Minimize CanX-7

CanX-7 (Canadian Advanced Nanospace eXperiment-7)

CanX-7 is a deorbiting nanosatellite demonstration mission of UTIAS/SFL (University of Toronto Institute for Aerospace Studies/Space Flight Laboratory). The CanX-7 satellite is being developed in direct response to the growing problem of space debris in the highly dense LEO (Low Earth Orbit). The primary mission of the CanX-7 mission will be to demonstrate a deorbiting technology suitable for a CubeSat platform. The deorbiting technology will be a modular drag sail that can be integrated to the outside of a satellite and therefore provide minimum intrusion to the internal electronics and payloads.

The overall goal is to limit the orbital life of a nanosatellite to the 25 year recommendation of the IADC (Inter-Agency Space Debris Coordination Committee), issued in 2007.

- Two protected regions (LEO, GEO)

- LEO guidelines ⇒ deorbit within 25 years from EOM (End of Mission).

Unfortunately, for microsatellites (< 100 kg) and nanosatellites (< 10 kg), that are ideal for responsive and short space missions, none of the active deorbiting approaches have sufficient technological maturity to be used consistently and reliably for this class of mission. Indeed, none of the technologies have successfully flown and served as a deorbiting device. Due to the energies and/or time required for deorbiting, there is a strong preference for passive deorbiting devices, i.e. devices that do not require that the satellite remain operational for deorbiting. Passive approaches include tethers and drag sails. 1)


Figure 1: Schematic view of the CanX-7 nanosatellite with the deployed drag sail (image credit: UTIAS/SFL)

The CanX-7 mission involves a nanosatellite that will incorporate a lightweight, compact, deployable drag sail under development at SFL. The mission is funded by DRDC (Defence R&D Canada), Ottawa, NSERC (Natural Sciences and Engineering Research Council) of Canada, and COM DEV Ltd. The mission will demonstrate the drag sail's customizability, modularity, stowability and effectiveness at achieving the deorbiting requirements of the IADC. The results will then be used to create a low cost, modular, and customizable deorbiting device for nanosatellites and microsatellites in low Earth orbit, thus alleviating the programmatic and technical risk to space missions when using satellites of this class.

The goals of the CanX-7 mission are: 2)

• Demonstrate a deorbit device for CubeSats

• Validate post-deployment deorbit and attitude models

• Operate a secondary payload, namely an aircraft ADS-B (Automatic Dependent Surveillance - Broadcast) receiver, provided by COM DEV Ltd. The objective is to demonstrate whether a spaceborne ADS-B technology can be used to provide a source of continuous surveillance for commercial aviation.


Deorbiting methods:

For most small satellites in LEO (Low Earth Orbit), the only viable means of achieving end-of-life disposal is to deorbit. In some cases, the inherent characteristics of a satellite (i.e. its ballistic coefficient) and its altitude are such that the satellite will naturally deorbit within 25 years or less. However, in many cases, because of either high ballistic coefficient or relatively high altitude, deorbiting must be accomplished using a dedicated system. Several approaches to deorbiting exist, and can be broadly categorized as either active (i.e. requiring continuous operation, usually steering) or passive (i.e. requiring only deployment to effectively deorbit, with no attitude control needed). 3)

Active methods: Active methods of deorbiting require attitude control beyond the end of spacecraft life, by definition. Maintaining such attitude control either requires the satellite attitude control system to be functioning properly (which cannot be assured at end-of-life) or necessitates an additional (integral) deorbiting attitude determination and/or control system, which increases complexity and cannibalizes precious mass and volume (both of which are at a premium in small spacecraft). Examples of active approaches include propulsion systems and controlled (steered) solar and drag sails.

The most traditional active method for deorbiting is to use a propulsion system. However, the problem with propulsive deorbiting is that you must be able to point the thruster—which, as described, implies the ability to control (or at least determine) the attitude of the satellite, which cannot be assured beyond EOL. Notwithstanding this consideration, propulsive deorbiting also requires additional propellant, which drives spacecraft mass. For larger satellites that already require high-performance orbital maneuvering systems, the additional ΔV to deorbit may be a manageable penalty, but for smaller satellites the added mass, testing and handling complexity can be deal breakers.

Controlled solar or drag sails have been proposed, in which the sail orientation is constantly controlled relative to either the solar vector for steered sailing or the satellite velocity vector to maximize drag. These approaches have the same drawback as using propulsive techniques, in that they must be continuously controlled—however, in the case of active solar or drag sails, instead of needing to maintain attitude for several minutes to execute the deorbiting maneuver, continuous attitude control may be required for months or even years! This is a significant burden to impose on a mission—particularly a small space mission, whose operations budget may have long since been exhausted at end of mission.

