The “Flying Water Tank”, aka “R2D2’s Dad”, otherwise know as the Starhopper – rises to 120m (500ft) during its second major test flight, August 27th, 2019. Credit: SpaceX
SpaceX successfully flew their Starhopper vehicle – designed to prove the viability of their upcoming Starship space vehicle – on August 27th, in its most complex test flight to date.
The Starhopper craft, dubbed “the flying water tank” on account it both lacks its conical nose (damaged beyond repair during a storm at the start of the year) and the fact it was fabricated for SpaceX by a company that specialises in building water tanks, lifted off from a pad at SpaceX’s test site in Boca Chica, Texas, rising vertically to a height of 150 metres (488 ft) before translating to horizontal flight to crab across to another pad at the test facility and then descended under power to touch down once more.
While the flight lasted less than a minute, it has, according to Musk, paved the way for two dramatic follow-up flights. As well as the Starhopper vehicle, SpaceX is currently building two full-size Starship prototypes – “Mk 1” is being built at Boca Chica, with “MK 2” under construction in Florida. It appears that the “Mk 1” vehicle will be used for the 20km flight.
Starship Mk 2 on the left of the image, standing upright and with additional elements nearby, under construction in Cocoa, Florida. Credit: SpaceX
Musk’s announcement of a potential attempt to reach orbital altitude drew questions on whether SpaceX plan to use their Super Heavy – essentially the “first stage” for Starship launches – with one of the Starship prototypes, or just make the attempt with the Starship on its own. In the past, Musk has indicated that a fuelled but unladen Starship should have the power to achieve orbit, but that would presumably be using all six of an operational Starship’s Raptor engines. By comparison, the Starhopper has a single Raptor motor and the Starship Mk 1 and Mk 2 craft will have 3 Raptors – at least initially.
As it stands, the “first generation” of Starship / Super Heavy is designed to be 9m (29 ft) in diameter and stand around 118m (390 ft) tall on the launch pad. Super Heavy is to be powered by 31 Raptor engines and the 48m tall Starship by 6 Raptors. Together, SpaceX stated that they will be capable of lifting around 100 tonnes of payload to orbit, with Starship capable of reaching the Moon or Mars with that payload or up to 100 crew and passengers.
All of that is pretty mind-boggling. If possible, it will make Starship / Super Heavy the most powerful launch system ever built in terms of thrust. But SpaceX is apparently going to go beyond that. Following the Starhopper test, and responding to a question, Musk indicated that a “next generation” craft based on Starship / Super Heavy could follow in “several years”. While planning a follow-up to Starship / Super Heavy is not surprising, the scale of the follow-up version is: in a further tweet, Musk suggested it will be 18m (60 ft) in diameter – twice that of Starship / Super Heavy.
Mathematics tells us that doubling the diameter of a circle quadruples its area. This means that if the current ratio of dimensions for Starship / Super Heavy is retained, the “next generation” version would stand 230 m (780 ft) tall and have eight times both the surface area and propellant tank volume of the current Starship / Super Heavy. All of which leads to a fuelled launch mass of around 40,000 tonnes. All of which is, frankly, entering the realm of idiocy; as I’ve previously (and subjectively) opined, it’s hard to see a launch vehicle with a 100-tonne payload mass being commercially viable unless the launch costs are such that it can turn a profit lifting around 5-10 tonne to orbit for the majority of its flights. As such, a vehicle twice the size (even if possible) has little to no chance, outside of highly specialised (and limited) launch roles.
An artist’s impression of a future “next generation” Starship / Super Heavy launch combination compared to SpaceX’s current family of launch vehicles, the current (2018) and previous (2016 and 2017) BFR designs. This assumes the “next generation” vehicle will have Musk’s stated 18m diameter and retain the same proportions as the current Starship / Super Heavy combination. Credit: Teslerati.
At such a size and mass, the new vehicle would require 100 Raptor motors just to get off the pad – or a system of engines several times more powerful. Take the noise and vibration issues this would introduce to the system, and I’ll say that it just isn’t going to happen. In the meantime, Musk is promising a public update on the status of Starship / Super Heavy on September 28th, 2019.
An artist’s impression of Europa Clipper (previously the Europa Multiple Flyby Mission), due for launch in 2022 or 2023 (depending on the launch vehicle used) making a flyby of Europa. Credit: NASA
There are a number of places within our solar system where life may have come to pass – and indeed, may still exist – beyond the Earth. There’s Mars, Saturn’s massive moon Titan, and the so-called “icy world” moons, such as Neptune’s Triton, Saturn’s Enceladus, and Jupiter’s Europa, all of which may harbour sub-surface oceans between their icy crusts and solid interiors.
Of these moons, Enceladus has shown clear signs of activity relating to the existence of a sub-surface ocean: the ESA / NASA Cassini mission captured images of great plumes of water erupting from the moon’s south polar region, and the Cassini vehicle passed through this plumes towards the end of its mission to “taste” them, confirm they were predominantly water.
However, the icy world that has garnered the most interest in terms of detailed study remains Jupiter’s Europa. Currently, there are two missions being developed to probe Europa in greater detail than ever before: NASA’s Europa Clipper and ESA’s Jupiter Icy Moons Explorer (JUICE).
