Astrophotos! UH Hilo astronomy students capture dazzling images from atop Maunakea
Students taking an astronomy course on galactic and extragalactic astrophysics traveled up Maunakea, telescopes in tow, to capture images of galaxies for the lab portion of their class.

By Samantha Dane/UH Hilo Stories.
Editor’s note: Student writer Samantha Dane accompanied an astronomy lab class on the evening of March 6 up to the Maunakea Visitors Center (9,200ft/2,804m elevation), where the lab students with their professor and technician set up telescopes just before dark outside the center and then spent hours braving the frigid temperatures collecting their data.
A group of University of Hawaiʻi at Hilo students taking an astronomy course this semester on galactic and extragalactic astrophysics (ASTR 351) travel up Maunakea with telescopes in tow. The objective of the field trip is to capture images of galaxies as a part of their research into galaxy formation for the lab portion of the class.


The 300-level course is taught by Pierre Martin, professor physics and astronomy and chair of the department.
“The goal [of the trip] is to observe four or five galaxies of different shapes and types, and then to make a series of measurements to quantify these differences,” says Prof. Martin.
Assisting with the equipment set up and technology aspects of the field trip is Joben Sasis, educational specialist at the physics and astronomy department. Students in the lab are Yannie Cheng, Akiyele Gilbert, and Oliver Kangwai. Physics and astronomy major Atlas Syncatto, a junior not enrolled in the lab class, joined the group to gain field experience with a new type of telescope not previously used in the lab.
The field lab helps the students achieve the aim of the course, which is to study the formation and form of the Milky Way and its surrounding galaxies, as well as learn how these forms have shifted over time. Students use existing data from observatories along with their own data (collected from this trip) to better understand the physics of these galaxies.
This visit to the 9,200-foot elevation, just outside the Maunakea Visitors Center, is a repeat attempt from the week before. The last lab trip didn’t go according to plan a couple weeks ago due to some unexpected weather. Fog and telescopes don’t mix, it turns out.
Setup and preparation
The students are using two portable Celestron telescopes for their observation, the preparation for which started weeks in advance on campus. Much of this preparation involves installing parts of the telescope such as the camera, filter wheel, guiding assembly, and spacers for focusing. Students also test the software to ensure the telescopes function well in the field. This is an important step, as it ensures the telescopes will be able to properly locate and photograph the galaxies they want using the software at hand.
Once on the mountain, the next step is selecting a spot to observe from, keeping in mind the surrounding landscape and light pollution.
Students then unload an entire SUV’s worth of equipment and begin the lengthy process of reassembling the two telescopes, starting with the tripod mount, telescope, camera, counterweight for the massive lens, and guiding system. Finally, the computers used to operate them are connected. All together, the telescopes are around the size of a person and take many hands to operate and ensure everything runs smoothly.
Next comes the calibration stage. The cameras on the telescopes responsible for imaging are aligned to an approximate location prior to sunset, and several calibrations are taken to improve the final image quality as the sun goes down. It’s a windy evening on the mauna, which makes this process more difficult than it should be. Telescopes and wind don’t go well together either, it turns out.
Even after the sun goes down, the prep work continues for a little longer. Students must ensure the telescope can point and track the movements of the stars through the night. Once they’re sure the telescope is fully calibrated, the observation can finally begin.
Let the observation run begin!

Once the telescope is focused, a sequence of consecutive exposures are taken.
“Typically, we would do 30-45 minutes in total for one filter,” says Prof. Martin. The wind only adds to this time, as exposures can be lost from wind shaking the telescope. The students rotate between filters for each galaxy, which can be a real test of patience when monitoring the telescopes in the frigid air. It’s difficult, time consuming work, but the end result is worth it.



The main reason behind using filters is to gain a better understanding of the galaxies based on their color. Many galaxies are either blue or red, and these colors reflect their characteristics, such as the rate of star formation within them.
The color of a galaxy can provide other important insight into its chemical composition and formation as well, and filters help the group to quantify and establish what colors the galaxies are. For example, some colors will appear brighter in a red filter than a blue one or vice versa, and this same concept is applied to the galaxies they image.
“This is why we used a set of three filters with the camera on the portable telescopes, to be able to quantify the color in function of different galaxies observed,” Martin says, as each one filters light differently and allows them to parse out what the galaxies are made of.
The team also utilizes a secondary smaller and fully automated telescope that images the galaxies without a filter, resulting in the traditional full color picture. Like the larger telescope, this one too takes repeated exposures to build up a full image.
The value of field lab experience

This type of field lab provides students with valuable and very transferable skills in the field of astronomy. Despite using only small telescopes in the lab, Martin says “their instrumentation and the techniques involved are very similar to what is done on the big [telescopes] so it’s very good training for the students.”
Atlas Syncatto, the junior majoring in physics and astronomy but not enrolled in the lab class, joined in the observation run to gain field experience with the smaller smart telescope as it was the first time the lab was trying it out. After graduation, Syncatto hopes to work at a Maunakea observatory as a telescope operator. This is an example of how the lab acts as a small-scale version of how larger observatory telescopes work, and UH Hilo as a whole acts as a pipeline to work at the highly advanced observatories, such as the ones further up Maunakea.
“It’s also a great chance to go up and observe and see all the beautiful stars,” says lab student Oliver Kangwai.
Getting the field experience even with smaller telescopes goes a long way for students, and it turns out the images they’re able to capture are just as beautiful as you’d expect after a hard night’s work. Color this reporter impressed!
Story by Samantha Dane, a biology major at UH Hilo.



