For these reasons, active approaches that require post-EOL control are viewed less favorably than passive methods for single- or multi-smallsat missions.

Passive methods: In contrast to active approaches, passive techniques do not require the satellite to remain operational during the deorbiting phase. Passive methods require no active control, relying only on natural perturbations and forces to accomplish deorbiting, and are therefore intrinsically much simpler than active methods. Examples of passive methods include drag sails, balloons, and ribbons or tethers. Passive systems are generally viewed here as preferable to active systems, given their “turn-key” characteristics—once a passive system is activated, it requires no long-term control or maintenance.

Tethers have often been advocated as promising deorbiting technologies for small satellites. However, such devices are usually extremely large when deployed (often hundreds of meters), have complex deployment (and deployed) dynamics, and have a demonstrated propensity to tangle and sever. Alternative concepts, such as inflatable balloons or inflatable drag sail devices, require the use of pressurized gas, which is problematic both for launch and for long-term leak-free storage. Inflatables can also be critically vulnerable to MMOD (Micrometeorite and Orbital Debris) punctures, which is problematic for worst-case deorbiting durations. Techniques for rigidizing inflatables following deployment to address MMOD concerns have been proposed, but add complexity and testability challenges.

Contrary to the above options, passive, mechanically-deployed drag sails offer a promising approach to deorbiting. Such drag sails are passive, requiring no attitude control—decidedly preferable to active methods—and they can be deployed using only stored mechanical energy, without pressurants or pyrotechnics.

Deorbiting Device “Killer Trades”: A comparison of common deorbit approaches discussed for small LEO spacecraft is provided in Table 1, in which the so called “killer trades” of each option—the driving requirements, constraints and risks inherent in each—are summarized. Of the options presented in Table 1, mechanically-deployed drag sails are viewed as most promising for deorbiting nano- and microsatellites below a certain size, provided the orbit altitude is sufficiently low to allow drag-based deorbiting. Mechanically-deployed drag sails offer the benefits of small characteristic dimension, no attitude control requirements, and no pressurized gasses, instead using only their own stored mechanical energy for deployment. For these reasons, the development of a drag sail-based deorbiting technology has been selected by SFL for CanX-7, as well as future missions.

Deorbit approach


Killer trades



- Requires high total impulse (challenging for small satellites)
- Requires active pointing / steering
- Requires long-term propellant storage

Solar sail


- Requires active pointing / steering
- Susceptible to jamming
- Susceptible to MMOD degradation

Electrodynamic or drag tether


- Large characteristic dimension
- Deployment complexity
- Susceptible to jamming / tangling
- Inclination-limited (electrodynamic tethers)

Inflatable drag device


- Requires long-term, leak-free storage of compressed gas
- Altitude-limited
- Susceptible to jamming
- Susceptible to MMOD degradation / puncture

Mechanically-deployed drag device


- Requires storage of mechanical energy
- Altitude-limited
- Susceptible to jamming
- Susceptible to MMOD degradation

Table 1: Summary of deorbiting techniques for LEO satellites




The CanX-7 nanosatellite will utilize the highly capable and proven 3U form factor. It will use passive thermal control and electronics currently used by the GNB (Generic Nanosatellite Bus) satellite series as several components used on the CanX-2 nanosatellite are no longer available. The bus size is 10 cm x 10 cm x 34 cm. The estimated mass budget is ~3.6 kg. 4) 5) 6) 7)


Figure 2: Illustration of the CanX-7 bus (image credit: UTIAS/SFL)

ADCS (Attitude Determination and Control Subsystem): Use of a 3-axis magnetometer (with flight heritage on AISSat-1) and panel currents for attitude determination. For attitude control, CanX-7 will utilize a set of three orthogonally printed magnetorquers, custom designed at SFL, each of which produces a maximum dipole of 0.2 Am2. The printed torquers will be used on AISSat-2, which is to be launched prior to CanX-7, and therefore will have earned flight heritage when CanX-7 is ready to launch. The torquers will be used to detumble the satellite after ejection and also in case of a spin up. They will also be used to orient the satellite in a favorable attitude prior to sail deployment to minimize any impact on communications.

EPS (Electrical Power Subsystem): The EPS is a DET (Direct Energy Transfer) system with PPT (Peak Power Tracking) functionality. A centralized PDU (Power Distribution Unit) based on the SFL Modular Power System provides switched power to spacecraft loads and collects power system voltage, current and temperature telemetry. EPS uses 8 body-mounted triple-junction solar strings. A Li-ion battery of 4.8 Ah capacity provides power during orbital eclipse periods. A battery heater is included to keep the battery within its operational limits. The battery is attached to a battery thermal control board located on the BCDR (Battery Charge/Discharge Regulator). The BCDR, in addition to monitoring the temperature of the battery, sets the operating voltage of the solar arrays, monitors battery voltage and regulates the charge and discharge current to the batteries.

