Space Sunday: of rockets and planets

SpaceX Crew Dragon (l) and the Boeing CST-100 Starliner: Further delays could threaten US access to the ISS. Credit: SpaceX / Boeing

The first SpaceX Crew Dragon (aka Dragon 2) vehicle destined to fly in space has arrived in Florida ahead of its launch, due in August 2018. The capsule is intended to be part of an uncrewed first flight to test the vehicle’s flight test systems.

Prior its transfer to Kennedy Space Centre (KSC), the capsule and service module were the subject of extensive thermal vacuum chamber tests at NASA’s Plum Brook Station in Ohio. The world’s only facility capable of testing full-scale upper-stage launch vehicles and rocket engines under simulated high-altitude conditions, the chamber is a vital part of pre-launch testing – although by the date of the capsule’s arrival at KSC, the results of the Ohio testing had not been made public.

SpaceX’s first Crew Dragon spacecraft is prepared to undergo testing at the In-Space Propulsion Facility of NASA’s Plum Brook Station in Sandusky, Ohio on June 13th, 2018. Credit: SpaceX

No official date for the first Crew Dragon flight has been released, but SpaceX are pushing ahead with work to prepare the vehicle for launch, in anticipation of the flight being given the green light for August. The test flight should see the uncrewed test vehicle fly to the International Space Station (ISS), with a follow-up 14-day crewed test flight due to take place in late 2018 / early 2019.

The arrival of the Crew Dragon test article at KSC came at the same time as a further US government report raised concerns about both SpaceX and Boeing – the other company contracted to make crewed flights to / from the ISS using their CST-100 Starliner capsule – being able to meet the current schedule for commencing formal operations.

A July 11th, 2018, report from the independent Government Accountability Office (GAO) points out that if any significant issues arise with either / both vehicles prior to their formal certification, it could see one or other or both companies being unable to commence active crew launches within the anticipated time frames specified by NASA. Were this to be the case, America would effectively be without the means to send astronauts to the Space Station, as the current contract to fly US crew aboard Russian Soyuz vehicles expires in November 2019.

Under the original schedule, the Boeing CST-100 was to have been certified for crew operations in January 2019, and the Crew Dragon in February 2019. However, both these dates were recently revised: the CST-100 certification slipping to December 2019 and Crew Dragon’s to February 2020.

With crew rotations to the ISS lasting 6 months, this slippage – which moved the first official crewed flights of both CST-100 and Crew Dragon to several months after the Soyuz contract ends – were not seen as a significant issue. However, the GAO report warns that certification of both vehicles could slip to around August 2020 should difficulties with either / both vehicles be encountered as a result of the test flights (or other reasons). This would potentially see a nine-month gap open between the last of the planned US Soyuz flights and a commencement of CST-100 / Crew Dragon flights, more than the span of a crew rotation, with no contingency currently in place to allow continued US access to the ISS until either of the new vehicles is ready to fly.

A “Temperate” Exoplanet?

Ross 128 is a red dwarf star just 11 light-years away from our Sun that over the years has been a source of interest for astronomers. First catalogued in 1926, the star is too faint to be seen with the naked eye, but is classified an old disk star with a low abundance of elements other than hydrogen and helium. Like most red dwarf stars, Ross 128 is given to violent flare activity, although its extreme age makes such events a lot less frequent than “younger” red dwarfs.

In mid-2017, Ross 128 caused something of a stir when a mysterious burst of signals was recorded apparently coming from its general vicinity. Dubbed the “Weird!” signals, the series of unusual “transmissions” were received by the  Arecibo radio telescope, Puerto Rico on May 12th/13th, 2017.

The 2017 Weird! signal that seemed to come from Ross 128 (but has never been re-acquired). Credit: UPR Aricebo

At the time, the signals caused a lot of excitement and talk of “aliens” being involved – although no planets had actually been detected around Ross 128. As I reported in July 2017, after further study, it was determined that the most likely explanation for the signals was that they’d been accidentally picked up from satellites occupying the same part of the sky as Ross 128 at the time Aricebo happened to be listening; all attempts to re-acquire them by numerous radio telescoped failed to do so.

