Research done through the clouds
Research done through the clouds
![]() |
| Research done through the clouds |
When it comes to talking about the universe, I’m not usually at a loss for words. But every so often, I see something so awe-inspiring and unusual that words don’t do it justice. And it seems that when I posted an image of this last year, it looks like I’m not alone here. Such is the case with noctilucent clouds, a strange and beautiful phenomenon that occurs high in the Earth’s mesosphere and requires a unique set of conditions to form. In fact, these cloud formations are so captivating that they’ve inspired communities of watchers, who share atmospheric data online in the hope of seeing one for themselves. So, what are noctilucent clouds? What gives them their ghostly luminescence? And what surprising insights can they offer, not just about Earth’s atmosphere, but perhaps the future of our planet? I’m Alex McColgan, and you are watching Astrum. Join me today as we view spectacular images of these eerily beautiful cloud formations, learn how they form, and understand why they are giving scientists a surprising window into Earth’s changing atmosphere.
Imagine a clear summer night. The Sun has dipped below the horizon, and Capella is shining brightly to the North. Suddenly, a bright streak erupts low in the northern sky. It might look like shining silver thread, or maybe an icy blue whirl. Slowly, the streaks get brighter and clearer, until finally, the whole sky glistens with a patchwork of eerily shining clouds. Night shining clouds such as this formation photographed over the Baltic Sea are truly spectacular, and no, they don’t actually emit light. They get their glowing appearance by reflecting solar radiation during astronomical twilight, when the sun is between 6 and 16 degrees below Earth’s horizon and remnant light is scattered in the upper atmosphere. Because noctilucent clouds form at very high altitudes (around 76 to 85 kilometres above the terrestrial surface), they can reflect the Sun long after an observer has fallen into Earth’s shadow.
So, while noctilucent clouds also form during daylight hours, they are only visible to the unaided eye at night. To make a noctilucent cloud, you need water, dust particles and incredibly cold temperatures. Unlike normal clouds, which form in the Earth’s troposphere, where 75% of the atmosphere’s mass and 99% of its water vapour occurs, noctilucent clouds form high in the upper mesosphere, which is the atmosphere’s third layer, above the stratosphere. Just a reminder, the lowest layer of atmosphere on the Earth is the troposphere, the boundary of which is the tropopause, then the stratosphere, stratopause, mesosphere, mesopause, thermosphere, thermopause, and then finally the exosphere. For more about all these layers, check out this video. The mesosphere is a tricky region to study, since its too high for aircraft to fly and too low for orbital spacecraft due to atmospheric drag.
![]() |
| Research done through the clouds |
Noctilucent clouds form slightly below the mesopause, which is the upper boundary between the mesosphere and thermosphere. The mesopause is also the coldest region of Earth, with temperatures that can plummet below 100 degrees Celsius. (By comparison, the coldest temperature ever recorded in Antarctica was minus 89.6 degrees Celsius!) These frigid conditions produce tiny ice crystals less than 100 nanometers in diameter, which then gather on dust particles. Researchers have learned that the mesosphere must reach minus 120 degrees Celsius for these ice crystals to form. That’s pretty cold! But if noctilucent clouds require such cold conditions, why do they occur during summer? Well, one unusual property of the mesopause is that it is colder in summer than in winter. Known as the mesopause anomaly, this happens because hot air in the lower troposphere expands, resulting in upswelling gasses that decompress in the mesosphere, causing adiabatic cooling.
Because noctilucent clouds require very low temperatures, they only appear for 60 to 80 days out of the year, peaking around 20 days after the solstice. If you want to see a night shining cloud formation, you’ll need a lookout spot between ±50 and ±70 degrees latitude. Although satellites have spotted many mesospheric clouds north of the 70th parallel, here on Earth, the polar regions have too much ambient light during summer for optimal viewing. So, if you happen to live in northern Norway or Alaska, you’ll have to travel south for your NLC watching! That’s a pretty good survey of what we know, so let’s talk about what we don’t. Saying the mesosphere is a very dry place would be a bit of an understatement. In fact, it is one million times dryer than air from the Sahara Desert. Not exactly a place you’d expect to find clouds! We currently think upswelling air from the troposphere is the likely source of this moisture.
More puzzling, however, is the question of where the dust is coming from. One theory is that it comes from space in the form of debris. The Earth gets bombarded daily with thousands of meteorites and other space debris. Could they leave enough dust to create such massive cloud formations? Or could there be other causes? Interestingly, NLCs were first sighted in 1895, two years after Krakatoa’s massive volcanic eruption in Indonesia which spewed debris into the upper atmosphere. It has to be something big like this because otherwise the atmospheric layers don’t mix very much, and so dust wouldn’t usually make it to the mesosphere. We also know that manmade sources, such as exhaust from space shuttles, can sometimes trigger noctilucent clouds, such as a 2014 incident when the SpaceX Falcon 9 caused noctilucent clouds over Orlando, Florida. In 2009, the United States Naval Research Laboratory successfully created an artificial NLC using exhaust particles from a suborbital sounding rocket.
![]() |
| Research done through the clouds |
And in 2018, the University of Alaska created a noctilucent cloud by releasing water from a suborbital rocket. But without such proximate causes, the source isn’t easy to pinpoint. Luckily, NASA has launched a satellite, known as the Aeronomy of Ice in the Mesosphere, or AIM, to answer these and other pressing questions. It was first launched in 2007 but as of 2022 is still operational. AIM is powered by two solar panels and is equipped with three payload instruments. The Cosmic Dust Experiment, which emits pulses to measure speeding dust particles. The Cloud Imaging and Particle Size, has four cameras that image mesospheric clouds from variable angles to create a detailed 2D panoramic view. And the Solar Occultation for Ice Experiment, which measures particles, temperature and atmospheric gasses in order to identify chemicals and conditions for NLC formation.
There have also been several experiments to synchronize AIM’s observations with those of low-flying aircraft, the first of which was conducted in July 2009. By synchronizing data between satellites and aircraft, scientists can construct far more detailed models of mesospheric cloud formation and their features than they could from AIM alone. For NASA and other atmospheric researchers, answering these questions is no idle matter. The mesosphere is a remarkably sensitive indicator of changes that are happening elsewhere in the atmosphere. The same features that make it so unusual, its rarified gasses and sensitivity to changes far down in the troposphere, make it a useful canary in the coal mine, so to speak. Decades of NLC study have made it clear that they are becoming more frequent, and climate researchers are now beginning to link changes in NLC distribution to global climate change.