The CanX-7 power demands range between 0.5-5 W with an average of 3 W of power generated by the solar array. The main power bus operates at 4.2 V which can be used directly by the loads without additional serial regulation.

C&DH (Command and Data Handling) subsystem: Use of generic nanosatellite bus electronics; single housekeeping microprocessor. The C&DH is responsible for communicating with the rest of the subsystems and relaying information between them.

TCS (Thermal Control Subsystem): The TCS is passive. This will be accomplished through thermal tapes, material selection and component layout. The main purpose of the thermal control subsystem is to keep satellite and its components within a temperature range acceptable for proper functionality. Heaters, as active measures for thermal control, are only used as a last resort for essential components unable to meet this temperature requirement through passive means.

TT&C (Telemetry Tracking and Command): Use of generic nanosatellite bus electronics; the uplink is provided in UHF band at 4 kbit/s, the downlink uses S-band . The UHF uplink uses an antenna system consisting of four canted monopoles that will deploy after ejection from the XPOD. This arrangement and the deployable mechanism, providing near omnidirectional coverage, are well established as they have been used on CanX-2. The S-band transmitter will provide the downlink capability for CanX-7 by utilizing two patch antennas. They are mounted on opposite faces of the satellite to provide near omnidirectional coverage over the full sphere of the satellite. The S-band transmitter nominally operates between 32 kbit/s and 1 Mbit/s. - Use of the existing SFL ground station in Toronto, Ontario, for spacecraft control and data reception.


Figure 3: Close-up of the deployed CanX-7 nanosatellite (image credit: UTIAS/SFL, Ref. 6)

Spacecraft form factor (3U CubeSat)

10 x 10 x 34 cm

Mass (including margin)

4 kg

Attitude control

±10º (2σ)

Attitude pointing mode

LMF tracking

Power generation
Battery capacity
Nominal bus voltage
Peak payload power

1.8 – 6.0 W
4.8 Ah
4.2 – 5.5 VDC
4.2 W

Command uplink
Telemetry downlink
Onboard data storage

UHF, 4 kbit/s
S-band, 32 kbit/s - 1 Mbit/s
Up to 1 GB

Bus operational temperature range

-20ºC to +60ºC

Launch interface

XPOD triple

Table 2: Overview of the CanX-7 nanosatellite parameters


Figure 4: Expanded view of the CanX-7 nanosatellite general layout (image credit: UTIAS/SFL)


Launch: A launch of CanX-7 as a secondary payload is planned for 2014/2015. Launch arrangements are in progress.

Orbit: Maximum initial altitude of 800 km.

Use of SFL's XPOD (eXperimental Push Out Deployer) for ejection of the CanX-7 nanosatellite into orbit. During launch, the drag sails and the deployables are in a stowed configuration. Once in orbit, CanX-7 will operate a secondary payload provided by COM DEV Ltd. for approximately six months.

DDS (Deployment Detection Subsystem): The objective of the DDS is to detect and verify the proper deployment of the drag sail. The DDS includes a COTS camera.

This drag sail payload is intended to be deployed at the end of a six-month phase of secondary payload operation. Sail deployment will be initially confirmed via on-board telemetry and images, while deorbiting performance will be verifiable within weeks following deployment. In order to provide a path towards adaptation on multiple satellite platforms, the CanX-7 drag sail payload is designed to be modular and scalable, consisting of four individual drag sail modules, each deploying its own independent sail. A total sail area of approximately 5 m2 is achieved with the full subassembly deployed.

CanX-7, assuming a 2014 launch to an altitude of 800 km. Figure 5 indicates that the CanX-7 spacecraft will deorbit within 5 to 10 years of initial deployment at its maximum design altitude, depending on LTAN and final spacecraft magnetic moment, which is uncontrolled on CanX-7 (Ref. 3).


Figure 5: Range of deorbit trajectories for CanX-7 (image credit: UTIAS/SFL)



Experiments: (Drag Sail, ADS-B)

Drag Sail:

The selected drag technology to be demonstrated on the CanX-7 mission must be capable of deorbiting cubesats within the IADC required timeline. Several devices that can be utilized as deorbiting devices for small satellites include: rockets, inflatables, rigidizable inflatables, electrodynamic tethers and drag sails. Several requirements that the drag device had to satisfy included being a passive device that does not require an active satellite to deorbit, require no high pressurized containers to deploy which could potentially complicate obtaining a launch, and be testable in a 1-g environment to allow for testing prior to flight (Ref. 4).

