The Aeronomy of Ice in the Mesosphere (AIM or Explorer 90) was a NASA satellite launched in 2007 to conduct a planned 26-month study of noctilucent clouds (NLCs).[2] It is the ninetieth Explorer program mission and is part of the NASA-funded Small Explorer program (SMEX).
In March 2023, NASA announced that battery power on the spacecraft had declined below the level needed to sustain operation. The spacecraft reentered Earth's atmosphere in August 2024[3]
Mission
Noctilucent clouds as seen by AIM
The scientific purpose of the Aeronomy of Ice in the Mesosphere (AIM) mission is focused on the study of polar mesospheric clouds (PMCs) that form about 80 km (50 mi) above the surface of Earth in summer and mostly in the polar regions of Earth. The overall goal is to resolve why PMCs form and why they vary. AIM expected lifetime was at least two years. AIM measures PMCs and the thermal, chemical and dynamical environment in which they form. This will allow the connection to be made between these clouds and the meteorology of the polar mesospheric summer echoes. This connection is important because a significant variability in the yearly number of noctilucent ("glow in the dark") clouds (NLCs), one manifestation of PMCs, has been suggested as an indicator of global change. The body of data collected by AIM will provide the basis for a rigorous study of PMCs that can be reliably used to study past PMC changes, present trends and their relationship to global change. In the end, AIM will provide an expanded basis for the study of long-term variability in the climate of Earth. The AIM scientific objectives will be achieved by measuring near simultaneous PMC abundances, PMC spatial distributions, cloud particle size distributions, gravity wave activity, cosmic dust influx to the atmosphere needed to study the role of these particles as nucleation sites and precise, vertical profile measurements of temperature, H2O, OH, CH4, O3, CO2, NO, and aerosols. AIM carries three instruments: an infrared solar occultation differential absorption radiometer, built by the Space Dynamics Laboratory, Utah State University (Solar Occultation for Ice Experiment - SOFIE); a panoramic ultraviolet imager (Cloud Imaging and particle Size Experiment - CIPS); and, an in situ dust detector (Cosmic Dust Experiment - CDE), both designed and built by the Laboratory for Atmospheric and Space Physics, University of Colorado. Ball Aerospace & Technologies Corporation constructed the spacecraft bus and GATS, Inc., Newport News, Virginia, led the data management effort.[4][5]
First seen in 1885, two years after the powerful eruption of the Indonesian volcano Krakatoa, scientists originally thought PMC's formed from the plumes of ash propelled into the sky during that eruption. But the clouds have persisted long after the effects of Krakatoa were felt. These days, some scientists think they are caused by space dust, while others believe that modern-day PMC's are indicators of changing climate of Earth. One thing is for certain: PMC's are shaped by the meteorology of the mesosphere, which does appear to be changing.[6]
Spacecraft
AIM in clean room
The AIM satellite is a 197 kg (434 lb), 1.4 × 1.1 m (4 ft 7 in × 3 ft 7 in) spacecraft, powered by two solar panels, carrying three instruments:[7]
Instruments
Illustration
Instrument Name
Abbr.
Description and scientific objective
Cosmic Dust Experiment
CDE
The instrument records impacts from cosmic dust particles as they enter Earth's upper atmosphere. The instrument uses fourteen polyvinylidene fluoride detectors, which emit a pulse of charge when impacted by a hypervelocity dust particle (velocity 1 km/s (0.62 mi/s)). A measurement of the value and variability of the cosmic dust input will allow scientists to determine the role the particles have in PMC (Polar Mesospheric Cloud) formation. CDE is a nearly identical replica to the Student Dust Counter on the New Horizons mission.[8]
Cloud Imaging and Particle Size
CIPS
The instrument has four cameras positioned at different angles, which provide multiple views of the clouds from different angles and will allow a determination of the sizes of the ice particles that make up the cloud,[9] and can be used to infer gravity waves in the atmosphere.[10]
Solar Occultation for Ice Experiment
SOFIE
The SOFIE uses solar occultation to measure cloud particles, temperature and atmospheric gases involved in forming the clouds. The instrument will reveal the mixture of chemicals that prompt NLC's formation, as well as the environment in which the clouds form.[11]
^Space Dynamics Laboratory (2010). "Programs: AIM – SOFIE". Utah State University Research Foundation. Archived from the original on 19 February 2007. Retrieved 16 March 2010.
^"AIM Mission - Launch". NASA. 4 June 2007. Archived from the original on 16 March 2010. Retrieved 16 March 2010. This article incorporates text from this source, which is in the public domain.
Launches are separated by dots ( • ), payloads by commas ( , ), multiple names for the same satellite by slashes ( / ). Crewed flights are underlined. Launch failures are marked with the † sign. Payloads deployed from other spacecraft are (enclosed in parentheses).
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