While there is no reason to change the view that the odd signals of May 2017 were from local satellites rather than originating with Ross 128, in November 2017 it was confirmed the star does in fact have a planet orbiting it.

Referred to as Ross 128 b, the planet was first detected in July 2017 by a team operating the High Accuracy Radial velocity Planet Searcher (HARPS) instrument at the La Silla Observatory in Chile. However, it was not until November of 2017 that the astronomers were able to confirm that had located the planet.  Since then, the planet has been the subject of indirect scrutiny to try to better determine its characteristics, and the results are interesting.

The HARPS data initially suggested the planet to be roughly around the size of Earth and orbiting in the star’s habitable zone. However, further characterisation of the planet – including whether or not it has an atmosphere – has been hampered by the fact that its orbit around its parent star means it doesn’t actually transit between Ross 128 and Earth.

An artist’s impression of Ross 128 b orbiting its parent star. Credit: ESO/M. Kornmesser

As this presents a barrier to analysing the planet directly by the effect it and its atmosphere (if it has one) has on light coming from its parent star, astronomers instead turned to studying Ross 128 itself in their attempts to better understand the potential nature of Ross 128 b.  In particular, a team led by Diogo Souto of Brazil’s Observatório Nacional used Sloan Digital Sky Survey‘s APOGEE spectroscopic instrument to measure the star’s near-infrared light to derive abundances of carbon, oxygen, magnesium, aluminium, potassium, calcium, titanium, and iron.

Continue reading “Space Sunday: of rockets and planets”


Space Sunday: Kepler, China, and a voyage to the Sun

An artist’s rendering of Kepler in its heliocentric orbit. Credit: NASA

In March 2018, I reported that NASA’s exoplanet hunting Kepler mission might be drawing to a close. The end of the mission was threatened when engineers confirmed that the observatory was showing signs of running out of fuel.

Responsible for locating 70% of the 3,750 exoplanets discovered to date, Kepler was launched in 2009 and has been one of the most successful missions NASA has run. Unfortunately, as a result of a change to its operational parameters following the failure of two of the four reaction wheels used to hold it steady while observing distant stars, the observatory has had to increase its use of its propellant reserves. As a result, on July 2nd, 2018, NASA Kepler was ordered into a “no-fuel-use safe mode” after telemetry reported an “anomalous” drop in fuel pressure in the spacecraft.

The observatory will remain in this mode until August 2nd, 2018, when it is due to use its manoeuvring jets to orient itself so it can transmit the data collected on its last observational campaign – the 18th in its extended mission – to Earth via the Deep Space Network. During the time between now and August 2nd, engineers will attempt evaluate the status of the spacecraft’s propulsion system to determine if it has sufficient fuel left to allow it to resume observations in what is called Campaign 19, scheduled to begin August 6th, 2018.

Kepler has been tremendously successful by any measure. In addition to its impressive raw planet tally – liable to raise as there are still more than 2,000 planet candidates still to be vetted – the data gathered by Kepler since 2009 seems to suggest that 20% of Sun-like stars host a roughly Earth-size planet in the habitable zone — that just-right range of distances where liquid water could exist on a world’s surface.

During its primary mission, from 2009 through May 2013, Kepler stared at about 150,000 stars simultaneously, hunting for periodic dipping in their brightness that might indicate a planetary body moving in front of them. Since 2014, it has been engaged on its extended K2 mission, comprising a series of observational campaigns lasting 80 days apiece, each focused on a slightly different area of sky.

However, if this is the beginning of the end for Kepler, it’s not the end of our exoplanet hunting efforts: if all is proceeding as planned, the Transiting Exoplanet Survey Satellite, launched in April, 2018, should be taking over the task – although admittedly, news on its “first light” image, which was due in June, has yet to be released.

China’s Super-Heavy Launch and Reusable Rocket Capabilities

Speaking during an event in China at the end of May 2018, Long Lehao, a chief designer with the China Academy of Launch Vehicle Technology (CALT), gave an update on two of China’s new launch vehicles: the Long March 9 super booster and the partially reusable Long March 8 rocket.

