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Equuleus
Equuleus
Equuleus
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Equuleus
Constellation
Equuleus
List of stars in Equuleus
AbbreviationEqu
GenitiveEquulei
Pronunciation/ɪˈkwuːliəs/ Equúleus, genitive /ɪˈkwuːliaɪ/
Symbolismthe pony
Right ascension20h 56m 10.9212s–21h 26m 20.0331s[1]
Declination13.0390635°–2.4773185°[1]
QuadrantNQ4
Area72 sq. deg. (87th)
Main stars3
Bayer/Flamsteed
stars		10
Stars brighter than 3.00m0
Stars within 10.00 pc (32.62 ly)0
Brightest starα Equ (Kitalpha) (3.92m)
Nearest starHD 200779
Messier objects0
Meteor showers0
Bordering
constellations		Aquarius
Delphinus
Pegasus
Visible at latitudes between +90° and −80°.
Best visible at 21:00 (9 p.m.) during the month of September.

Equuleus is a faint constellation located just north of the celestial equator. Its name is Latin for "little horse", a foal. It was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. It is the second smallest of the modern constellations (after Crux), spanning only 72 square degrees. It is also very faint, having no stars brighter than the fourth magnitude.

Notable features

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The constellation Equuleus as it can be seen by the naked eye.
The constellation Equuleus, color and contrast enhanced.

Stars

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Further information: List of stars in Equuleus

The brightest star in Equuleus is α Equulei, traditionally called Kitalpha, a yellow star magnitude 3.9, 186 light-years from Earth. Its traditional name means "the section of the horse".[2]

There are few variable stars in Equuleus. Only around 25 are known, most of which are faint. γ Equulei is an α2 CVn variable star, ranging between magnitudes 4.58 and 4.77[3] over a period of around 12½ minutes. It is a white star 115 light-years from Earth, and has an optical companion of magnitude 6.1, 6 Equulei. It is divisible in binoculars.[2] 6 Equulei is an astrometric binary system itself,[4] with an apparent magnitude of 6.07.[5] R Equulei is a Mira variable that ranges between magnitudes 8.0 and 15.7[6] over nearly 261 days. It has a spectral type of M3e-M4e[6] and has an average B-V colour index of +1.41.[7]

Equuleus contains some double stars of interest. γ Equulei consists of a primary star with a magnitude around 4.7 (slightly variable) and a secondary star of magnitude 11.6, separated by 2 arcseconds. ε Equulei is a triple star also designated 1 Equulei. The system, 197 light-years away, has a primary of magnitude 5.4 that is itself a binary star; its components are of magnitude 6.0 and 6.3 and have a period of 101 years. The secondary is of magnitude 7.4 and is visible in small telescopes. The components of the primary are becoming closer together and will not be divisible in amateur telescopes beginning in 2015.[2] δ Equulei is a binary star with an orbital period of 5.7 years, which at one time was the shortest known orbital period for an optical binary. The two components of the system are never more than 0.35 arcseconds apart.

Deep-sky objects

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Due to its small size and its distance from the plane of the Milky Way, Equuleus is rather devoid of deep sky objects such as star clusters and nebulae. Some very faint galaxies in the New General Catalogue between magnitudes 13 and 15 include NGC 7015, NGC 7040, and NGC 7046. NGC 7045 is a triple star that was mistaken as a nebula by its discoverer, John Herschel.[8] Other faint galaxies in the Index Catalogue include IC 1360, IC 1361, IC 1364, IC 1367, IC 1375, and IC 5083. IC 1365 is a group of galaxies. The magnitudes of these objects vary from 14.5 to 15.5, making them hard to see in even the largest of amateur telescopes.[9]

Mythology

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Seen in Urania's Mirror (1825)

In Greek mythology, one myth associates Equuleus with the foal Celeris (meaning "swiftness" or "speed"), who was the offspring or brother of the winged horse Pegasus. Celeris was given to Castor by Mercury. Other myths say that Equuleus is the horse struck from Poseidon's trident, during the contest between him and Athena when deciding which would be the superior. Because this section of stars rises before Pegasus, it is often called Equus Primus, or the First Horse. Equuleus is also linked to the story of Philyra and Saturn.[10]