The drag sail was concluded to be the proper fit for deorbiting cubesats. Other potential methods had several complications or didn’t meet one or more of the requirements, making the development or inclusion a higher risk to the demonstration mission.

CanX-7 will accomplish its main objective by employing four deployable drag sails, each stowed within its own module, to demonstrate the ability to deorbit at different rates while maintaining some redundancy in the deorbiting system for the purpose of experimentation. These drag sail modules have either superior or competitive packaging and mass efficiency to state-of-the-art solar sails; and even at the demonstrator scale represent a sail design for cubesats, instead of a sail that simply fits inside a cubesat, while precluding any other useful payload. CanX-7 will also be used to validate deorbit models to aid in the deorbiting analyses of future SFL satellites.

At the end of mission operation, the drag sail modules will be deployed in order to deorbit the satellite, as shown in Figure 6.

By demonstrating the success of the deorbiting solution on-orbit, the drag sail will earn flight heritage, which will enable easier adoption into future missions. In using this deorbiting technology (or larger upgrades) on future SFL satellites, the laboratory is helping to mitigate the global problem of orbital debris.


Figure 6: CanX-7 spacecraft with deployed drag sail (image credit: UTIAS/SFL)

Lifetime analysis:

The drag sail device is required to deorbit its host spacecraft within 25 years to meet IADC guidelines. It was sized with the aim of deorbiting a reference spacecraft which is larger than CanX-7. Sizing for a larger spacecraft increases the versatility of the drag sail and will also facilitate a rapid (much less than 25 year) demonstration of the deorbit technology during the CanX-7 mission. Early on in the development of the drag sail, an area of 4.0 m2 was chosen to be sufficient to meet both of these objectives (Ref. 4).

Various analyzes were completed in order to determine the required drag area to deorbit within the set period of 25 years. The drag sail was chosen as the deorbit device to demonstrate on the CanX-7 mission and therefore the expected lifetime and performance for this device had to be analyzed prior to beginning the detailed design of the drag sail device.

Methodology: A combination of fixed-attitude and variable-attitude simulations were performed in order to evaluate the deorbit performance of the CanX-7 drag sail. The fixed attitude simulations were performed using the deorbit toolbox in STK (Satellite Tool Kit) and served as a baseline against which the variable-attitude simulations could be compared. The variable-attitude simulations were performed using a quasi-coupled, orbit-attitude dynamical numerical integrator using MATLAB/SIMULINK. The term ‘quasi’ here refers to the fact that fully-coupled attitude orbit simulations were not performed. Instead, the approach was to perform short-term, variable attitude simulations for many fixed orbits; the results from each of these static orbit cases were then combined to evaluate the overall performance of the drag sail over the deorbit lifetime.

Constant-Attitude (STK) Simulations: An analysis was carried out to determine the required drag area of the sail in order to meet the lifetime requirement. STK software was used to model the satellite with the HPOP (High Precision Orbit Propagator). STK was used to get an idea of lifetimes for different sized satellites.

The STK simulations for the CanX-7 satellite were completed at several different altitudes, chosen based on the altitudes of current and future satellite missions at SFL, as well as with drag coefficients of 2.2 and 2.4. The typically accepted value of 2.2 was found not to be representative of on-orbit conditions and 2.4 was found to be more realistic. For comparison, deorbit lifetime results using both drag coefficients are shown in Figure 7. The lifetimes for the CanX-7 satellite are well below the IADC recommendation of 25 years to facilitate a potentially quicker deorbit or to act as functional redundancy.

Variable-Attitude Simulations: The STK simulations described in the previous section do not account for the time-varying nature of the spacecraft’s projected drag area. For on-orbit satellites, the instantaneous projected area will be a function of attitude. Even with an aerodynamic drag device which is designed to take advantage of the “shuttle cock” effect, achieving an aero-stable configuration is unlikely at altitudes above 650 km and perhaps even lower depending on the spacecraft and sail properties. This can be realized by examining Figure 8 which shows the upper limits of disturbance torque magnitudes expected for a small satellite in LEO.

Note that in Figure 8, a band is shown for each disturbance; the band captures the range of maximum torque which is dependent on various spacecraft and environment parameters. It can be seen that above 600 to 650 km the geomagnetic disturbance due to the inherent residual magnetic dipole moments of the spacecraft will dominate. It is not until the altitude drops to around 450 km ,that the aerodynamic disturbance becomes dominant and aero-stabilization could be reasonably expected. This is especially difficult for highly asymmetric spacecraft such as CanX-7, which has a wide range of projected areas, varying from 0.034 m2 when the drag sail is edge-on to the velocity vector, to a maximum of 4 m2 when the drag sail is perpendicular to the velocity vector. In a word, relying on deorbit analyses which assume constant drag area could give very misleading results. It is therefore necessary to account for the attitude dynamics when assessing the deorbit performance.