The Long March 9 – referred to as the CZ-9, or Changzheng 9 in Chinese – is slated to enter service in 2030, and is central to China’s interplanetary ambitions. It is also a huge increase in scale a capability for the nation’s launch systems. The core three-stage rocket will stand 93 metres tall, using a 10-metre diameter first stage. It will be assisted at launch by four 5-metre diameter strap-on boosters – these alone being the same diameter as China’s Long March 5, currently the country’s most powerful rocket. The most powerful variant of the vehicle will be capable of launching 140 tonnes to low-Earth orbit (LEO), 50 tonnes to the Moon and around 44 tonnes to Mars.

China’s Long March 9 (CZ-9), flanked by launch vehicles past and present, including Russia’s never successfully flown N-1 lunar rocket from the 1960s. Via: Wikipedia

By comparison, NASA’s Space Launch System (SLS) vehicle will have a core stage 8.4 metres in diameter, with its most powerful variant (Block 2) capable of placing 130 tonnes into LEO, and SpaceX’s BFR with a 9-metre diameter core and be capable of putting 150 tonnes into LEO.

In his presentation, Long confirmed the first CZ-9 is slated for launch in 2030 – around the time the Block 2 variant of the SLS is due to fly. One of the first missions earmarked for the super booster is an automated Mars sample return mission, with crewed lunar missions also on the cards for the vehicle. In addition, the CZ-9 could be used to deploy a system of solar power satellites the Chinese government and military are said to be considering.

Meanwhile, the Long March 8, based on the core of China’s current mid-range launcher, the Long March 7, is expected to make its first flight in 2021. Capable of lifting a more modest 8 tonnes to LEO, the first stage of the booster is designed to be reusable, employing a similar methodology to SpaceX’s Falcon 9 first stages to return to Earth and land.

An artist’s impression of the Long March 8 first stage about to make a soft-landing at the end of a launch flight. Credit: Shanghai Academy of Spaceflight Technology

While the payload capacity of the Long March 8 might sound small, it is ideal for typical satellite payloads. More to the point, the use of the Long March 7 first stage means the system could be “upgraded” to work with that vehicle, which is capable of placing 13 tonnes into LEO.

Continue reading “Space Sunday: Kepler, China, and a voyage to the Sun”

Space Sunday: asteroids, telescopes and dust

Credit: Mopic/Shutterstock

Saturday, June 30th marked International Asteroid Day, a global event involving researchers, astronomy groups, space agencies and more talking about asteroids  – and the risk some of them present to Earth.

Since 2013, and the Chelyabinsk event which saw a meteor  roughly 20 metres across, caught on film as it broke up high over the Russian town, the tabloid media has seemingly been obsessed with reporting meteors about to collide Earth and wreak havoc.

Fortunately, the vast majority of the estimated 10 million objects which have orbits passing close to Earth – referred to as NEOs, for Near Earth Objects, are unlikely to actually strike our atmosphere or are of a small enough size not to pose a significant threat if they did, despite all the screaming of the tabloids.

A map showing the frequency of small asteroids entering Earth’s atmosphere between 1994 and 2013. The dot sizes are proportional to the optical radiated energy of impacts measured in billions of Joules (GJ) of energy. A total of 556 events are recorded on the map, representing objects ranging in size from 1m to 20m. Credit: NASA’s Near Earth Object (NEO) programme

Which is not to say NEOs don’t pose a potential threat. Not all of the 10 million objects with orbits passing close to, or intersecting, the orbit of Earth have been properly mapped. Take 2018 LA (ZLAF9B2), for example. As I reported at the start of June, this asteroid, some 2 metres across, was only identified a handful of hours before it slammed into Earth’s upper atmosphere over Botswana at approximately 17,000 kilometres per second, to be caught on film as it burnt up. The energetic force of the accompanying explosion has been estimated to have been in the region of 0.3 to 0.5 kilotons (300 to 500 tonnes of TNT).