Europe’s subsurface ocean as it might exist – a place that might support life. Credit: NASA
Europa Clipper has had something of an up-and-down ride. Originally, scientists wanted to send a vehicle to study all of the icy moons around Jupiter – Europa, Callisto and mighty Ganymede. However, the US $16 billion price tag for the mission (including vehicle development, launch and operation) was too high. It was scaled back to a more modest US $4.3 billion mission, the Europa Orbiter, which would have included a lander. Then it was scaled back again to a US $2 billion mission.
In 2014, the mission eventually morphed into the Europa Multiple Flyby mission: rather than placing a vehicle directly in orbit around Europa, this would put the vehicle in orbit around Jupiter from where it would be able to make multiple fly-bys of Europa. This then became Europa Clipper – which has still suffered from attempts to axe it, surviving only because it has very strong support within the US Congress.
This support has allowed the mission to both receive continued funding and proceed through various design and review activities. As a part of this, on Monday, August 19th, 2019, NASA announced that it had formally confirmed the mission can proceed to what is called Phase C, a process that will see the mission through the final spacecraft design and then on to assembly and testing.
We are all excited about the decision that moves the Europa Clipper mission one key step closer to unlocking the mysteries of this ocean world.
– Thomas Zurbuchen, NASA associate administrator for science
While Enceladus was the first moon where we positively witnessed plumes of water ice erupting from the surface (2005), evidence that similar outgassing may be occurring at Europa has been gathered by the Hubble Space Telescope. This information, gathered in the form of images, and data gathered by the magnetometer instrument carried by NASA’s Galileo space vehicle that surveyed Jupiter and his moons in the 1990s, offer the clearest indication that there is an ocean of water, possibly containing more than twice the volume of all the Earth’s oceans and sea combined, sitting beneath the surface ice on Europa.
The solar-powered craft – solar power being a lot cheaper than nuclear RTGs – will carry a total of nine primary science instruments, with eight confirmed as being:
The Europa Thermal Emission Imaging System (E-Themis) will provide high spatial resolution, multi-spectral imaging of Europa in the mid and far infra-red bands to help detect active sites, such as potential vents erupting plumes of water into space.
The Mapping Imaging Spectrometer for Europa (MIS), an imaging near infra-red spectrometer that will probe the surface composition of Europa, identifying and mapping the distributions of organics (including amino acids and tholins), salts, acid hydrates, water ice phases, and other materials. Scientists hope to be able to relate the moon’s surface composition to the habitability of its ocean.
The Europa Imaging System (EIS), a visible-spectrum wide and narrow angle camera instrument that will map most of Europa at 50 m (160 ft) resolution, and will provide images of selected surface areas at up to 0.5 m resolution.
The Europa Ultraviolet Spectrograph (Europa-UVS) instrument will be able to detect small plumes of material ejected by Europa, and will provide valuable data about the composition and dynamics of the moon’s exosphere.
The Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON), a dual-frequency ice penetrating radar instrument designed to characterise and sound Europa’s ice crust from the near-surface to the ocean, revealing the hidden structure of Europa’s ice shell and potential water pockets within.
The Plasma Instrument for Magnetic Sounding (PIMS) working in conjunction with a magnetometer, PIMS is key to determining Europa’s ice shell thickness, ocean depth, and salinity. PIMS will also probe the mechanisms responsible for weathering and releasing material from Europa’s surface into the atmosphere and ionosphere and understanding how Europa influences its local space environment and Jupiter’s magnetosphere.
The Mass Spectrometer for Planetary Exploration (MASPEX) will determine the composition of the surface and subsurface ocean by measuring Europa’s extremely tenuous atmosphere and any surface materials ejected into space.
The Surface Dust Mass Analyser (SUDA), a second mass spectrometer that will measure the composition of small solid particles ejected from Europa, providing the opportunity to directly sample the surface and potential plumes on low-altitude flybys. The instrument is capable of identifying traces of organic and inorganic compounds in the ice of ejecta.
The ninth instrument will be a magnetometer, although this has yet to be sourced – the dedicated instrument, called Interior Characterisation of Europa using Magnetometry (ICEMAG) was cancelled due to spiralling costs and development complications. It will be replaced by a more “off the shelf” system that will be less sensitive than ICEMAG, but the mission team are confident they can compensate for this be more frequent re-calibration operations during the mission.
A pair of composite images of the side of Europa facing away from Jupiter. The rust / brown colour is likely the result of sulphur ejected from Jupiter’s inner moon Io being deposited on Europa by Jupiter’s radiation belt. The lines appear to be cracks in the surface, created by gravitational flexing of the Moon, which causes newer ice to form, indicative of water being forced upwards. Additionally, the yellow staining appears to be sodium chloride – the same as found in our own oceans – deposited on Europa as a result of material being ejected through the cracks. Credit: NASA/JPL / University of Arizona
Early concepts for a Europa mission – as noted above – included a lander – and possibly even a drilling mechanism and an automated submarine that could potentially be dropped under the ice and explore the ocean under it. These ideas were dropped – perhaps wisely – until more is known about the structure and thickness of the surface ice and exactly what lies beneath it. However, Europa Clipper has some additional payload capacity – around 250 kg – and NASA has been seeking ideas on what might be flown; some of the suggestions have included by a payload of supporting CubeSats or a small-scale lander.
While the Europa Clipper mission won’t actually orbit Europa, the multiple fly-bys will enable it to achieve almost global coverage of the moon, allowing for the widest amount of data to be gathered. This will be transmitted back to Earth in the 7-day periods between each close fly-by.
