimize the risk of COVID-19 infection. In that time, we’ve been making great strides commissioning the DESI spectrograph and starting it’s five-year survey, which is intended to result in the most comprehensive 3D map of the universe yet made. The instrument is already getting results. For those who don’t recall earlier posts about DESI, it has 5000 optical fibers mounted at the prime focus of the Mayall 4-meter telescope. Each fiber can be positioned to align precisely with an object on the sky. The fibers run to a spectrograph where the light is analyzed and redshifts of distant objects such as galaxies and quasars can be measured. The following image shows how much sky DESI gets in one pointing. It shows the nearby Andromeda Galaxy taking up much of the field, but as an example, you see that one fiber has landed on a distant quasar. It’s spectrum is displayed in the inset box. Each of the pizza-slice segments represents the 500 fibers in one petal of the DESI instrument.

The disk of the Andromeda Galaxy (M31), which spans more than 3 degrees across the sky, is targeted by a single DESI pointing, represented by the large circular overlay. The smaller circles within this overlay represent the regions accessible to each of the 5000 DESI robotic fiber positioners. In this sample, the 5000 spectra that were simultaneously collected by DESI include not only stars within the Andromeda Galaxy, but also distant galaxies and quasars. The example DESI spectrum that overlays this image is of a distant quasar that is 11 billion years old. Credit: DESI collaboration/DESI Legacy Imaging Surveys/LBNL/DOE & KPNO/CTIO/NOIRLab/NSF/AURA/unWISE

Summer in Arizona is monsoon season. In short, we get a lot of rain. Clear skies can be few and far between. As a result, this is the time of year engineers often choose to shut down the telescopes to do maintenance and make modifications. The DESI instrument has been performing well, but that doesn’t mean it can’t be improved. The fibers in each of those pizza-slice shapes are aligned by a system called the “Command Action Network” or CAN-Bus for short. It was determined that the CAN-Bus system in DESI could be improved. To do this, each petal has to be removed from the Mayall’s prime focus and placed in an area where it can be worked on. We’re able to do this work this summer because of the availability of COVID vaccines. We do take care to practice social distancing where possible and, especially in the wake of the Delta variant’s rise, we’re staying masked throughout the day. This next photo shows DESI with four of the petals removed.

DESI opened up. The red device in the foreground is used to carefully extract the petals.

The trickiest part of this operation is that the DESI petals are all attached by several yards of fiber optic cable to the spectrographs two stories below. When we remove the petals, we don’t want to torque or strain those cables too much. The petals are lifted down and placed on the floor beside the telescope. Once there, they’re placed into clean tents where they’re worked on. Here we see two members of the DESI team diligently working on the CAN-Bus electronics behind the fiber positioners.

Working on the petals. The fiber optic cables come out of the tent, run along the top and then over the rail to the spectrographs below.

Finally when all the new electronics are installed, the petals have to be tested. Among other things, we need to make sure we didn’t break any of the fibers as we handled the petals. DESI is designed to be able to shine light from the spectrograph up through the fibers. We call these “back illuminators” and a camera mounted just below the telescope’s primary mirror can take an image of the back illuminated fibers to see what position they’re in. Here we see the petal out of the telescope with the back illuminators turned on.

DESI’S fibers glowing a friendly blue, telling us all is well after the work has been completed.

Once the upgrades are completed, the petals are reattached to the telescope. This is a big collaborative effort involving many people from around the country and around the world. Once it’s done, we should have made what was already a powerful machine designed to answer questions about dark energy into an even more powerful machine.

Assembling the Puzzle

This has been another week helping to install the Dark Energy Spectrographic Instrument or DESI at the Mayall 4-meter telescope at Kitt Peak. In short, the goal of DESI is to study the effect of dark energy on the expansion of the universe. We plan to collect spectra of tens of billions of galaxies and quasars with the goal of making a three-dimensional map of the universe out to about 11 billion light years. You can read more about the DESI project at https://www.desi.lbl.gov/

The DESI project is spearheaded by Lawrence Berkeley Lab in California and being installed at Kitt Peak in Arizona. However, it really represents a worldwide collaboration. There are scientists working on this project from England, France, Spain, Italy, South Korea, China, France, Canada, Colombia, Australia, and others plus numerous institutions within the United States. All of these agencies are not only contributing expertise, but actually building components that will go into the finished instrument.