To offer a couple of quick comparisons with this event:

  • The 2013 Chelyabinsk superbolide (roughly 10 times the size of 2018 LA (ZLAF9B2) disintegrated at an altitude of around at 29.7 km at a velocity between 60,000-69,000 km/h, producing an energy release equivalent to 400-500 kilotons (400,000-500,000 tonnes of TNT). This was enough to blow out windows and send 1,491 people to hospital with injuries, including several dozen temporarily blinded by the flash of the explosion. The first 32 seconds of the video below convey something of the force of that event.

  • In June 1908 a cometary fragment estimated between 60 and 190 metres cross disintegrated some 5 to 10 km above Tunguska, Siberia. This generated an estimated downward explosive force of between 3 to 5 megatons and an overall force of somewhere between 10 to 15 megatons (again for comparison, all the bombs dropped by allied forces in World War 2 amounted to around 3.4 megatons of combined explosive force). This is believed to have generated a shock wave measuring 5.0 on the Richter scale, flattening an estimated 80 million trees covering an area of 2,150 square kilometres. Were it to occur today, such an event would devastate a large city.

There are two sobering points with these two events. The first is that astronomers estimate only about one-third (1600) of objects the size of the Tunguska event meteoroid which might be among that 10 million NEOs have so far been mapped. The second is that many NEOs can remain “hidden” from our view. the Chelyabinsk superbolide, for example passed unseen as the Sun completely obscured its approach to Earth.

There have been several proposals for trying to deal with the potential risk of a PHA – Potentially Hazardous Asteroid – impact over the years. One currently in development is the NASA / Applied Physics Laboratory (APL) Double Asteroid Redirection Test (DART) mission intended to demonstrate the kinetic effects of crashing an impactor spacecraft into an asteroid for planetary defence purposes.

The target for this mission is rather interesting. DART will be launched on an intercept with 65803 Didymos, an asteroid around 750 metres across – but this will not be the vehicle’s target. That honour goes to a much smaller asteroid – around 170 metres across (so in the size range of the Tunguska object) – orbiting 65803 Didymos and informally referred to as “Didymoon”.

Originally, DART was to be a part of a joint NASA/APL and European Space Agency effort, with ESA supplying a vehicle called the Asteroid Intercept Mission (AIM). This would have been launched ahead of DART on a trajectory that would place it in orbit around the 65803 Didymos / “Didymoon” pairing, allowing it to track / guide DART to its target and record the entire impact and its aftermath.

AIM never received funding, leaving the NASA/APL mission, which is currently scheduled for launch in 2021 and will intercept “Didymoon” in 2022. However, in the last few weeks, ESA has announced a revised mission to 65803 Didymos called Hera. Like AIM, it is designed to orbit the asteroid and is moon, and a call has been made to combine it with DART under a new joint mission called Asteroid Impact and Deflection Assessment (AIDA).

This would require DART to be delayed for a number of years to give ESA time to obtain approval for Hera and design, build and launch the craft – so the intercept would not take place until 2026. While this is a delay, it would mean that scientists would be able to better characterise “Didymoon” ahead of DART’s arrival, and witness the impact and its aftermath in real-time.

The original DART / AIM mission – to study the use of kinetic vehicles to divert an asteroid – now potentially superseded by the DART / Hera mission. Credit: NASA / APL / ESA

It’s not clear whether or not DART will be delayed. If it isn’t, then it has been proposed DART carries a camera equipped cubesat similar to those AIM would have used in support of its mission. This could then be separated from DART ahead of the impact so it could image the event as it flies by “Didymoon”. The Hera mission would then arrive a few years after the impact and assess the outcome, including imaging the impact crater on the asteroid and changes to its orbit and its rotation, which can help scientists determine how efficient the impact was in transferring its energy into “Didymoon”.

Continue reading “Space Sunday: asteroids, telescopes and dust”

Space Sunday: stations, Ceres, doubts and rockets

Tiangong-2, with one of the two docking ports visible. Credit: China News

China may be preparing to de-orbit its Tiangong-2 orbital laboratory, possibly to avoid a situation similar to that relating to the so-called “uncontrolled” re-entry of their Tiangong-1 facility, which re-entered the Earth’s atmosphere and broke-up / burnt-up in April 2018.