Created by Hipparchus and included by Ptolemy, it abuts Pegasus; unlike the larger horse, it is depicted as a horse's head alone.[2] [11]

Equivalents

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In Chinese astronomy, the stars that correspond to Equuleus are located within the Black Tortoise of the North (北方玄武, Běi Fāng Xuán Wǔ).[12]

See also

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References

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[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia

Equuleus

View on Grokipedia
from Grokipedia
EQUULEUS (EQUilibriUm Lunar-Earth point 6U Spacecraft) is a mission consisting of a 6U , measuring approximately 10 cm × 20 cm × 30 cm and weighing 10.7 kg, developed jointly by the and the University of Tokyo's Intelligent Space Systems Laboratory (ISSL). Launched on November 16, 2022, as one of ten aboard NASA's Artemis I mission via the , EQUULEUS achieved a in space to demonstrate low-thrust for efficient maneuvers beyond and to perform scientific observations from the Earth-Moon 2 (EML2). Its primary engineering goal is to validate water-based for orbit transfers to libration points, marking the first such success for a using this technology. The mission's engineering objectives focus on energy-efficient navigation in the Sun-Earth-Moon gravitational regime, utilizing a water resistojet propulsion system (AQUARIUS) with as to reach and maintain a around EML2, approximately 60,000 km behind the . This demonstration supports future low-cost deep-space exploration by small spacecraft, building on JAXA's heritage since 2003 and emphasizing components for affordability. Scientifically, EQUULEUS addresses three key areas in cislunar space: imaging the structure and dynamics of Earth's plasmasphere to study effects; monitoring flux for hazard assessment in future lunar missions; and detecting lunar impact flashes on the 's to quantify activity. EQUULEUS carries three specialized instruments to fulfill its scientific payload: PHOENIX, an extreme ultraviolet (EUV) imager that captures global images of helium ions in the plasmasphere and observes lunar exospheric emissions like sodium atoms, with a field of view of 11.9° × 11.9° and integration times up to one hour; CLOTH (Cis-Lunar Object Detector within Thermal Insulation), a lightweight dust detector integrated into the spacecraft's thermal blanket, sensitive to particles larger than 4 µm traveling at over 10 km/s across a 439 cm² area; and DELPHINUS, a high-speed camera system operating at 60 frames per second to detect faint lunar impact flashes down to 4.5 visual magnitude during the Moon's night side. These instruments enable unprecedented observations from a platform, with PHOENIX notably imaging the plasmasphere's contraction during geomagnetic storms in May 2023 en route to EML2. Communications with were lost on May 18, 2023, after it completed its major orbital maneuvers en route to EML2, having achieved its primary engineering objectives. Results from its plasmasphere observations have been published in peer-reviewed journals to advance understanding of magnetospheric dynamics. The mission's success underscores the viability of nanosatellites for interplanetary science, paving the way for scalable exploration architectures.

Background and Development

Mission Objectives

The EQUULEUS mission, a collaboration between the Japan Aerospace Exploration Agency (JAXA) and the University of Tokyo, primarily aims to demonstrate advanced low-thrust trajectory control techniques to enable a CubeSat to reach and maintain an orbit around the Earth-Moon L2 Lagrange point within the Sun-Earth-Moon system. This involves utilizing a water-based resistojet propulsion system for efficient orbital maneuvering, including low-energy transfers that leverage gravitational influences from Earth, the Moon, and the Sun. As the first CubeSat to attempt libration point orbit insertion through such miniature propulsion in this gravitational regime, the mission seeks to validate technologies for future deep space exploration by small satellites. A key secondary objective is to conduct ultraviolet imaging observations of Earth's plasmasphere to map its spatial distribution and study plasma dynamics, thereby contributing to improved understanding of space weather phenomena and radiation environments that affect satellites and human spaceflight. By positioning at the Earth-Moon L2 point, EQUULEUS enables global and sequential imaging of the plasmasphere from a vantage point beyond low Earth orbit, providing data on how solar activity influences plasma behavior and geomagnetic storms. This aspect of the mission supports broader efforts in space weather forecasting and mitigation of risks to space infrastructure. Additionally, the mission includes a tertiary objective to monitor lunar surface impacts and the dust environment, assessing potential hazards for upcoming lunar exploration initiatives. Observations of impacts on the Moon's far side will detect flashes produced by collisions, while measurements of dust particles in the Earth-Moon region aim to characterize their origins, distribution, and implications for safety. These investigations help evaluate the dynamic environment in space, informing protective measures for future missions. The overall mission duration is targeted to achieve at least six months of scientific operations following deployment and arrival at the L2 , allowing sufficient time for propulsion demonstrations and data collection across all objectives. This timeline aligns with the expected propellant lifespan, ensuring comprehensive testing of capabilities in deep space.