Figure 7: Required drag area to deorbit from different altitudes (image credit: UTIAS/SFL)

Decoupling the Attitude and Deorbit Dynamics: Performing fully coupled attitude and deorbit simulations is impractical due to the very different associated timescales. To adequately simulate attitude dynamics, the required maximum time step is on the order of seconds. Propagating for a full 25 year deorbit period would require on the order of at least 100 million integration steps. Furthermore, due to the uncertainty in final spacecraft and orbit parameters, many such simulations must be performed to ensure the design meets the requirements in all expected configurations.

An alternative approach was developed which effectively decouples the orbit and attitude simulations. The methodology uses short-term (on the order of 10’s of orbits) attitude simulations to evaluate the deorbit performance in individual slices of an entire solar cycle (approximately 11 years). The results from many of these slices are then combined appropriately to arrive at a result which approximates the deorbit performance for the entire solar cycle. The output of this analysis is referred to as the WSCEA (Whole Solar Cycle Effective Area) and can be compared directly against the constant-area simulations performed using STK to estimate the deorbit lifetime.


Figure 8: Maximum attitude disturbance torques experienced by the CanX-7 spacecraft (image credit: UTIAS/SFL)

Design of Experiments: The primary system parameters which affect the WSCEA are: orbit altitude, inclination and LTAN (Local Time at the Ascending Node); spacecraft residual magnetic dipole; spacecraft mass MOI (Moment of Inertia), configuration of drag sail, and the inherent damping of the spacecraft (due to structural damping, magnetic eddy current damping, etc.). While some of these parameters can be estimated to a reasonable accuracy during the design and development of the spacecraft (i.e., spacecraft MOI and configuration of the drag sail), the rest will not be defined until the spacecraft is fully assembled and the operational orbit is selected. For this reason, a design of experiments was developed which enveloped all of the possible configurations of spacecraft and orbit.

Orbit and Spacecraft Configurations: The considered orbits were sun-synchronous orbits (SSO) with an altitude of 800 km which is the worst case from a deorbit performance point-of-view (note that the drag sail is designed to deorbit spacecraft with altitudes of 800km or less). Although the drag sail is designed to work within any near polar orbit (with inclinations between 80º and 100º), only SSO were analyzed since they envelope the rest in terms of deorbit performance; if the orbit is not sun-synchronous, the performance tends to average out over time, having weaker performance with LTANs near 6:00 or 18:00 hrs, and increased performance with LTANs near 12:00 or 24:00 hrs. By considering orbits with constant LTANs, the upper and lower limits can be put on the expected performance. Table 3 shows a summary of the considered orbits.


Considered values


800 km


80º, 90º, 100º

Constant LTAN (Local Time at the Ascending Node)

3:00 hr, 6:00 hr, 9:00 hr, 12:00 hr, 15:00 hr, 18:00 hr, 21:00 hr, 24:00 hr

Table 3: Considered orbits for the design of experiments

Aside from inherent damping, the residual magnetic dipole moment of a satellite is the spacecraft-dependent parameter that has the greatest effect on the deorbit performance, because it has the greatest impact on spacecraft attitude during periods when solar disturbances are low. To understand the sensitivity of deorbit performance to the magnitude and orientation of the residual dipole, seven spacecraft configurations were considered that envelope the expected design range for the CanX-7 spacecraft. Table 4 summarizes the considered configurations; the direction refers to the angle between the sail plane and the residual dipole of the spacecraft, when the dipole points in a direction parallel to the drag sail plane the angle is 0º.

Residual magnetic dipole moment

Spacecraft configuration








Magnitude [Am2]




Angle between drag sail plane and residual dipole






Table 4: Considered spacecraft configurations

Results: The results from the design of experiments are displayed in Figure 9 which shows the WSCEA (Whole Solar Cycle Effective Area) for orbits with altitude 800 km, inclination of 100º, and various LTANs; the results for other inclinations follow the same trend.


Figure 9: WSCEA results for inclination of 100º (image credit: UTIAS/SFL)

Deorbit lifetime for the CanX-7 mission: In general, the results indicate that the WSCEA for the CanX-7 mission will be between 1.2 and 3.0 m2 with an average of about 2.1 m2 (at the maximum initial altitude of 800 km). Comparing this to the results from the constant-area lifetime simulations shown in Figure 9, the deorbit lifetime from 800 km for the CanX-7 spacecraft will be between 4 and 10 years depending on the magnetic properties of the spacecraft. The 4 m2 SFL-designed drag sail is therefore sufficient to meet the deorbit requirements.