Orbital information published by the U.S. Strategic Command’s Joint Force Space Component Command, through the Joint Space Operations Centre, indicates that Tiangong-2 has moved from an altitude of around 380 by 386 km down to 292 by 297 km.

No official announcement regarding the status of the Tiangong-2 space lab has been made by the China Manned Space Engineering Office (CMSE), however, China has made no secret of its plans to establish a permanent orbital presence over the Earth in the 2020s – and that to do so, they would discontinue operations with both Tiangong-1 and Tiangong-2. and de-orbit both.

Measuring 10.4 metres in length and some 3.3 metres in maximum diameter, Tiangong-2 weighs 8.6 metric tonnes – making it the same overall size and weight as Tiangong-1, launched in 2011. The re-entry of that unit came after a series of alarmist headlines claiming it would “crash” to Earth after it was reported the Chinese only had partial control over it. Because of that tabloid farrago, some have speculated the alteration in Tiangong-2’s orbit is to allow China to retain full control over the facility, including when it re-enters the atmosphere.

Jing Haipeng (l) and Chen dong (r) aboard Tiangong-2. The only crew to visit the facility Credit: CCTV

Launched in September 2016, Tiangong-2 hosted a single crewed visit that same year, which lasted 30 days. In 2017 served as a test-bed for verifying on-orbit automated docking and refuelling capabilities  – two aspects of operations vital to the Chinese ambitions of developing their large-scale space station – using the Tianzhou-1 cargo spacecraft.

Tiangong-2 carried a range of science payloads, including POLAR, a gamma-ray burst detector developed by an international collaboration including Swiss, Chinese and Polish institutes. According to principal investigator Nicolas Produit, this astro-particle experiment collected excellent data during six months of operations, with science results to be published shortly. It is the kind of international collaborative effort China would like to develop with its new station.

Artist’s impression of the planned Chinese space station complex. Credit: CCTV

China is aiming to launch the first module of the space station proper, named Tianhe, around 2020. This mission first requires the nominal return-to-flight of the heavy lift Long March 5 launch vehicle, which suffered a launch failure in July 2017. When completed, the space station will mass between 60 and 100 metric tonnes, including two experiment modules due for launch in 2022. It will be capable of hosting three astronauts in rotations of up to six months at a time. A further element of the station will be a free-flying Hubble-class space telescope capable of docking with the station to receive propellants and undergo maintenance and repairs.

More on Ceres and the Building Blocks of Life

In February 2017, I wrote about the discovery of the basic building blocks of life on Ceres, which has been the subject of the joint NASA / ESA Dawn mission since March 2015.

The discovery of aliphatic compounds on the surface of Ceres was made by an international team of scientists who had been reviewing data from the Visible and Infra-red Mapping Spectrometer (VIMS) aboard the spacecraft. Now, a new study conducted by a team of researchers from Brown University suggests that these patches contain more organic material than previously thought.

Dawn spacecraft data show a region around the Ernutet crater where organic concentrations have been discovered (labelled “a” through “f”). The colour coding shows the strength of the organics absorption band, with warmer colours indicating the highest concentrations. Credit: NASA/JPL / UCLA / ASI / INAF / MPS / DLR / IDA

Aliphatics are a type of compound where carbon atoms form open chains that are commonly bound with oxygen, nitrogen, sulphur and chlorine – all of which are necessary for the evolution of life. This doesn’t actually mean that Ceres supports life, because these molecules can also arise from non-biological processes. Nevertheless, the presence of these compounds does raise the questions.

The team behind original discovery of the aliphatics, found within a 1000 km² region around of the Ernutet crater, concluded that between 6 and 10% of the spectral signature detected on Ceres could be explained by organic matter. As hydrothermal activity had been detected on Ceres, the researchers hypothesised that the molecules were endogenous in origin – that is, they came from inside the protoplanet. Given that ammonia-bearing hydrated minerals, water ice, carbonates, and salts have also been detected on Ceres, there is the suggestion that it may have an interior environment that can support prebiotic chemistry.