Design and Construction

The EQUULEUS CubeSat was a joint development project led by the Japan Aerospace Exploration Agency's () Institute of Space and Astronautical Science (ISAS) and the Intelligent Space Systems Laboratory (ISSL) at the . The initiative began in September 2016, with the mission selected as a secondary for NASA's Exploration Mission-1 (later renamed Artemis I) in April 2016, and the critical design review completed in June 2018. Assembly of the flight model was finalized in the months leading up to its launch on November 16, 2022. Key design challenges centered on miniaturizing and scientific instruments to fit within the constrained 6U form factor (approximately 10 cm × 20 cm × 30 cm), while ensuring operational reliability in the harsh deep space environment. Engineers addressed these by drawing on heritage from prior missions like and Hisaki, adapting structures for low-thrust trajectory control amid chaotic cislunar dynamics. A major innovation was the integration of the AQUARIUS water resistojet propulsion system, which combined trajectory correction, attitude control, and momentum dumping functions within standards, using non-toxic water propellant stored in a 1.2 kg tank. Cost efficiency was achieved through extensive use of (COTS) components, such as reaction wheels (XACT-50) and solar array paddles with gimbals, enabling rapid development while minimizing expenses compared to traditional deep space probes. The spacecraft underwent rigorous testing phases from 2021 to 2022, including ground vibration tests to simulate launch loads, thermal vacuum tests to replicate conditions, and electromagnetic compatibility assessments to ensure . These were primarily conducted at facilities affiliated with the and JAXA's ISAS, with additional support from the Kyushu Institute of Technology for specialized environmental simulations. The development team comprised researchers and students from , the University of Tokyo's ISSL, and collaborating institutions, with students leading subsystems such as attitude determination and control to foster hands-on . This collaborative approach, involving over 50 participants across academic and agency roles, emphasized and innovation in engineering.

Technical Specifications

Physical Characteristics

EQUULEUS is a 6U with deployed dimensions of 10 × 20 × 30 cm. The spacecraft has a wet mass of 10.3 kg, including 1.2 kg of water propellant. Its structure features an aluminum frame supporting deployable solar arrays and antennas, along with radiation shielding to protect electronics from the deep-space radiation environment. The power system relies on deployable solar panels that generate up to 15 W on average, supplemented by lithium-ion batteries to sustain operations during eclipses; the design emphasizes efficiency for the extended distances in space. Attitude control is achieved through the XACT-50 system with reaction wheels for three-axis stabilization (pointing accuracy of 0.1 degrees) and water thrusters for momentum management. Communication is handled by an X-band , with compatibility to NASA's Deep Space Network for deep-space operations.