Currently, the mission launch date has yet to be finalised, and this in part depends on the selected launch vehicle. The preferred launcher is NASA’s upcoming Space Launch System (SLS). If used, this would see the mission launched in 2023, with the booster powerful enough to put Europa Clipper on a 3-year direct flight to Jupiter. However, there is no guarantee that SLS will be available in the proposed time frame, so NASA is also looking to use a commercial vehicle such as the SpaceX Falcon Heavy or the ULA Delta IV Heavy. Either of these would allow the mission to launch in 2022, but as they are less powerful than SLS, they would require Europa Clipper use 3 gravity assist manoeuvres, two at Earth and one at Venus, in order to send it on its way, increasing the transit time to Jupiter to 6 years.
The 14 new surface feature names (in yellow) approved for Pluto by the International Astronomical Union on August 8th, 2019. The names in white were approved by the IAU in 2017. Credit: NASA / JHU/APL
On August 8th, 2019, the International Astronomical Union (IAU) approved the names for 14 more significant features on the surface of Pluto, imaged by the New Horizons space vehicle as it flew past the Pluto-Charon system in 2015.
The IAU claimed the authority to officially name or approve the name of planets, dwarf planets, moons, asteroids and planetary features in our solar system during its inaugural General Assembly, held in Rome in May 1922, 3 years after it had been formed by the founding nations of Belgium, Canada, France, Great Britain, Greece, Japan, and the United States, and by which point its membership had grown to 19 nations around the world (today membership stands at 82 nations).
As the sole authority, it means that any names given to things like planetary surface features – such as “Mount Sharp” on the surface of Mars are entirely unofficial, hence why they are referred to in quotes in these Space Sunday articles. The IAU may determine names on things like surface features entirely by itself (as is the case with “Mount Sharp”, which is officially designated Aeolis Mons), or they may take recommendations from other organisations or groups.
In the case of the 14 names first assigned to features on Pluto by the IAU in 2017, the organisation ratified the suggestions made by the New Horizons mission team. Keeping with this “tradition”, the August 8th, 2019 announcement of the 14 “new” names for surface features first employed by the mission team.
The first 14 names to be approved by the IAU (2017) for features on Pluto include the Tombaugh Regio, named for Clyde Tombaugh, who first identified Pluto as a planetary body; the great frozen nitrogen lake of Sputnik Planitia, and the Hillary and Tenzing mountains, named for the two men formally recorded as the first to reach the summit of Mount Everest. Credit: NASA / JHU/APL
All 14 represent people and missions that contributed to the understanding of Pluto and the Kuiper Belt, as well as drawing on figures from mythology and aerospace exploration in general. They cover a range of surface features on Pluto images by the New Horizons vehicle as it dashed through the Pluto-Charon system that include entire regions of the planet and items such as mountain ranges, plains, valleys and craters. They comprise (in alphabetically order):
Alcyonia Lacus, possibly a frozen nitrogen lake, it is named for the “bottomless” lake in the vicinity of Lerna, Greece, and regarded as one of the entrances to the underworld in Greek mythology.
Elcano Montes, a mountain range named for Juan Sebastián Elcano (1476–1526), the Spanish explorer who in 1522 completed the first circumnavigation of the Earth (a voyage started in 1519 by Magellan).
Hunahpu Valles, a system of canyons named for after one of the Mayan Hero Twins who defeated the lords of the underworld in a ball game.
Khare crater honours planetary scientist Bishun Khare (1933–2013), who specialised in the chemistry of planetary atmospheres and who published several seminal papers on tholins, the organic molecules that probably account for the darkest and reddest regions on Pluto.
Kiladze crater is named for Rolan Il’ich Kiladze (1931–2010), who made pioneering early investigations the dynamics, astrometry and photometry of Pluto.
Lowell Regio, is a large region honouring Percival Lowell (1855–1916), founder of the Lowell Observatory and organiser of the search that eventually led Clyde Tombaugh to locate Pluto.
Mwindo Fossae, a network of long, narrow depressions named for the Mwindo Epic of the Nyanga people.
Piccard Mons, a mountain and suspected cryovolcano named for Swiss inventor and physicist and high altitude balloon pioneer, Auguste Piccard (1884–1962).
Pigafetta Montes, a mountain range honouring Antonio Pigafetta (c. 1491–c. 1531), the Italian scholar and explorer who chronicled the discoveries made during the first circumnavigation of the Earth, aboard Magellan’s ships.
Piri Rupes, a range of cliffs named for Piri Reis (also Ahmed Muhiddin Piri c. 1470–1553), an Ottoman navigator and cartographer known for his world map. He also drew some of the earliest existing maps of North and Central America.
Simonelli crater, name after astronomer Damon Simonelli (1959–2004), whose wide-ranging research included the formation history of Pluto.
Vega Terra, a large land mass named after the Soviet Vega 1 and 2 missions, the first spacecraft to fly balloons on another planet (Venus) and to image the nucleus of a comet (1P/Halley).
Venera Terra, named for the Venera missions sent to Venus by the Soviet Union from 1961–1984; they included the first human-made device to enter the atmosphere of another planet, to make a soft landing on another planet and to return images from another planetary surface.
A computer-generated image showing New Horizons’ location in our solar system on August 10, 2019. The green line shows where the vehicle has travelled since its 2006 launch, the red indicates its future path. This perspective is from above the Sun and “north” of Earth’s orbit. Credit: JHU/APl
Since its flyby of the Pluto-Charon system, the New Horizons vehicle has continued its voyage out through the Kuiper Belt. Most of this has been with the vehicle in a state of hibernation to conserve power, however, in January 2019, the craft encountered Kuiper Belt Object (KBO) Ultima Thule, aka 2014 MU69 (see my January 28th 2019 Space Sunday article), and data from that encounter is still being transmitted back to Earth.