Dawn mission (NASA / JPL) – click for full size

However, rather than relying on Earth rocks on which to base their work and findings, the team from Brown University used carbonaceous chondrite meteors, which have been shown to contain organic material that is slightly different from what we are familiar with here on Earth. As a result, they determined that the organics found on Ceres were distinct from their terrestrial counterparts – and the up to 40 to 50% of the spectral signal we see on Ceres is explained by organics – far more than originally estimated.

If this latter estimate is correct, it raises the question about where it came from – 40% is a lot for the compound to be entirely endogenous in origin. Rather, the high concentrations seem to be more consistent with being deposited by a comet impact.

Given that the asteroid belt is composed of material left over from the formation of the Solar System,  determining where these organics came from could shed light on how organic molecules were distributed throughout the Solar System early in its history, and the role this distribution may have played in the development of life here in Earth.

If, however, the compound deposits are endogenous in origin, there is still the question of what mechanisms were / are in play to result in such high concentrations emerged in Ceres’ northern hemisphere, and then preserve them in these locations. This is a question unlikely to be answered without follow-up missions able to obtain and analyse samples gathered from the surface of the protoplanet.

Continue reading “Space Sunday: stations, Ceres, doubts and rockets”

Space Sunday: drills, neutrinos and a spaceplane

In May I wrote about an attempt to return the drill mechanism on the Mars Science Laboratory (MSL) rover Curiosity to operational status. As I noted in that report, use of the sample-gathering drill was suspended in December 2016, after problems were encountered with the drill feed mechanism – the motor used to extend the drill head leading to fears that continued use of the drill feed mechanism would see it fail completely, ending the use of the drill.

At the time of that report, a live test of the drill on Mars had just been carried out, but the results hadn’t been made public. However, on May 23rd, NASA issued an update confirming the test had been successful, and a sample of rock had been obtained.

The new drilling technique is called Feed Extended Drilling (FED). It keeps the drill head extended and uses the weight of the rover’s robot arm and turret to push the bit into a target rock. This is harder than it sounds, as it requires the weight of the rover’s arm to provide the necessary pressure to help push the drill bit into a rock – something it is not designed to do, and risks either breaking the drill bit or cause it to become stuck.

Engineers had spent more than a year developing the technique using Curiosity’s testbed “twin” on Earth before carrying out a preliminary test on Mars in February (see here), which was not intended to gather any sample. For the May 19th, 2018, test the mission team combined the FED approach to drilling with using the drill’s percussive mechanism with the intention of both testing the combined technique with an attempt to obtain a sample of rock.

The sample in question is of specific importance to the mission team, although it required a literal turnaround for the rover. For the last few months, Curiosity has been traversing “Vera Rubin Ridge” on “Mount Sharp”. In doing so, the rover passed a distinct rock formation mission scientists realised could fill a gap in their understanding about how “Mount Sharp” may have formed. However, at the time, there was no way to obtain a sample. Once it looked likely that drilling operations could be recovered, the decision was made in April to reverse the rover’s course and return to the rock formation, where the test was successfully carried out.

The team used tremendous ingenuity to devise a new drilling technique and implement it on another planet. Those are two vital inches of innovation from 60 million miles away. We’re thrilled that the result was so successful.

– Curiosity Deputy Project Manager Steve Lee.

The 5 cm (2-in) deep hole in a target called “Duluth”, captured by the rover’s Mastcam on May 20th, 2018 (Sol 2057) after a successful test allowed a rock sample to be gathered by the rover since October 2016. Credit: NASA/JPL / MSSS

The rover has since resumed its traverse towards an uphill area enriched in clay minerals that the science team is  also eager to explore. The next stage for the engineers it so figure out how to transfer the gathered sample ready for analysis by the rover’s on-board laboratory.

Previously, this would have involved passing the sample through another system on the rover’s “turret”, called CHIMRA (Collection and Handling for In-Situ Martian Rock Analysis). However, transfer into CHIMRA in part requires the use of the drill feed mechanism. As this can no longer be used in case it breaks. the idea – yet to be tested – is to try positioning the drill head over the hoppers feeding the science suite and then running the drill in reverse, allowing the sample  – held within the hollow drill bit – to trickle back out, and hopefully into the hoppers.