Propulsion System

The EQUULEUS spacecraft is equipped with the AQUARIUS propulsion system, a water-based resistojet designed specifically for deep-space control on a 6U . AQUARIUS, standing for AQUA ResIstojet propUlsion System, operates through electrothermal vaporization, where deionized water is heated to produce steam that is then expelled through nozzles to generate thrust. This mechanism enables low-pressure operation below 100 kPa, utilizing waste heat from onboard communication components to vaporize the propellant efficiently. The system employs 1.2 kg of deionized as , stored in a bladder tank to avoid and ensure reliable feed under microgravity conditions. Nominal performance specifications for the Delta-V thrusters include a of 4 mN and a of 70 seconds, providing a total delta-V capability of up to 70 m/s, which supports critical from the initial to the Earth-Moon L2 point. On-orbit measurements (as of 2024) for reaction control thrusters show approximately 6 mN and 91 s . Eight thrusters are arranged in a configuration that allows for redundancy, , and integrated attitude control during burns, enabling precise three-axis stabilization and momentum management. AQUARIUS represents a pioneering innovation as the first deep-space propulsion system to use —a non-toxic, propellant—in place of hazardous alternatives like , thereby simplifying handling, reducing system complexity, and minimizing environmental risks. This approach not only aligns with sustainable propulsion goals but also demonstrates the feasibility of water resistojets for missions requiring moderate delta-V in .

Scientific Instruments

PHOENIX Imager

The PHOENIX (Plasmaspheric Helium ion Observation by Enhanced New Imager in eXtreme ultraviolet) instrument is an extreme ultraviolet (EUV) telescope designed for imaging Earth's plasmasphere from deep space. It operates at a wavelength of 30.4 nm, corresponding to the He II emission line, enabling the detection and mapping of helium ions (He⁺) that form a key component of the plasmasphere. This capability supports EQUULEUS's broader objective of investigating the cislunar space environment by providing remote observations of plasma dynamics beyond low-Earth orbit. The instrument's design emphasizes to fit within the constraints of a 6U , occupying less than 1U volume. It features a normal-incidence primary mirror with a 53 mm diameter, coated in / (Mo/Si) multilayers for selective reflection at 30.4 nm, paired with a metallic thin filter to block unwanted longer wavelengths. The is 69.4 mm, achieving a of 10.7° × 11.0°. Detection is handled by a photon-counting system using three-stage microchannel plates (MCPs) coupled to a resistive encoder, which amplifies incoming EUV photons and determines their positions via charge division across four electrodes. This setup provides a of approximately 0.19° per effective (0.18° × 0.13° at center), allowing global imaging of the plasmasphere when viewed from distances such as the Earth-Moon L2 point. Images are captured with a on the order of 1 hour, including integration times up to 1 hour, to build temporal sequences over several months. As of 2025, PHOENIX has successfully captured global images of the Earth's plasmasphere, validating its design for deep-space EUV observations. PHOENIX consumes a maximum of 1.8 W of power and has a total mass of approximately 0.54 kg, including the (0.48 kg) and board (0.06 kg). The miniaturized employ a mechanical shutter for exposure control and a high-voltage circuit (~2.5 kV) to drive the MCPs, ensuring efficient operation within the CubeSat's limited resources. Pre-launch calibration was conducted at JAXA's facilities, where focus was optimized using a CCD proxy detector and shim adjustments, verifying sensitivity to low plasma densities equivalent to 10⁴ ions/cm³ through simulated He⁺ emissions. A distinctive aspect of PHOENIX is its ability to construct three-dimensional maps of the plasmasphere by integrating sequential two-dimensional images taken from varying side-on perspectives as moves along its trajectory. This tomographic approach leverages the spacecraft's orbital dynamics to infer depth and density variations, providing insights into plasma refilling and processes without requiring onboard spectrometric resolution beyond the fixed 30.4 nm band.