Drag Sail Design:

The CanX-7 drag sail payload design is modular, consisting of four separate sail modules which combine to form a subassembly that fits within the constraints of the 3U CanX-7 bus. Each individual sail in the subassembly can be released individually and commanded directly over the spacecraft uplink. The drag sail modules are wedge-shaped, and each deploys a trapezoidal sail supported at its corners. Figure 10 shows a single drag sail module in its pre-deployed state, while Figure 11 shows an exploded view. For CanX-7, the four modules are assembled in two decks, and mated to each other and the spacecraft with two interface brackets. This complete assembly is shown in Figure 12 (Ref. 3).


Figure 10: Single drag sail module (image credit: UTIAS/SFL)


Figure 11: Drag sail expanded view (image credit: UTIAS/SFL)


Figure 12: Drag sail subassembly (four modules, 3U configuration), image credit: UTIAS/SFL

Sail Module Electronics: The sail module electronics are responsible for processing deployment commands sent from the ground; driving the release mechanism heater; and collecting telemetry on deployment confirmation and the extent of deployment. The sail is deployable only via ground command on CanX-7, requiring two separate ARM and FIRE commands sent in sequence to be initiated.

At the payload subassembly level, each drag sail module is connected to three multi-drop busses: a power bus; a telemetry bus (asynchronous serial) from the housekeeping computer; and a command bus (synchronous serial) from the UHF receiver. Figure 13 shows a high-level sail module interconnection diagram, in which each sail module is shown on the power and data busses that run through the sail subassembly.

At the individual drag sail module level, each unit contains its own compartmentalized telemetry and drive electronics, and the operation of each module is independent from adjacent modules. Each drag sail module contains:

• A microcontroller connected to the spacecraft’s housekeeping computer and UHF receiver, which accepts commands to deploy the sail and transmits telemetry when instructed

• A driver circuit to monitor and activate the release mechanism heater

• A microswitch to detect whether the sail door is closed or open

• A Hall effect sensor to monitor motion of the boom reel.

The sail modules receive ARM and FIRE deployment commands directly from the spacecraft command uplink. The sail modules also receive commands and transmit telemetry to the spacecraft housekeeping computer through a dedicated serial interface.


Figure 13: Block diagram of the drag sail payload electrical interconnection (image credit: UTIAS/SFL)


The drag sail modules are conceptualized to be compatible with the three standard UTIAS-SFL-made spacecraft buses as shown in Figure 14. Each drag sail module is triangular in shape, and deploys a 1 m2 triangular sail formed from metalized polymer film supported at each corner (Figure 15). Four modules are deployed to form a complete square sail. The plane of the drag sails is offset from the spacecraft’s center of mass, creating the potential for an aero-stable attitude at low altitudes.


Figure 14: Four sail modules integrated with CanX-7 (left), GNB (middle), and NEMO (right) spacecraft (image credit: UTIAS/SFL)


Figure 15: Drag sail module, deployed (image credit: UTIAS/SFL)

Module integration and shape: The modular approach to the design of the CanX-7 deorbiting payload allows for integration with any compatible spacecraft without substantially altering the existing bus design. In comparison, an integrated approach in which the drag sail components are housed by the existing bus structure would demand increased engineering effort beyond the scope of the mission for which the sail is designed. However, this choice means that opportunities for platform-specific optimization are traded for cross-platform compatibility.

The adoption of several modules, as opposed to a single module, creates more options for placement on irregularly shaped spacecraft. For integration with a cubesat bus, the modules are stacked atop one of the forward or aft square faces. Stacking the modules or covering them with solar panels (Figure 16, top left) eliminates the possibility of accessing their interior from the top or bottom face. This imposes a design constraint whereby the deployment mechanism and sail stowage solution must allow for access from the side panels for rewinding and repacking during testing of the fully-integrated spacecraft.

Integration with the other busses is more straightforward. For integration with a larger cube-shaped bus such as the Space Flight Laboratory’s GNB, the modules are simply mounted on one of the exterior faces, and covered with a solar panel (Figure 16, top right). On the NEMO bus the multi-module approach is particularly convenient, because it allows four modules (or more) to be mounted around the perimeter of a bus face, without requiring the whole face to be free of protrusions that might obstruct the sail’s deployment (Figure 16, bottom).

The choice of a triangular sail module shape allows the booms to follow a straight path as they exit the module, which results in less resistance to tape motion than curved tape paths. The resulting footprint of the reel and straight tape paths lends itself to placing two triangular modules side-by-side to form a square, which conveniently matches the cross section of a CubeSat. Therefore, within the same volume both modules may be twice the height while using half the footprint of a square module. This height is used to accommodate ¾ inch-wide tape springs, which are sufficiently stiff to deploy the sail onto a smooth flat surface, and in certain orientations to support their own weight in a 1 g environment.