Currently, the New Horizons mission is funded until April 2021, and may well be extended beyond that date. The vehicle’s radioisotope thermoelectric generator (RTG), which uses the heat from the radioactive decay of plutonium 238 to provide it with electrical power, is expected to provide sufficient energy for its science instruments until the mid-to-late 2030s. So the science team responsible for the mission at the John Hopkins University Applied Physics Laboratory are currently seeking potential KBO targets the craft could fly by in the mid or late 2020s.
Ultima Thule from a distance of 6,700 km, January 1st, 2019. Credit: NASA / JHU/APL / SwRI
Should the vehicle retain sufficient power for some of its instruments, it may be able to study the outer heliosphere (the “bubble” of space surrounding our solar system and created by the outward flow of energise particles from the Sun) in the late 2030s. If it does, it will add to the data gathered on that distant region of space, 100+ AU from Earth (1 AU = the average distance of the Earth from the Sun) by the Voyager spacecraft.
Parker Solar Probe: One Year In
August 12th, 2019, marked the first anniversary of NASA’s Parker Solar Probe. As I reported in Space Sunday: to touch the face of the Sun, this is an ambitious mission to repeatedly fly through the Sun’s corona – the hazardous region of intense heat and solar radiation in the Sun’s atmosphere that is visible during an eclipse – to gather data that could help answer questions about solar physics that have puzzled scientists for decades.
Named for Eugene Parker, the physicist who first theorised the solar wind, the constant outflow of particles and magnetic fields from the sun, the mission is now into its third orbit of the Sun, and due to make a further close solar approach on September 1st, 2019.
The spacecraft carries four suites of scientific instruments to gather data on the particles, solar wind plasma, electric and magnetic fields, solar radio emission, and structures in the Sun’s corona. This information will help scientists unravel the physics driving the extreme temperatures that make the corona hotter than the “surface” of the Sun – and the mechanisms that drive particles and plasma out into the solar system.
So much information has been gathered by the probe during its first two orbits of the Sun that the mission team on Earth is still analysing it. They hope to have the first results available before the end of the year – not that they are complaining!
We’re very happy. We’ve managed to bring down at least twice as much data as we originally suspected we’d get from those first two perihelion passes.
– Nicky Fox, director of NASA’s Heliophysics Division
An artist’s impression of the Parker Solar Probe swinging around the Sun at a distance of 6.2 million km (3.85 million mi) . Credit: NASA
Nor is that all; the probe’s elliptical 170-188 day orbit means that it has just 11 days per orbit in which to gather data – and these coincide with perihelion, when the craft must withstand temperatures of around 1,370ºC (2,500ºF). To achieve this, the probe is equipped with a 2.3m hexagonal solar shadow-shield that performs three tasks: it absorbs and reflects sunlight away from the vehicle whilst also preventing radiation penetrating its instrument bay and burning-out its circuits and instruments (incident solar radiation at perihelion is approximately 475 times the intensity at low Earth orbit) and also casting a long shadow in which the rest of the vehicle can remain relatively “cool”. Data on the shadow-shield and from within the vehicle as it passes through the corona reveal the shield is working better than anticipated.
So, with another six years of its planned 7-year primary mission, the Parker Solar Probe is set to revolutionise our understanding of the Sun’s corona and the mechanisms powering it.
The data we’re seeing is showing us details about solar structures and processes that we have never seen before. Flying close to the sun—a very dangerous environment—is the only way to obtain this data, and the spacecraft is performing with flying colours.
– Nour Raouafi, Parker Solar Probe project scientist, JHU/APL
June 2011: a pristine assembled MSL Curiosity rover sits within its assembly clean room at NASA’s Jet Propulsion Laboratory prior to being stowed and mounted within its delivery system in preparation for its December 2011 launch to Mars. Credit: NASA/JPL
Seven years ago on August 6th, 2012 at 05:17 UTC, NASA’s Mars Science Laboratory rover Curiosity arrived in Gale Crater on Mars. I’ve covered the progress of the mission throughout (just follow my MSL / Curiosity tag), and those articles in fact gave birth to this Space Sunday column; but it’s been a while since I’ve last updated on things.
Since its arrival on Mars, Curiosity has driven a total of 21 km (13 mi) from its landing point to the base of the crater’s central mound, Aeolis Mons, and has ascended 368 metres (1,207 ft) up the side of the mound, which NASA informally call “Mount Sharp” to its current location.
How Curiosity Reached Mars, (1) cruise stage – provided power and data collection during flight from Earth to Mars; (2) aeroshell protecting rover and skycrane during journey and during entry into the Martian atmosphere, with parachute system (6); (3) the skycrane used to winch the rover down to the ground whilst hovering a few metres in the air; (4) the rover in its stowed configuration; (5) the heat shield that protected the vehicle during its entry into the Martian atmosphere. Credit: NASA/JPL
Along the way, Curiosity has revealed a lot about Mars – including confirmation that Gale Crater has been host to multiple bodies of water during its early life, and that the conditions were suitable for microbial life to have potentially arisen on the planet.