If It’s A Particle Jim, Then It’s Not As We Know Them

Neutrinos are elementary particles that interact only via the weak subatomic force and gravity. Their behaviour is explained by the Standard Model of particle physics.

In essence – and very broadly speaking – the Standard Model is a list of particles that go a long way toward explaining how matter and energy interact in the cosmos. Some of these particles – quarks and electrons, for example – are the building blocks of the atoms that make up everything we’ll ever touch with our hands. Others, like the three known neutrinos, are more abstract: high-energy particles which can be created naturally (within the core of stars or during supernova events, for example), or artificially (e.g. in nuclear reactors or nuclear explosions), and which stream through the universe, barely interacting with other matter. Billions upon billions of solar neutrinos pass through each of us every second without ever affecting us.

The LSND. Credit: Los Alamos National Laboratory

These neutrinos can be broken into three known “flavours”:  electron, muon and tau neutrinos. As waves of neutrinos stream through space, they periodically “oscillate,” jumping back and forth between one flavour of the three flavours and another – or that’s the theory.

In the 1990s, the Liquid Scintillator Neutrino Detector (LSND) at the Los Alamos National Laboratory, New Mexico, reported more neutrino detections than the Standard Model’s description of neutrino oscillation could explain, resulting in a new flavour of “heavy” neutrino being posited: the “sterile neutrino”.

At the time, the discovery met with excitement; physicists had long noticed a discrepancy between the predicted and actual number of anti-neutrinos, or the antimatter partners to neutrinos, produced in nuclear reactors. Sterile neutrinos could offer an explanation for the discrepancy. The only problem with the idea is that other than the LSND results, no-one has been able to find evidence for the existence of “sterile neutrinos”.

Until, possibly, now. A paper just published suggests that another neutrino detector – the MiniBooNE, operated Fermilab in Chicago – has also reported a similar result to LSND, resulting in the suggestion some neutrinos are oscillating into the “heavier” sterile neutrinos and then back into one of the recognised flavours. What’s more, combining the results of the MiniBooNE experiment with those of LSND suggests there is just a one-in-500 million chance of both results being a fluke.

Continue reading “Space Sunday: drills, neutrinos and a spaceplane”

Space Sunday: the Moonwalker and the artist

Astronaut and painter, Alan Bean in his Studio in Texas. Credit: unknown

The pool of men who flew to the Moon, and those who walked on its surface, as a part of NASA’s Apollo programme is sadly shrinking. And on Saturday May 26th, 2018, it became even smaller with the news that Alan Bean, the fourth man to set foot on the Moon had passed away.

His passing was unexpected. Although 86 years of age, he was in good health and was travelling with his family when he suddenly fell ill while in Indiana two weeks ago. He was taken to the Houston Methodist Hospital in Houston, Texas, to receive treatment, but passed away whilst at the hospital.

Born on March 15th, 1932 in Wheeler County, Texas, Alan LaVern Bean received a Bachelor of Science degree in Aeronautical Engineering from the University of Texas, Austin in 1955. While at the UT Austin, he accepted a commission as a U.S. Navy Ensign  in the university’s Naval Reserve Officers Training Corps and attended flight training.

Alan Bean in 1969 in a NASA publicity photograph ahead of the Apollo 12 mission. Credit: NASA

Qualifying as a pilot in 1956, he served four years  based in Florida flying attack aircraft. He was then posted to the U.S. Naval Test Pilot School (USNTPS) at Patuxent River, Maryland, where his instructor was the irrepressible Charles “Pete” Conrad. The two stuck up an enduring friendship which was to eventually take them to the Moon.

As a naval test pilot, Bean flew numerous aircraft prior to transferring back to fighter operations in 1962, again serving in Florida for a year. In 1963, he was accepted into NASA as a part of the Group 3 astronaut intake.