In an earlier post, I spoke about how we worked to remove the Mayall telescope’s original top end. The top end originally housed both a secondary mirror and a prime focus camera. Both of these have been used to make groundbreaking discoveries over the last five decades. The Mayall was the telescope Vera Rubin used to study rotation curves of galaxies, which led to the discovery of dark matter. I’ve helped with observations that have led to the confirmation of numerous exoplanets. We’re now replacing the telescope’s original top end with a new one that will hold 5000 fibers at prime focus. Each of those fibers will run to spectrographs that will break up the light from objects in the sky so it may be analyzed and the position of the object can be measured. In the photo above, you can see the new top end being assembled to the left of the telescope.

To get light from the sky onto the fibers, the telescope will collect it with the primary mirror. That sits in the big white structure at the center of the big blue horseshoe-like structure in the photo above. The mirror will direct that light to the top end. Because the mirror is curved, allowing the light to be collected and redirected, it means the focus changes across the field of view. To deal with that, you need to put some lenses in front of the fibers, sort of like glasses. Another real world problem of telescopes is that as you point toward the horizon, light gets spread out. So you need optics to compensate for where you’re pointing in the sky. Sort of like glasses that automatically adjust themselves for where you’re looking.

Scientists from England assembled those specialized “glasses” for the telescope. Those arrived last week and I was on hand during their assembly at Kitt Peak. You see those assembled optics in the lower photo. Scientists from Italy built the “Hexapod” pointing system, which keeps those optics aligned. That arrived and was tested about a month ago. Scientists from Fermilab in Chicago are responsible for integrating those systems and putting them together in the top end ring. That process will start next week. It’s all quite a puzzle and it’s been remarkable to see it all come together. It’ll be even more amazing to see what science it yields.

Of course, work at Kitt Peak helps to inspire my science fiction. As a reminder, this is the last weekend of the Smashwords Summer/Winter sale. You can learn about my science fiction books that are on sale at:

We also have fantasy and steampunk titles on sale. You can learn about them at:

A Vampire in Daylight

In my novel Vampires of the Scarlet Order, I introduced Daniel McKee, a vampire who works as a telescope operator. In my novels, the vampires often need to find ways to earn incomes since I’ve always been a bit skeptical that it’s easy to stash away vast amounts of wealth given nothing but time. Of course, being vampires, my characters must find night work, which can be a challenge, especially in some professions. Fortunately, Daniel was an astronomer when he became a vampire, so his progression to an all-nighttime position wasn’t difficult.

Daniel is autobiographical only in the sense that he’s a telescope operator. As I’ve mentioned in earlier posts, the Mayall 4-meter is undergoing a major refit. The entire top ring in the picture above will be coming off and replaced with a new top ring that holds 5000 optical fibers which will be used to collect light from millions of objects around the sky. Because the refit is so extensive and so time-consuming, there’s no nighttime work to do on the telescope, so those of us who work as telescope operators have been spending one shift a month supporting the refit operation during the day. I find myself wondering what Daniel would make of that!

In fact, Daniel would probably quit to find an operator’s position elsewhere. Otherwise, he might find work to do that would allow him to remain on a nighttime schedule, such as programming or manual writing. Sadly, Daniel would miss out on a fascinating engineering endeavor and some good camaraderie. In the photo above, the engineering crew is installing a scaffolding that will give them access to the telescope’s top end. However, the scaffolding isn’t just for access. It will help hold the telescope struts in place after the current top ring is removed and before the new one is installed. It will be sturdy to support people and to assure that the telescope will function after this exercise is over.

What’s more, observatories require more than night time staff to function. There is a large contingent of people who work at the observatory during the daytime. They support the infrastructure, such as water services, electricity, and internet. They provide engineering support, keeping the telescopes operational years after construction when original parts are no longer manufactured and the telescope must be upgraded to work with new electronics. This is a great team of people that I unfortunately don’t get to interact with on most nights because they go home right as I’m starting my work day. So it has been great to get to know some of these “unseen” co-workers.

Sadly once you become a vampire, even good people can look like a tasty treat, so perhaps it’s just as well Daniel wouldn’t interact with the observatory’s day staff, but I’m delighted I’ve had the opportunity!