Nor did the rover have to wait to make the discovery: it did so literally within weeks of its hair-raising arrival when it had barely started on its journey and was exploring an ancient riverbed on the floor of Gale Crater (dubbed “Yellowknife Bay”), when analysis of samples gathered revealed all the essential ingredients which – if mixed with water (that once flowed through the riverbed) – might have given life a kick-start and to have been enough to possibly sustain it during the warmer, wet periods of Mars’ early history.
As well as this, Curiosity has revealed much about the ancient conditions on Mars, has found hematite (which requires the presence of water to form), done much to reveal atmospheric processes at work on the planet, and helped track Martian weather and climate processes.
There have been a few causes for concern along the way. Early on in the mission it was revealed that the rover’s six aluminium wheels had suffered more wear and tear than had been anticipated, prompting some changes to the rover’s route as it approached “Mount Sharp”.
Most particularly, the rover’s drill mechanism has had its share of issues, some of which have required changes to how the drill is operated.
However, none of this has really impacted on the rover’s mission – in fact, Curiosity has recently obtained its 22nd drill sample from Mars, as it examines a region the mission team call the “Clay Unit”, one of several closely packed areas with strong differentiators scientists want to examine. Clay forms in the presence of water, and the area has sufficient enough clay deposits to be detected from orbit, and Curiosity has recovered samples with the highest amounts of clay minerals found to date by the mission.
This area is one of the reasons we came to Gale Crater. We’ve been studying orbiter images of this area for 10 years, and we’re finally able to take a look up close.
– Kristen Bennett, U.S. Geological Survey and co-lead for Curiosity’s clay-unit campaign
A panoramic view of “Teal Ridge” in the “Clay Unit” showing sharp differentiations in rock and surface material that suggest the evolution of a lake-like environment. June 18, 2019, the 2,440th Martian day, or sol, of the mission. Credit NASA/JPL
Quite why this particular area is so rich in clay deposits is unclear, but the area is home to complex geologic features, such as “Teal Ridge” and “Strathdon,” a rock made of dozens of sediment layers that have hardened into a brittle, wavy heap. Unlike the thin, flat layers associated with lake sediments Curiosity has studied, these wavy layers in these features suggest a more dynamic environment. Wind, flowing water or both could have shaped this area.
Both “Teal Ridge” and “Strathdon” represent changes in the landscape suggestive of the evolution of the ancient lake environment. This is further exemplified by the area above the “Clay Unit”, and towards which Curiosity is slowly making its way. It’s an area rich is sulphate deposits, indicative that it was drying up or becoming more acidic in ancient times whilst the lower slopes were still rich in water.
The Clay and Sulphate bearing regions on “Mount Sharp” and the proposed path Curiosity is following through them. Credit: NASA/JPL
Cutting down slope through the “Sulphate Unit” is the Gediz Vallis and Ridge, which appears to have been form by water running down “Mount Sharp” at some period after both the Clay Unit and Sulphate Units before spreading into the “Greenheugh Pediment”. This points to the area having seen some considerable changes as a result of climate changes on Mars.
We’re seeing an evolution in the ancient lake environment recorded in these rocks. It wasn’t just a static lake. It’s helping us move from a simplistic view of Mars going from wet to dry. Instead of a linear process, the history of water was more complicated. It’s finally being able to read the paragraphs in a book — a dense book, with pages torn out, but a fascinating tale to piece together.
– Valerie Fox, Division of Geological and Planetary Sciences, Caltech
Curiosity is powered by a radioisotope thermoelectric generator (RTG) that uses a core of plutonium-238. The heat given off by the decay of the isotope is converted into electric voltage by thermocouples and stored within two lithium-ion batteries that directly power the rover’s systems. This ensures the rover obtains constant power during all seasons and through the day and night, with waste heat is also passed through the vehicle’s interior to keep systems and instruments at their operating temperature and without the need for additional electric heating systems.
However, over time, the amount of electrical voltage the RTG can generate decreases. Overall, Curiosity’s RTG is expected to provide sufficient power (100+ Watts) to run all of the rover’s systems for 14 years – so 2019 marks the half-way point. Which is not to say that Curiosity only has seven more years of operations. Rather, it means that in around 7 years power generation is going to fall below the 100 watts mark, and it may become necessary for rationing power between systems on the rover, reducing some of its capacity.
The mission included the first stage of a privately-funded initiative to transfer living DNA to the Moon – a kind of “Noah’s Ark Mark II”, providing a repository from which plants and animals could be regenerated to repopulate the Earth should a catastrophe akin to a flood of biblical proportions overtake the planet. In particular for this first phases of the project, a 30-million-page archive of human history viewable under microscopes, as well as human DNA were carried by the lander in a DVD-like “Lunar Library” – which also includes tardigrades.
The tardigrade. Credit: 3DStock/Shutterstock
Science fiction fans might recognise this name from the television series Star Trek: Discovery. However, far from being the stuff of sci-fi shows and stories, tardigrades are very real (if a lot, lot smaller than their Star Trek “breathren”) and also exceptionally hardy.
Known colloquially as water bears or moss piglets, tardigrades are a phylum of water-dwelling eight-legged segmented micro-animals that can be found almost anywhere on Earth, from the tops of mountains to the bottoms of the oceans, from the tropical stew of rain forests to the frozen wastes of the polar regions. They can survive extremes of temperature and pressure (both high and low), air deprivation, radiation, dehydration, and starvation and exposure to outer space.