He had originally applied as a part of the Group 2 intake in 1962 alongside Conrad, but failed to make the cut. Coincidentally, Conrad’s Group 2 application  – which was successful – was also his second attempt to join NASA. He’d actually been part of the Group 1 intake, but  – always rebellious – he walked away for being subject to what he felt were demeaning and unnecessary medical and psychological tests.

Bean’s flight career at NASA was initially choppy: he was selected as a back-up astronaut with the Gemini programme but did not secure a flight seat. He then initially failed to gain an Apollo primary or back-up flight assignment. Instead he was assigned to the Apollo Applications Programme testing systems and facilities to be used in both lunar missions and training for flights to the Moon. In this capacity he was the first astronaut to use the original Weightless Environment Training Facility (WETF). This is a gigantic pool in which astronauts may perform tasks wearing suits designed to provide neutral buoyancy, simulating the microgravity they will experience during space flight. He became a champion for the use of the facility in astronaut training, which was used through until the 1980s, when is was superseded by the larger Neutral Buoyancy Laboratory (NBL) used in space station training.

On October 5th, 1967, Apollo 9 back-up Lunar Excursion Module (LEM) pilot Clifton Williams was tragically killed in an air accident. As a result, “Pete” Conrad, the back-up crew commander specifically requested Bean be promoted to the position of his LEM pilot. This placed the two of them, together with Command Module (CM) pilot Richard F. Gordon Jr on course to fly as the prime crew for Apollo 12, the second mission intended to land on the Moon.

Bean and Conrad approached their lunar mission with huge enthusiasm and commitment. In contrast to some of their comrades, who at times found the intense geological training the Apollo astronauts went through a little tiresome, they became extremely engaged in the training – which resulted in them gathering what Harrison Schmitt – the only true geologist to walk on the Moon thus far – later called, “a fantastic suite of lunar samples, a scientific gift that keeps on giving today.”

The Apollo 12 crew (l to r): Charles “Pete” Conrad, Commander; Richard F. Gordon Jr , Command Module pilot; and Alan Bean, Lunar Excursion Module pilot. Credit: NASA

In particular, Bean and Conrad became deeply involved in one of the primary aspects of their mission – a visit to the Surveyor 3 space craft.

The Surveyor programme was a series of seven robotic landers NASA sent to the Moon between June 1966 and January 1968, primarily to demonstrate the feasibility of soft landings on the Moon in advance of Apollo. Scientists were particularly keen that Conrad and Bean land close enough the probe so they could collect elements from it for analysis on Earth to see what exposure to the radiative environment around the Moon had treated them.

However, Bean had his own plans for the trip to the Surveyor vehicle: with Conrad, he conspired to smuggle self-timer for his Hasselblad camera in their equipment. The pair planned to secretly set-up the camera and use the timer to capture a photograph the pair of them standing side-by-side on the Moon – and confuse the mission control team as to how they had managed the feat! Unfortunately, Bean couldn’t locate the timer in their equipment tote bag until it was too late for the picture to be taken. Instead, he later immortalised the scene in his painting The Fabulous Photo We Never Took.

“The Fabulous Photo We Never Took” by Alan Bean. Courtesy of

Apollo 12 launched on schedule from Kennedy Space Centre on November 14th, 1969, during a rainstorm. Thirty-six-and-a-half seconds after lift-off, the vehicle triggered a lightning discharge through itself and down to the Earth through the Saturn’s ionized plume. Protective circuits on the Service Module falsely detected electrical overloads and took all three fuel cells off-line, along with much of the Command/Service Module (CSM) instrumentation.

A second strike then occurred 15.5 seconds later, resulting in further power supply problems, illuminating nearly every warning light on the control panel as it caused a massive instrumentation malfunction. In particular, the “8-ball” attitude indicator was knocked out and the telemetry feed to Mission Control became garbled. However, the vehicle continued to fly correctly, the lightning not having disrupted the Saturn V’s own instrumentation unit.

Left: Apollo 12 is struck by lightning, the discharge passing down the vehicle into its exhaust plume. Right: the launch complex tower is also struck by lightning after the departure of the Saturn V rocket. Credit; NASA

Continue reading “Space Sunday: the Moonwalker and the artist”