NASA’s Balloon Program Analysis Group recently presented a roadmap to NASA, to guide them on how to plan and fund future balloon astronomy programs. Balloons have been used for over a century to conduct physics experiments, astronomical observations and Earth observing work, but remain relatively unknown to the general public. Balloon astronomy share many advantages with space telescopes, but at a fraction of the cost.
The first modern balloon-based scientific experiment was in 1912, when Austrian physicist Victor Hess lifted 3 electroscopes to an altitude of 5300 meters (although meteorologists had been using balloons to measure air temperature at different altitudes as far back as the late 19th century). Hess was trying to prove that background radiation emanates from radioactive minerals in the ground, but instead he found that ionizing radiation levels actually increased at high altitudes. This experiment, which discovered the high-speed particles that we now call cosmic rays, and which earned Hess a Nobel Prize, marked the beginning of the field of high-energy astrophysics.
Balloon astronomy
Modern balloon missions serve a wide range of scientific fields. Cosmic-ray observations are a valuable source of data for particle physics experiments. Cosmic-ray particles often carry energies far greater than what scientists can achieve in particle accelerators like the Large Hadron Collider, so these missions can collect valuable data by watching for collisions between cosmic rays and air molecules in the upper atmosphere.
But balloons often perform more traditional astronomical observations as well. Small telescopes (less than 1 meter aperture) are often hoisted above the atmosphere to study exoplanets. They can directly observe protoplanetary dust belts around stars, and detect new exoplanets using the transit method.
The high altitude of balloon flights means that infrared (IR) telescopes can be placed above the water vapor in our atmosphere. Since water vapor absorbs IR light very effectively, these telescopes can do high-resolution observations of very faint stars that would be impossible from the ground. Similarly, radio telescopes operating in the terahertz (THz) band, which is also blocked by atmospheric water vapor, can be lifted high enough to study the interstellar medium.
Benefits
Balloons can position scientific instruments and observatories at a high enough altitude to gain many of the benefits of observatories in space, but with few of the drawbacks. The most obvious advantage of balloons over satellites is cost; the James Webb Space Telescope (JWST) cost almost 9 billion dollars, and even modern commercial launch providers, with their reusable rockets, are still priced out of reach for smaller research programs and institutes. Balloons can hoist extremely bulky and heavy payloads to the very edge of space, and stay airborne for extended periods, at a tiny fraction of the price of a rocket launch.
Because these missions are cheap, they can tolerate a much higher level of risk. This not only means that junior or undergraduate researchers can get directly involved in the development of the instruments, but also that the experiment can be more ambitious; it’s much easier to accepta failed experiment if it didn’t cost too much!
Balloon missions also have a very high rate of recovery. Satellites tend to either be abandoned in space, or re-enter the atmosphere. Balloon missions, on the other hand, are usually fitted with GPS receivers and constantly transmit telemetry, so that their owners know exactly where to find them then they eventually return to Earth.
Testing and development
One effect of the advantages listed above is that balloons are often used as a testbed for new observing technologies and instruments. Many instruments sent into space, both in orbital observatories and on probes sent to other planets, are based on designs first tested in balloons.
For example, scintillating-optical-fibre hodoscopes are instruments used to detect cosmic-rays, and are commonly used in space. One was used in the Cosmic Ray Isotope Spectrometer (CRIS), which has been operating flawlessly on the ACE spacecraft for the past 23 years. Another is part of the CALorimetric Electron Telescope (CALET), which has been working on the International Space Station (ISS) since 2015. These instruments were first used with balloon-borne cosmic-ray experiments, and so benefited from years of development and testing before ever being launched into space.
Similarly, the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) and the ISS’s second Alpha Magnetic Spectrometer (AMS02) both rely on on instrumentation originally designed for the near-space high altitudes where balloons operate.
Design requirements
Balloons used for balloon astronomy have three basic design requirements: They should be able to float to very high altitudes, they should be able to lift heavy payloads, and they should be able to fly for a very long time before returning to Earth.
Helium balloons are only partially filled at launch. As they rise, and atmospheric pressure drops, the helium inside the balloon expands so that it is only fully inflated when it reaches it’s working altitude, and doesn’t burst on it’s way up. This is not a stable situation though. As the local temperature and pressure changes, so the gas inside the balloon will expand and shrink, causing the balloon to climb or fall to different altitudes, or even burst. To manage this, NASA uses two different designs.
Zero-pressure balloons (ZPB) carry a supply of ballast or helium, and are able to control their altitude as needed. If a ZPS balloon starts climbing too high, it vents some of the gas, deflating the balloon slightly, and if it starts to fall, it can either reinflate the balloon, or drop ballast. This is a very effective method of maintaining a stable altitude, but it does limit the lifetime of the mission — when the gas or ballast are finished, it can no longer maintain altitude and must descend.
Superpressure balloons (SPB) are made from much stronger materials – they don’t stretch, so the volume of the gas doesn’t change during flight. This requires that the gas inside the balloon be at a higher pressure than the surrounding atmosphere at all times, hence the name. SPBs are designed to maintain a relatively consistent altitude during the day night cycle, without needing to carry expendables, which lets them fly missions for very long periods.
ZPBs can fly for up to 8 weeks during the summer in Antarctica, but generally only manage shorter flights of a few days. They can hoist payloads of up to 4 tonnes into the low stratosphere, but less than a tonne into the high stratosphere. SPBs, by contrast, can handle flights of up to 100 days, but can’t fly as high as ZPBs, nor manage such heavy payloads.
To read the report in full, visit https://arxiv.org/abs/2210.01198
The post Many Next-Generation Telescopes are Carried on Balloons. Here's What the Next Decade Holds in Balloon Astronomy appeared first on Universe Today.
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