Thanks to advancements in IT and DIY fabrication, missions reserved for national space agencies just a decade ago are becoming increasingly accessible to hobbyists. Cue the High Altitude Photography Platform (HAPP), created by Christopher Couch and James Mayes.

The two engineers designed and built the HAPP, which is comprised of a jet-stabilized aircraft resembling the iconic three-man Apollo re-entry vehicle: a balloon system designed to take the aircraft to its 30km apogee and all the peripheral equipment and electronics that made that project successful. Though not the first high-altitude photography project, the HAPP is the first to capture stabilized 360-degree video.

Even more amazing was the project’s focus on DIY: over 80% of the 22 months for development were dedicated to creating tools and methods rather than actually producing flight hardware. The result is a project that can be replicated by hobbyists using locally sourced parts.

The HAPP can drift as much as 100km during each mission, so it was important to keep track of the lander and provide flight data to air traffic control. The RockBLOCK 9603 was vital in sending telemetry and system sensor data from the Arduino-based flight control computer at an altitude of up to 22km on the maiden flight, mission HAPP-M1.

While the power supply was in a temperature-controlled enclosure, the U-Blox board and PCBs were exposed to the atmosphere for the duration of the mission, experiencing temperatures ranging from +42°C down to -45°C, and pressures from 1atm down to 0.05atm.

The project’s creators have done a great job in documenting the project build and sharing the valuable knowledge they’ve gained.

In the spring of 2017, an international team of students from Luleå University of Technology in Sweden gathered together to brainstorm a REXUS/BEXUS program idea. The European program supports scientific and technological experiments on research rockets and balloons, sending two of each into space every year.

After some deliberation by the team, it was a scientific article on the potential of a manned mission to the upper Venusian atmosphere that gave the impetus for the Balloon Ejection Student Prototype INvestigation (BESPIN) Project. Though Venus’s runaway greenhouse effect makes the planet’s surface hot enough to melt lead, at a height of 50km temperature and pressure conditions are very similar to those found on Earth. This makes a balloon-assisted manned mission to Venus highly plausible.

That’s why the BESPIN experiment is made up of two parts – a flotation probe and a descent probe. At apogee (around 80km), both probes are ejected as a single free-falling unit (FFU) from the rocket’s nose-cone. The FFU freefalls until it reaches an altitude of about 5km, when a parachute is deployed on the descent probe.

When the FFU’s velocity has dropped below 7 m/s, a balloon on the flotation probe will inflate. Once it’s fully inflated, the descent and flotation probes will separate. The descent probe will continue parachuting down towards the ground, while the flotation probe uses its fully inflated balloon to attempt a controlled descent.

Following the deployment of the descent probe parachute, the team will be using a RockBLOCK 9603 to communicate housekeeping and positional data to a ground station. Like the rest of the equipment, the RockBLOCK will be undergoing rigorous testing to ascertain its suitability for vibration, shock, and pressure changes associated with the mission.

More on this story from the European Space Agency.

Professor Kirk Martinez and his team from the University of Southampton, UK, are using moving rover units equipped with RockBLOCKs to measure how Icelandic glaciers respond to small-scale changes in temperature and precipitation throughout the year.

Global warming has resulted not just in the melting of glaciers throughout the world, but in their accelerated movement as well. The increased temperatures mean that a larger amount of water is finding its way underneath glaciers, effectively acting as a lubricant and causing glaciers to speed up.

Using differential GPS (dGPS), Professor Martinez can accurately calculate glacier speeds by measuring location differences as small as 2cm. In the past, achieving such spatial resolution in remote locations and over the course of months was financially prohibitive.

But not anymore, thanks to the next generation of low-cost hardware being used in his Ice Tracker project. In previous research, sensor probes were also placed in and under glaciers, collecting data on conditions, pressure, stresses, and subglacial movement.

All of us at Rock Seven (now trading as Ground Control) wish Professor Martinez and his team the very best of luck.

Twinkling stars may be a gift for song writers and romantics, but they’re a bane for cosmologists who need a clear view of the sky to gather important data. Compensating for the many distorting kilometers of the Earth’s atmosphere is usually done by adaptive optics or by placing a telescope in orbit. But both solutions are notoriously expensive and difficult.

An international team of collaborators made up of the University of Toronto Physics and Astronomy Departments, the Dunlap Institute, and the Institute for Aerospace Studies, the Durham University Centre for Advanced Instrumentation, Princeton University, and the Jet Propulsion Laboratory, went for a tried-and-tested solution dating back to the late 1700s – and thus the Balloon-borne Imaging Telescope (aka. SuperBIT) was born.

Floating a 0.5m telescope above 30km (and 99%) of the Earth’s atmosphere required some heavy revising of 300-year-old ballooning technology. An array of precision gyroscopes, motors, and actuators, as well as a custom-built star tracker, were used to achieve advanced image stabilization. The result is crisp one- to five-minute exposures in the near-infrared, red, green, blue, and ultraviolet bands, as well as in broadband.

The team is now getting ready for a third engineering flight from Palestine, Texas, while the main ultra-long-duration balloon flight (ULDB) is scheduled for 2020 in New Zealand. It’s this final mission that will demonstrate the SuperBIT’s capability as a facility-class instrument.

When fully operational, the SuperBIT will study strong and weak gravitational lensing and map out the distribution of dark matter around hundreds of galaxy clusters.

Photos (c) Department of Physics, University of Toronto.

Ground Control offers users the ability to connect to all Gill meteorological sensors, taking key data on a regular basis and transmitting it over satellites at an affordable price.

Collecting data from extremely remote systems is now becoming commonplace, and there are a number of existing GSM/GPRS services which allow this. However, they assume that there’s some form of mobile network coverage, whereas a lot of extremely remote installations are far from civilization or in areas where there are gaps in the mobile network coverage.

Now, there’s a way to collect data from your remote sensors regardless of where the systems are installed, using the global network of Iridium satellites and the RockFLEET‘s M2M/IoT ability.

Alongside the meteorological data, the RockFLEET unit also transmits position data – particularly useful where installed on buoys or other equipment that may move position either accidentally or by design. By getting regular position reports, you can receive early warnings if your equipment is moving off-station. RockFLEET is designed to provide global tracking and M2M/IoT (machine-to-machine / internet of things) data communication from anywhere in the world.