You can read more about Daniel’s adventures in Vampires of the Scarlet Order. Learn more about the novel at: http://www.davidleesummers.com/VSO.html

The adventures of the Scarlet Order before Daniel became a member are featured in Dragon’s Fall: Rise of the Scarlet Order. Read a sample chapter and learn more at: http://www.davidleesummers.com/dragons_fall.html

I will be signing both of these novels next month on the Friday, May 25 at Boutique du Vampyre in New Orleans, Louisiana from 3-6pm. That’s the Friday of Memorial Day weekend. I’ll also be doing a special reading from the novels afterwards at Potions, an amazing speakeasy bar nearby. Be sure to drop by the signing to learn more about the reading. Mark your calendars!

Arizona and NM STEM Resources for Kids

At Phoenix Comicon, I was on a panel called “Growing Up With Science.” Our goal was to suggest ways to keep kids—and particularly girls and minorities—interested in science, technology, engineering, and math fields. This post attempts to collect several of the suggested places around Arizona and New Mexico parents can take their kids to investigate these fields. The photo below is from the Phoenix Comicon photo collection and shows the panelists: Dean Frio, Martha Alice, Karen Knierman, David Lee Summers, and Aireona Raschke.

STEM-Panel

The categories below are presented roughly in the order we presented them during the panel.


General Education Resources

School of Earth and Space Exploration at Arizona State University “is training the next generation of explorers and citizen scientists.” They offer a number of field trips, teacher workshops and partnerships with local schools, exploring astronomy and earth sciences. For more information, visit: http://sese.asu.edu/outreach

Ask a Biologist is a program at Arizona State University where kids can ask questions, access age-appropriate science articles, and interact with activities and online games. http://askabiologist.asu.edu/

Kitt Peak National Observatory Visitor Center. Museums and visits to science facilities are a great way to interest kids in science. Kitt Peak offers year round tours and even night programs where people can observe with docents expert at interpreting the night sky. Get more information at: http://www.noao.edu/outreach/kpvc/

Lowell Observatory is a center for astronomical research and works to bring the results of that research to the general public. They have an outstanding visitor center in Flagstaff and terrific online resources at: http://lowell.edu/

Biosphere 2 serves as a center for research, outreach, teaching and life-long learning about Earth, its living systems, and its place in the universe. They offer guided tours to individuals and schools, plus they also offer teacher training programs. Learn more at: http://b2science.org/

Asombro Institute for Science Education works to foster an understanding of the Chihuahuan Desert through programs given to schools in Southern New Mexico and West Texas, plus programs offered at the Chihuahuan Desert Nature Park. Learn more at: http://www.asombro.org/


Experiences and Camps

Astronomy Camp is held each year at Kitt Peak National Observatory and run by Dr. Don McCarthy of the University of Arizona. It gives students hands on experiences in both astronomy and engineering. More information at: http://astronomycamp.org

MathMovesU is a program hosted by Raytheon which has a number of on-line activities and provides scholarships so kids can attend math and science events. http://www.mathmovesu.com/

Phoenix Zoo Camp gives kids an opportunity to spend time during summer and winter breaks at the zoo engaged in activities learning about nature and animals. More information at: http://phoenixzoo.org/camps-programs/camp-zoo/

Young Women in Computing is a camp hosted by the computer science department at New Mexico State University in Las Cruces. In addition to the camp itself, they host after school programs, contests, and teacher-program collaborations. They work not only with young women, but young men as well. Get more information at: https://sites.google.com/site/ywicnm/


Citizen Science Projects

Citizen science projects are projects where you can contribute to projects and discoveries. Generally, you are given an on-line tutorial for the project then taken to a set of data that requires analysis. This is a great way for both adults and kids to contribute to real, on-going science projects.

Zooniverse is a literal clearing house of citizen science projects that can be done from your home computer with an internet connection. The projects range from astronomy, to biology, to climate. Find a project and get involved at: www.zooniverse.org

Amazing Space uses the Hubble Space Telescope’s discoveries to inspire and educate about the wonders of our universe. http://amazing-space.stsci.edu/

Gila Monsters at Saguaro National Park is a program where people can report Gila Monster sightings in and around Saguaro National Park and help preserve these amazing animals. http://www.inaturalist.org/projects/gila-monsters-at-saguaro-national-park

McDowell Mountains Citizen Science Program is the steward program that supports the McDowell Sonoran Field Institute by training and deploying volunteers on the various research projects. The program offers opportunities to Conservancy stewards as well as students and community volunteers. Get details at: http://www.mcdowellsonoran.org/content/pages/citizenScienceProgram#sthash.C1Eu2uUO.tvY4etUl.dpuf