The tardigrades were stored dehydrated tardigrade – which puts them into a state of suspended animation – and “encased in an epoxy of Artificial Amber”. In this state, they could in theory be revived if exposed to heat and moisture. But even without these, the tardigrade could survive for years on the Moon – specimens have been recovered after being in a dehydrated state for decades. Such is the design of the unit in which they are stored, those responsible for the project believe it “highly likely” it survived Beresheet’s impact on the surface of the Moon.
Sadly, it is unlikely we’ll ever get to know if this is the case; the crash point for the Israeli lander puts in it in an area of the Moon’s south polar region far removed from any planned destinations for NASA’s Artemis missions, making recovery very unlikely.
Steam Powered Satellites and Autonomous Exploration
Am August press release from NASA reveals the agency has completed tests of what is effectively the world’s first steam-propelled satellite in Earth’s orbit. Admittedly, it not a particularly big vehicle being tested – it is small enough to compete with a box of tissues – but the test is an important step in examining technologies for future automated space exploration.
The test took place on June 21st, 2019, and was part of a coordinated manoeuvre between two CubeSats operating in low-Earth orbit, carried out as part of NASA’s Optical Communications and Sensor Demonstration (OCSD) mission.
The steam-propelled CubeSat in an artist’s impression. Credit: NASA
The two tiny vehicles were orbiting the Earth around 9 km (5.8 mi) apart when they automatically established a radio communications cross-link with one another. One then ordered the other to fire its thruster and close the gap between them. Rather than using a traditional hypergolic propellant or inert gas, both of the CubeSats carry small tanks of water which can be heated to produce steam that is ejected through an engine nozzle to generate propulsion.
This demonstration is important on two counts. The first is that it shows the potential for a series of small satellite drones to command one another to carry out assorted operations entirely independently of control from Earth. Such a group of drones could work cooperatively on a mission – say a survey of the asteroid belt or the icy moons of Jupiter. They could operate in unison, commanding one another, or under the autonomous control of a “mother ship” that could have facilities for storing (and returning) samples to Earth.
The second is that, in using water as a means of propulsion, these vehicles could in theory be easily fuelled and refuelled with water – water which might in turn be obtained from the frozen bodies these craft are exploring.
Demonstrations such as this will help advance technologies that will allow for greater and more extended use of small spacecraft in and beyond Earth-orbit. It is exciting to think about the possibilities enabled with respect to deep space, autonomously organizing swarms of small spacecraft.
– Roger Hunter, programme manager,
NASA Small Spacecraft Technology Programme
Perseid Meteor Shower
Every July / August, the Earth passes through a haze of stellar debris left by Comet 109P/Swift-Tuttle. The result is of this passage is the Perseid meteor shower (called this because they appear to originate from the constellation of Perseus), is one of the brightest meteor displays one can see in the northern hemisphere. The shower tends to last around a month, from July 17th (ish) through to August 24th.
Observing the Perseids in 2019
This year, the peak period for activity should be August 12th and 13th, when between 60 and 100 meteors an hour might be visible streaking across the night sky. In Europe, the best time to see them is after midnight, while America gets it a little easier and earlier. To check time in your location try timeanddate.com, which should give local observation times.
Unfortunately, the moon will be very close to full on the night of the peak, and this will affect the visibility of the fainter meteors. Of course, you’ll also need to be somewhere that’s dark enough to see the night sky without it being blotted too heavily by surrounding Earthly light pollution.
To help people observe the peak period, there are a number of planned livestreams on the web – including the two below.
“Flight”: Christopher C. Kraft Jr. (February 1924 – July 2019), the man who created NASA’s mission control and the role of the flight director. Credit: NASA
During the celebrations marking the 50th anniversary of the Apollo 11 mission in July, came a note of sadness: the passing of Chris Kraft.
This is a name that may not be familiar to some, but Christopher C. Kraft, Jr., was one of the most influential figures of NASA’s pioneering early years of America’s human space flight, who joined the agency from its forebear, the National Advisory Committee for Aeronautics (NACA).
Born in Virginia in February 1924, to Bavarian immigrants, Kraft began his studies at Virginia Polytechnic Institute and State University (Virginia Tech) studying aeronautical engineering. During this time he applied to join the US Navy, but was rejected due to an injury to his right hand that occurred during childhood. He graduated in December 1944 with a Bachelor of Science degree.
On graduation, he applied to both the Chance Vought aircraft company and NACA. On arrival at the former on his first day of work, he was told that he could not be hired without his birth certificate, which he had not brought with him. Annoyed, he returned home and accepted the offer from NACA instead.
At NACA he was assigned to the flight research division, working under Robert Gilruth, who was to become his mentor. Most of Kraft’s work was theoretical – although it did lead him to be the original discoverer of wingtip vortices causing the majority of turbulence behind an aircraft. While he enjoyed it, he also found it taxing to the point of considering leaving, when the NACA was subsumed by NASA.
Kraft (l) and mentor Robert Gilruth (r) celebrate the first orbital rendezvous between two crewed vehicles, Gemini 6 and 7, December 1965. Astronaut L. Gordon Cooper Jr stands behind them, centre, with arms folded. Credit: NASA
Gilruth then invited Kraft to join a new project he was heading – the Space Task Group – charged with putting a man in orbit. As a result, Kraft became one of the original thirty-five engineers to be assigned to Project Mercury. In his new role, he was assigned to the flight operations division at NASA, charged with determining how the Mercury missions would be managed and operated from the ground. He was reporting in to Chuck Matthews, who essentially passed off the division’s requirements to Kraft in a throwaway comment:
Chris, you come up with a basic mission plan. You know, the bottom-line stuff on how we fly a man from a launch pad into space and back again. It would be good if you kept him alive.