DELPHINUS Camera

The (DEtection camera for Lunar impact PHenomena IN 6U Spacecraft) is a visible-light camera system aboard the nanosatellite, designed primarily to observe lunar impact flashes from the Earth-Moon L2 to assess fluxes in space. It consists of two redundant CCD cameras, each equipped with a 50 mm , F/1.4 lens, enabling detection of bright, short-duration flashes produced by impacts on the Moon's surface. The system also supports observations of near-Earth objects, such as potentially hazardous asteroids, during the spacecraft's cruising phase. Each camera features a 659 × 494 resolution with 7.4 μm square pixels, providing sensitivity across the 400–800 nm wavelength band for capturing visible-light phenomena. The deliver a narrow of approximately 5.6° horizontally and 4.2° vertically, optimized for resolving impact sites from distances up to 60,000 km. With a maximum of 60 fps and exposure times as short as 1/60 second, DELPHINUS achieves a of 4.5 Vmag (S/N = 2), sufficient to detect flashes from meteoroids as small as 10 cm in diameter. This capability allows for imaging, accommodating both intense impact flashes and fainter trails from smaller particles. An onboard FPGA-based image processing board performs real-time analysis using matching to identify and flag potential impact events, enabling data compression and selective downlink to manage the spacecraft's limited communication bandwidth. The system has a total mass of 0.64 kg (0.57 kg for the telescopes and 0.07 kg for the processing board) and consumes up to 4 W of power during peak operation. By providing space-based, weather-independent monitoring of the Moon's far side, contributes to evaluating hazards for future lunar missions.

CLOTH Detector

The CLOTH (Cis-Lunar Object detector within THermal insulation) is a compact dust impact sensor integrated into the EQUULEUS CubeSat to measure the flux of micrometeoroids and small debris particles in the cislunar environment. Designed as a hybrid instrument combining multi-layer thermal insulation (MLI) with piezoelectric sensing, CLOTH enables passive monitoring without requiring dedicated external hardware, conserving mass and power in the constrained 6U CubeSat platform. Its primary role supports mission objectives by providing in-situ data on particle hazards for future lunar exploration. The detector utilizes multiple layers of (PVDF) piezoelectric films embedded within the spacecraft's MLI on the +Y and -Y panels, generating electrical signals upon impacts that deform the films. This multi-layer setup facilitates time-of-flight measurements between PVDF layers, enabling reconstruction of particle trajectories and velocity vectors, while signal amplitude correlates with impact energy to estimate particle mass. The system detects particles larger than approximately 4 μm in at speeds exceeding 10 km/s, with a sensitivity threshold equivalent to impacts around 10^{-11} g, covering an effective area of 439 cm² across the two panels. CLOTH's electronics include a compact circuit board (100 × 100 mm) that processes and stores data, such as timestamps and signal profiles, for later downlink. The instrument weighs 0.06 kg total (0.03 kg for sensors and 0.03 kg for the circuit) and consumes a maximum of 1.0 W, allowing near-continuous operation throughout the mission. involved laboratory impact tests using JAXA's guns with soda-lime particles accelerated to speeds up to 6 km/s, validating detection efficiency and estimation accuracy.

Mission Execution

Launch and Deployment

EQUULEUS was launched on November 16, 2022, at 06:47:44 UTC from Launch Pad 39B at NASA's in , aboard the (SLS) Block 1 rocket as part of the uncrewed Artemis I mission. The served as one of ten secondary payloads selected to demonstrate deep-space technologies and science capabilities beyond . Prior to launch, EQUULEUS was delivered to NASA's Kennedy Space Center in July 2021 for processing and integration as a secondary payload on the Interim Cryogenic Propulsion Stage (ICPS) of the SLS, including environmental testing to ensure compatibility with the launch environment. The spacecraft, designated with COSPAR ID 2022-156E and SATCAT number 55905, was stowed in a dispenser mounted on the Orion stage adapter between the Orion spacecraft and the ICPS. EQUULEUS separated from the ICPS on November 16, 2022 (JST), approximately seven hours after liftoff, entering an initial following the burn. Within hours of separation, ground controllers confirmed the spacecraft's signal at 22:50 JST (13:50 UTC), indicating successful power-up, and initiated attitude stabilization using onboard magnetorquers to orient the solar arrays toward the Sun. Mission operations included redundant deployment mechanisms in the ICPS dispensers and a dedicated ground team prepared for real-time anomaly response, ensuring robust post-separation activities.