Figure 16: Drag sail module integration on a triple cubesat (top left), GNB (top right), and NEMO (bottom) bus (image credit: UTIAS/SFL)

Deployment Mechanism: The CanX-7 payload works on the basic principle of stored mechanical energy. Stored mechanical energy is perceived to be more reliable than electrically driven deployment and require less capability from a spacecraft’s power system, which may become unreliable or have diminished output at the end of its life.

The use of tape springs wound on a reel arose out of a desire to use COTS parts for simplicity and rapidity of prototyping. A reel is the natural shape for storing tape springs, and is used in similar deployable structures such as the Rolatube bistable reeled composite, lenticular cross section booms, TRAC boom, and STEM–derived booms. Conveniently, tape springs are capable of not only forming the stiff boom structure, but of providing the energy for their own deployment as well.

The use of the tape springs as the source of energy for deployment means that they must be stored in an enclosure that converts the uncoiling motion of the tape springs into linear motion of the booms. The sail module’s circular tape enclosure serves this purpose, and is formed from rollers which exert little resistance against the rotational motion of the coiled tape springs.

The tapes are prevented from deploying by restraining them at the free ends that form the boom tips. This is accomplished by means of a door. The door will be opened by a torsion spring, and held closed by a pin that will positively prevent the door from opening due to vibration during launch. This “door release mechanism” will be disengaged to trigger deployment.

A piece of ground support equipment will serve as a separate “rewind mechanism” used to retract the booms into the sail module, when the interior of the module is inaccessible. The rewind mechanism will consist of an external rewind gear that will interface with a set of gear teeth located around the perimeter of the reel. A ratchet will prevent rotation of the external gear in the deployment direction.

Boom material and performance: Unlike a solar sail, a drag sail needs only to present frontal area in the ram direction without any need for the membrane to be made flat by holding it in tension. Therefore, the open section of tape-springs that otherwise makes them unsuitable for supporting longitudinal compression loads is acceptable for this application, in which they are loaded primarily in bending by the extremely small drag force. To ensure that the tape springs are loaded in a direction in which they resist bending loads, the booms are oriented such their convex side faces the sail. Each outboard corner of the triangular sail is attached to the boom tips by a pair of flexible lines that connect to the two corners of the boom section (Figure 17).


Figure 17: Sail attachment and boom deformation under Earth-gravity (image credit: UTIAS/SFL)

The magnitude of the drag load varies with the projected area of sail in the velocity direction. The greatest drag load occurs when the sail is face on to the velocity vector, as might occur when the spacecraft aero-stabilizes at lower altitudes. Under a drag load roughly perpendicular to the unloaded plane of the sail, the line closest to the direction in which the load is applied carries the majority of the sail tension, which imparts a moment to the boom tip that causes the entire boom to twist such that the concave side of the boom faces the direction of load application. On the ground, the result of this mounting arrangement is that the booms deform to a shape in which they are sufficiently strong to withstand the combined load of the sail’s mass and the boom’s mass. On orbit, the sail will be subjected to vastly smaller loads: At 300 km (the lowest altitude at which the sail is required to operate) the distributed drag force on each sail segment will be approximately 2 mN, which is more than 100 times less than mass of the sail film alone.

Sail Material and Stowage: The sail will be formed from metalized polymer film. Metalization is employed to protect the polymer from atomic oxygen and UV radiation. Ideally, the sail material would be transparent to eliminate disturbance torques from solar radiation pressure that, in polar sun synchronous orbits, serve to stabilize the sail into attitudes where it presents less area in the ram direction. However, resilient transparent polymer films (e.g., LaRC-CP1) are challenging to acquire due to export control laws. (Incidentally, metalized films of any kind thinner than 7.6 µm are difficult to acquire for the same reason.) Therefore, 12.7 µm thick Kapton film with a 300 Å aluminum coating on both sides will be employed as the sail material. Kapton is capable of withstanding the expected worst-case hot temperature of ~ 225ºC that the sail will reach in direct sunlight.

The sail module is required to be re-stowable without substantial disassembly or any de-integration from the spacecraft. Therefore, the sail is folded and packed into a separate sail cartridge that may be installed in the sail module, and removed after a deployment. The sail cartridge incorporates a door that serves the dual purpose of restraining the tightly packed sail material and restraining the spring-loaded boom tips. Compared to installing a loose sail bundle into an integrated sail module directly, installing a cartridge reduces the risk of damaging the sensitive solar cells and thermal coatings on the exterior of the spacecraft.

The sail is folded in an accordion or “Z” pattern in two perpendicular directions. The first direction is parallel to the outboard sail edge, and the second direction folds the resulting strip into a bundled shape that matches the irregular layout of the sail cartridge. The fold does not form enclosed volumes that could trap air, and is simple to re-fold, re-pack, and re-use.