Kraft realised that just like test pilots, whom he had supported through the X-1 flight programmes, astronauts would need a system of communications and support back on Earth during critical phases of the mission. He also knew they would also require a ground-based tracking system and instrumentation for the telemetry of data from the spacecraft. Through this, he came up with the idea of a single control centre to monitor and operate missions in real-time; a concept never before tried.
I saw a team of highly skilled engineers, each one an expert on a different piece of the Mercury capsule. We’d have a flow of accurate telemetry data so the experts could monitor their systems, see and even predict problems, and pass along instructions to the astronaut.
– Chris Kraft, Flight: My Life in Mission Control, 2001
Within this structure, Kraft particularly identified the need for a single individual who would have overall control and coordination over the flight centre engineers, and make the real-time decisions about the conduct of the mission. He called that role the Flight Director, and nominated himself as the man for the role.
The first iteration of the mission control concept was the Mercury Control Centre at Cape Canaveral. During this time, Kraft continued to define and refine the role of the flight director, gaining the singular title Flight as a mark of respect, although his own stubbornness that could make him something of a controversial figure in the eyes of management – but not enough to prevent him being awarded the NASA Outstanding Leadership Medal on the recommendation of the NASA Administrator, and awarded by President John F. Kennedy.
During Mercury, Kraft selected and trained three engineers to become the first generation of flight directors with him: Glynn Lunney, John Hodge and man who also grew into a legend as he followed Kraft, Gene Kranz. As the more intensive Gemini missions took place, Kraft took on a new role: head of mission operations, but remained entirely hands-on with the flight director programme, continuing to select and train other flight directors and continuing a flight director in his own right.
Kraft, lower right, with his hand-picked team of original NASA flight directors, Gene Krantz (bottom left), Glynn Lunney, (top left) and John Hodge (top right). Credit: NASA
Mid-way through the Gemini programme, Kraft was asked to oversee the design and implementation of the brand-new mission control centre that would form a part of the new Manned Spacecraft Centre, near Houston, Texas (now the Johnson Space Centre), which would become the nerve centre for all of NASA’s human spaceflight operations.
Kraft, Lunney and Kranz worked directly on the requirements for the new mission control centre, located at Building 30 at the new space centre, liaising with contractors and determining the design of the two primary Mission Operations Control Rooms (each referred to as MOCR, or “moe-ker”).
By the mid-1960s, Kraft was made Director of Flight Operations, and closely involved in planning the Apollo programme. He joined with Gilruth, now the head of the Manned Spacecraft Centre and possibly the most powerful man in NASA next to the agency’s administrator, George Low, the manager of the Apollo Spacecraft Programme Office and Donald Kent “Deke” Slayton, the head of the Astronaut Office, to take on an entirely unofficial, but essential role:
The four of us … had become an unofficial committee that got together often in Bob’s [Gilruth’s] office to discuss problems, plans and off-the-wall ideas. Not much happened in Gemini or Apollo that didn’t either originate with us or with our input.
– Chris Kraft, Flight: My Life in Mission Control, 2001
Kraft at the flight director’s console during Gemini IV, June 1965, despite having been promoted to Director of Flight Operations. Credit: NASA
In 1969, Kraft officially became Gilruth’s deputy in running the Manned Spacecraft Centre, and succeeded him as overall facility director in January 1972. He remained in that role past his due retirement in 1980, remaining firmly embedded in the space shuttle programme. However, his stubborn and outspoken nature in matters relating to that programme brought him into conflict with NASA Administrator James M. Beggs and others, and he suddenly announced his belated retirement at the end of 1982.
Kraft indirectly returned to the shuttle programme in 1994, when he was appointed chairman of an independent review committee with the remit to investigate ways in which NASA could make that programme more cost effective. His report, published in February 1995, recommended NASA’s should outsource shuttle operations to a single private contractor.
Christopher J. Kraft Jr., February 1924-July 2019 in his official NASA portrait, 1979. Credit: NASA
More contentiously, it was sharply critical of the post-Challenger accident safety regime at NASA, claiming it was “duplicative and expensive”, while claiming the shuttle had become “a mature and reliable system”.
NASA’s own Aerospace Safety Advisory Panel responded that, “the assumption that the Space Shuttle systems are now ‘mature’ smacks of a complacency which may lead to serious mishaps.” Nonetheless, responsibility for shuttle operations was turned over to United Space Alliance.
In 2003, the investigation into the Columbia accident, directly cited the recommendations made by Kraft’s committee as potentially contributing to that accident, by encouraging NASA to view the shuttle as an operational, rather than experimental vehicle and distracting attention from continuing engineering anomalies. In typical form, Kraft defended his report, insisting thespace shuttle was “the safest space vehicle ever built”.
Kraft received numerous awards throughout his career, and in on April 4th, 2011, he was guest of honour at a ceremony at Johnson Space Centre’s Building 30 Mission Control Centre when it was renamed the Christopher C. Kraft, Jr., Mission Control Centre, in recognition of the facility’s 50 years managing US human space flight, and Kraft’s unique place in both NASA’s and the building’s histories.
Christopher Kraft passed away on July 22nd, 2019 at the age of 95 and leaving his wife of 69 years, Betty Anne, and son and daughter Gordon and Kristi-Anne, and their families.