Trajectory and Operations

Following its deployment from the I on November 16, 2022, entered a aligned with the initial injection trajectory provided by the . The spacecraft then performed preliminary checkout operations, confirming nominal functionality of its systems during the initial phase. On November 21, 2022, executed a planned Earth-Moon flyby at an altitude of approximately 5,000 km, capturing images of the Moon's far side during the pass. To transition from the post-flyby trajectory to a stable around the Earth-Moon L2 point, EQUULEUS conducted a series of maneuvers using its AQUARIUS water resistojet system, beginning in late November 2022. These included three primary delta-V burns for insertion and eleven trajectory correction maneuvers, accumulating a total delta-V of over 17 m/s across more than 440 thruster firings. The spacecraft completed these major maneuvers to prepare for transfer to the target L2 . However, contact was lost on May 18, 2023, before insertion could be achieved. During this transit period, in February 2023, EQUULEUS imaged Comet C/2022 E3 (ZTF) using its onboard cameras, documenting the comet's passage against the stellar background. Mission operations progressed through distinct phases: commissioning from November to December 2022, focused on system verification and initial maneuvers; followed by a transit phase from January to May 2023, during which initial science observations, including imaging of the plasmasphere and Comet C/2022 E3 (ZTF), were conducted en route to EML2. A contingency mode was activated in response to an anomaly detected in May 2023, when the experienced attitude tumbling that limited generation. Recovery efforts involved uplink commands from ground stations, but contact was lost on May 18, 2023, marking the end of active operations. Despite the loss of contact, the mission achieved its primary engineering goals of demonstrating water-based propulsion for cislunar transfer, with scientific data analyzed and published as of 2025. Communications were facilitated by a network of ground stations, including JAXA's Usuda Deep Space Center in for primary tracking and NASA's Deep Space Network facilities, such as those in , , to support the deep-space link during transit and orbital phases. These assets enabled reliable uplink of commands and downlink of telemetry and imaging data throughout the mission duration.

Scientific Results and Status

Key Findings

The PHOENIX imager onboard EQUULEUS captured images of the Earth's plasmasphere in May 2023, revealing its three-dimensional structure and demonstrating contraction during geomagnetic storms, with the plasmapause shrinking by approximately 1 Earth radius on the night side. These observations highlighted significant density variations along magnetic field lines, providing new insights into plasma dynamics influenced by solar wind interactions. Published in April 2025 in the Journal of Geophysical Research: Space Physics, these results marked the first CubeSat-based ultraviolet imaging of the plasmasphere from a cis-lunar vantage point, enhancing space weather forecasting models. DELPHINUS conducted observations during lunar flybys in the cruise phase. The CLOTH detector recorded events in the region during the cruise phase. EQUULEUS's AQUARIUS water resistojet system enabled successful insertion into the Earth-Moon L2 , validating thruster efficiency. These findings from PHOENIX and the propulsion demonstration underscore 's contributions to understanding environmental hazards and Earth's magnetospheric responses.

Current Status and Legacy

As of 2025, the spacecraft remains in a tumbling mode that began in May 2023, characterized by intermittent power generation and no successful communication since May 18, 2023. This loss of contact followed key operational anomalies during its trajectory to the Earth-Moon L2 point, limiting further real-time data collection but preserving a substantial of observations. Recent developments have focused on post-mission , with archived reprocessed in 2024 and 2025 to enhance scientific yield. A notable advancement came in a 2025 JAXA-supported publication detailing PHOENIX imager observations from May 2023, which provided global and sequential images of the Earth's plasmasphere, confirming established models of its structure and dynamics. Ongoing efforts continue to apply this data toward forecasting, integrating it with models to predict plasma distributions and their effects on operations. EQUULEUS's legacy centers on its demonstration of green for nanosatellites, utilizing a water resistojet system (AQUARIUS) that achieved the world's first successful deep-space control with an environmentally benign . This innovation has influenced subsequent small satellite designs, particularly for NASA's and the , by validating low-thrust maneuvering in space for cost-effective deep-space exploration. The mission's archived dataset, made publicly available by , supports broader research into radiation environments, while its development by the University of Tokyo and provided hands-on training for over 20 students in deep-space operations and inspired follow-on concepts for L2-point monitoring. Looking ahead, EQUULEUS data contributes to radiation hazard predictions essential for the emerging lunar economy, enabling safer human and robotic activities beyond . The mission's overall cost-benefit analysis underscores the viability of low-budget deep-space technologies, achieving significant scientific and engineering milestones with a 6U platform at a fraction of traditional mission expenses.