Sail imaging: The CanX-7 Camera Boom (CamBoom) is a deployable boom containing three COTS imagers used for imaging the drag sails following deployment. The use of imagers was down-selected as the most direct and compelling means of verifying not just whether the sails have deployed, but also to assess the quality of deployment. The CamBoom will use three VGA resolution imagers. The current design, with field of view projections for the three imagers, is shown in Figure 18.


Figure 18: Imager projections on the deployed sails (image credit: UTIAS/SFL)


ADS-B (Automatic Dependent Surveillance - Broadcast)

CanX-7 will also accommodate a secondary ADS-B receiver payload being developed by COM DEV and RMC. This secondary payload will be operated for six months following spacecraft commissioning, both in order to emulate an operational implementation of a deorbiting device (in which the drag sails are deployed once operations of a given payload cease), as well as to undertake potentially the first on-orbit demonstration of aircraft tracking from a nanosatellite. ADS-B signals are transmitted by aircraft in L-band (1090 MHz), and encode aircraft identity and position information derived from onboard navigation systems. Transmission power from aircraft ranges from 75 W to 500 W (49 dBm to 57 dBm), occurring at randomized intervals using PPM modulation (Ref. 3).

The continuing increase in commercial aviation traffic, combined with the inability of current radar surveillance to track aircraft beyond sight of land, have led to increasing interest in monitoring air traffic from space. When combined with other situational awareness techniques, spaceborne ADS-B monitoring can assist in flight planning over oceans and remote areas, which in turn would allow for decreased flight times, improved aircraft fuel economy, and reduced engine emissions.

The concept of operations for the CanX-7 ADS-B payload is illustrated in Figure 19. Aircraft encode position, velocity, time and identity from on-board instruments and GPS satellites, and transmit ADS-B signals which are received by CanX-7 and transmitted to the CanX-7 ground station during next access. The ADS-B receiver for CanX-7 is illustrated in Figure 20.


Figure 19: CanX-7 ADS-B concept of operations (image credit: UTIAS/SFL)


Figure 20: ADS-B payload and payload computer (image credit: COM DEV, UTIAS/SFL)

1) “CanX-7 Deorbiting Demonstration Mission,” UTIAS/SFL, URL:

2) Barbara Shmuel, “Canadian Advanced Nanospace EXperiment 7 (CanX-7) Mission Analysis, Payload Design and testing,” Thesis submitted for the degree of Master of Applied Science, UTIAS, University of Toronto, 2012, URL:

3) Grant Bonin, Jesse Hiemstra, Thomas Sears, Robert E. Zee, “The CanX-7 Drag Sail Demonstration Mission: Enabling Environmental Stewardship for Nano- and Microsatellites,” Proceedings of the 27th AIAA/USU Conference, Small Satellite Constellations, Logan, Utah, USA, Aug. 10-15, 2013, paper: SSC13-XI-9, URL:

4) Barbara Shmuel, Jesse Hiemstra, Vincent Tarantini, Fiona Singarayar, Grant Bonin, Robert E. Zee, “The Canadian Advanced Nanospace eXperiment 7 (CanX-7) Demonstration Mission: Deorbiting Nano- and Microspacecraft,” Proceedings of the 26th Annual AIAA/USU Conference on Small Satellites, Logan, Utah, USA, August 13-16, 2012, paper: SSC12-I-9, URL:

5) Fiona Singarayar, “Preliminary Development and Detailed Structural Design and Analysis for the CanX-7 Nanosatellite,” Thesis submitted for the degree of Master of Applied Science, UTIAS, University of Toronto, 2012, URL:

6) Jesse Hiemstra, Barbara Shmuel, Fiona Singarayar, Vincent Tarantini, Brad Cotten, Bryan Johnston-Lemke, Grant Bonin, Robert E. Zee, “The CanX-7 Drag Sail Mission - A cubesat for demonstrating a small-satellite compatible deorbiting device,” 2012 Summer CubeSat Developers’ Workshop, Logan, Utah, USA, Aug. 11-12, 2012, URL:

7) Barbara Shmuel, Fiona Singarayar, Grant Bonin, Dr. Robert E. Zee, “CanX-7: A Canadian Demonstration Mission for Deorbiting Nano- and Microspacecraft,” ASTRO’12 16th ACSI Astronautics Conference, Québec City, Canada, April 23-26, 2012

The information compiled and edited in this article was provided by Herbert J. Kramer from his documentation of: ”Observation of the Earth and Its Environment: Survey of Missions and Sensors” (Springer Verlag) as well as many other sources after the publication of the 4th edition in 2002. - Comments and corrections to this article are always welcome for further updates.