A GSLV Mk III lifts-off with the Chandrayaan-2 mission from India’s Satish Dhawan Space Centre, Sriharikota, 09:13 UTC, Monday, July 22nd, 2019. Credit ISRO
The Indian Space Research Organisation (ISRO) successfully launched its Chandrayaan-2 mission to the lunar south pole on Monday, July 22nd, after suffering a week’s day to the schedule. This is an ambitious mission that aims to be the first to land in the Moon’s South Polar region, comprising three parts: an orbiter, a lander and a rover.
Although launched atop India’s most powerful rocket, the GSLV Mk III, the mass of the mission means it cannot take a direct route to Mars, as the upper stage isn’t powerful enough for the mass. Instead, Chandrayaan-2 was placed into an extended 170km x 39,120 km (105 mi x 24,300 mi) elliptical orbit around the earth. For the next month, the orbiter will gradually raise this obit until it reaches a point where lunar gravity becomes dominant, allowing Chandrayaan-2 to transfer into a similarly extended lunar orbit before easing its way down to a 100 km (60 mi) circular polar orbit around the Moon, which it is scheduled to achieve seen days after translating into its initial lunar orbit.
How Chandrayaan-2 will reach the Moon and its operational orbit. Credit: ISRO
During this period, the combined vehicle will carry out multiple surveys of the Moon’s survey, focusing on the South Pole. It will also release the 1.47-tonne Vikram lander (named for Vikram Sarabhai, regarded as the father of the Indian space programme) which will make a soft decent to the lunar surface, which will take several days prior to making a soft landing.
The orbiter vehicle is designed to operate for a year in its polar orbit for one year. It carries a science suite of eight systems, including the Terrain Mapping Camera (TMC), which will produce a 3D map for studying lunar mineralogy and geology, an X-ray spectrometer, solar X-ray monitor, imaging spectrometer and a high-resolution camera.
The Vikram lander, with four science payloads, will communicate both directly with Earth and the orbiter. It will also facilitate communications with the Pragyan rover, which will be deployed within hours of the self-guiding lander touching down. Between them, the lander and rover carry 5 further science experiments and both are expected to operate for around 14 days.
Testing the deployment of the Pragyan rover from the Vikram lander. Credit: ISRO
Craters in the South Polar region lie in permanent shadow and experience some of the coldest temperatures in the solar system and NASA’s Lunar Reconnaissance Orbiter (LRO) has revealed they contain frozen water within them, water likely unchanged since the early days of the Solar System, and thus could hold clues to the history of the Solar System – hence the interest in visiting the region and learning more. The frozen water is also of interest to engineers as it could be extracted to provide water for lunar base; water that could be used for drinking, or growing plants and could also me split to produce oxygen and hydrogen – essential fuel stocks.
The Chandrayaan-2 mission marks a significant step forward for India’s space ambitions; assuming the Vikram lander is successful, the country will become only the forth nation to land on the Moon after the United States, Russia and China. As a part of its expanding activities in space, the country hopes to fly it first astronauts into space in 2022 and have an operational space station by the end of the 2020s.
2019 OK
No, I’m not making a statement about the year – that’s the name of a chunk of space rock measuring 57 to 130m (187 to 42ft) across that passed by Earth at a distance of around 73,000 km (45,000 mi), putting it “uncomfortably close” to the planet. What’s more, we barely released it was there: 2019 OK was positively identified by the Southern Observatory for Near Earth Asteroids Research (SONEAR), just a couple of days prior to is passage past Earth, and was confirmed by the ASAS-SN telescope network in Ohio, leaving just hours for an announcement of its passage to be made.
Since then, the asteroid’s orbit has been tracked – forward and back (which revealed it had been previously spotted by observatories, but its small size and low magnitude meant its significance wasn’t realised). These observations confirmed 2019 OK is a reactively short-period object, orbiting the Sun every 2.7 years. It passes well beyond Mars before swinging back in and round the Sun, crossing the Earth’s orbit as it does so. However, while it may pass close to Earth on occasion, it’s highly unlikely it will ever strike us.
Credit: NASA
It does, however, remind us that near-Earth objects (NEOs) are common enough to be of concern; 2,000 were added to the list 2017 alone. The size of 2019 OK reminds us that there are more than enough of them to be of a significant enough size to pose a genuine threat.
In 2013, an asteroid measuring just 20m across entered the atmosphere to be ripped apart at an altitude of around 30 km above the Russian town of Chelyabinsk. The resultant resulting shock wave shattered glass down below and injured more than 1,000 people. 2019 OK is at a minimum 2.5 times larger than the Chelyabinsk object – and possibly as much as 10 times larger, putting it in the same class of object that caused the Tunguska event of 1908, when 2,000 sq km (770 sq mi) of Siberian forest was flattened by an air blast of 30 megatons as a result of a comet fragment breaking up in the atmosphere.
Hence why observatories such as SONEAR, ASAS-SN telescope network, the Catalina Sky Survey, Pan-STARRS, and ATLAS and others attempt to track and catalogue NEOs. The more of them we can located and establish their orbits, the more clearly we can identify real threats – and have (hopefully) a lead time long enough to take action against them.
A computer model show the passage of 99942 Apophis on April 13th, 2029. The blue dots represent satellites in orbit around Earth and the pink line the orbit of the International Space Station. Credit: NASA JPL
Oh, and if you thought 2019 OK was big, consider 99942 Apophis. It’s around 400-450m across, and will swing by Earth at a distance of just 31,000 km on – wait for it – Friday, April 13th, 2029 (so get ready for a lot of apocalyptic predictions in the months leading up to that date!).
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