References

  1. https://www.eoportal.org/satellite-missions/equuleus
  2. https://www.isas.jaxa.jp/en/topics/004046.html
  3. https://global.jaxa.jp/press/2022/11/20221126-1_e.html
  4. https://www.spiedigitallibrary.org/conference-proceedings-of-spie/13546/135460I/EQUULEUS--Artemis-1-CubeSat-to-successfully-demonstrate-trajectory-control/10.1117/12.3061014.pdf
  5. https://global.jaxa.jp/about/president/presslec/202211.html
  6. https://ieeexplore.ieee.org/abstract/document/9076200
  7. https://cosmos.isas.jaxa.jp/omotenashi-equuleus-the-tiny-spacecraft-onboard-the-worlds-most-powerful-rocket/
  8. https://digitalcommons.usu.edu/cgi/viewcontent.cgi?params=/context/smallsat/article/4399/&path_info=SSC19_WKV_04.pdf
  9. https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2024JA033389
  10. https://ntrs.[nasa](/page/NASA).gov/citations/20220003814
  11. https://digitalcommons.usu.edu/context/smallsat/article/4109/viewcontent/SSC18_VII_05.pdf
  12. https://global.jaxa.jp/projects/activity/int/topics.html
  13. https://ui.adsabs.harvard.edu/abs/2024cosp...45..340A/abstract
  14. https://pale-blue.co.jp/news/299/
  15. https://www.nasa.gov/humans-in-space/international-partners-provide-science-satellites-for-americas-space-launch-system-maiden-flight/
  16. https://ui.adsabs.harvard.edu/abs/2020JAnSc..67..950O/abstract
  17. https://www.sciencedirect.com/science/article/pii/S0094576524006921
  18. https://www.researchgate.net/figure/Configuration-model-of-the-thermal-vacuum-test-of-EQUULEUS-FM-Shows-the-Thermal-Desktop_fig3_368601524
  19. https://arkedgespace.com/en/news/series-exhaustive-report-on-arkedge-space-by-minoru-otsuka-first-article-searching-for-the-secret-of-the-mass-produced-6u-satellite
  20. https://www.eoportal.org/satellite-missions/aqt-d
  21. https://www.jstage.jst.go.jp/article/tastj/16/5/16_427/_pdf
  22. https://digitalcommons.usu.edu/smallsat/2023/all2023/95/
  23. https://www.jstage.jst.go.jp/article/tastj/17/3/17_17.315/_pdf
  24. https://www.nasa.gov/mission/artemis-i/
  25. https://global.jaxa.jp/press/2022/11/20221117-1_e.html
  26. https://www.nasa.gov/reference/artemis-i-2/
  27. https://digitalcommons.usu.edu/smallsat/2023/all2023/52/
  28. https://www.nasaspaceflight.com/2022/11/artemis-i-cubesats/
  29. https://digitalcommons.usu.edu/cgi/viewcontent.cgi?article=5578&context=smallsat
  30. https://digitalcommons.usu.edu/cgi/viewcontent.cgi?article=5621&context=smallsat
  31. https://www.space.com/japanaese-moon-cubesat-sees-green-comet-C2022E3-video
  32. https://digitalcommons.usu.edu/cgi/viewcontent.cgi?article=5827&context=smallsat
  33. https://digitalcommons.usu.edu/context/smallsat/article/5671/viewcontent/SSC23_P1_09.pdf
  34. https://www.nanosats.eu/sat/equuleus.html
  35. https://spie.org/Publications/Proceedings/Volume/13546
  36. https://www.researchgate.net/publication/334111997_Mission_Analysis_for_the_EM-1_CubeSats_EQUULEUS_and_OMOTENASHI
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