Space Sunday: mini mission updates

An artist’s impression of the Psyche spacecraft en route to 16 Psyche. Credit: NASA

Due to launch in just under 2 months, on or shortly after October 5th, 2023, NASA’s Pysche mission is intended to explore the origin of planetary cores by studying the metallic asteroid of the same name.

The 14th mission in NASA’s Discovery programme, the spacecraft is currently going through the last of its pre-launch preparations, the latest being the installation and folding of its massive solar arrays.

With a total span of almost 25 metres and covering a total area of 75 square metres, these are among the largest arrays used on a NASA deep-space mission. They will be capable of generating 20 kilowatts of power during the early phases of the mission as the spacecraft departs Earth, where they will be primarily used for the purposes of vehicle thrust. However, Psyche is so far from the Sun that by the time the craft arrives, they will only be able to generate around 2 kilowatts – enough to boil two kettles side-by-side.

Technicians begin to retract one of the two solar arrays following its installation on NASA’s Psyche spacecraft. Credit: NASA/Kim Shiflett

For propulsion, the spacecraft will use four Hall-effect thrusters (HETs). Based on the discovery by Edwin Hall after whom they are named, these are a form of ion propulsion in which the propellant – most often  xenon or  krypton gas – is accelerated by an electric field. They provide an efficient thrust-to-propellant load ratio, allowing the spacecraft utilise a minimum propellant load – around a tonne – for the 5 year 10 months transit to asteroid 16 Psyche and the 21-month primary science mission.

The overall thrust produced by the HETs is equivalent to holding a single AA battery in the hand. However, as they can run for extended periods, they will be able to gently accelerate the spacecraft to 200,000 km/h during the 4 billion kilometre cruise out to the asteroid belt. They will also provide sufficient thrust to allow the spacecraft to slow itself and enter orbit around the asteroid in readiness to start its science mission.

16 Psyche is the heaviest known M-type asteroid – those with higher concentrations of metal phases (e.g. iron-nickel) than other asteroids – in the solar system. It was in 1852 by Italian astronomer Annibale de Gasparis, who named it for the Greek goddess Psyche, with the “16” prefix indicating it was the sixteenth minor planet to be discovered.

An artist’s rendering of 16 Psyche based on radar studies of the asteroid and albedo-based features witnessed through imaging. Credit: Peter Rubin/NASA

Initially, it was thought that asteroid was the exposed iron core of a protoplanet, exposed after a violent collision with another object that stripped off its mantle and crust. However, more recent studies lean heavily towards ruling this out – but it still might be a fragment of a planetesimal smashed part in the very earliest days of the solar system’s creation. As such, studying the asteroid might answer questions about planetary cores and the formation of our own planet.With the solar arrays installed and stowed, the next significant milestone for the mission will be the loading of the xenon propellant, which will occur over a two-week period starting in mid-August. This will be followed by the spacecraft being mated with its payload mount and then integrated into the upper stage of the SpaceX Falcon Heavy which will launch the mission from Kennedy Space Centre’s Pad 39B.

Euclid Arrives at L2 and Starts Commissioning Tests

The European Space Agency’s (ESA’s) Euclid space telescope has arrived in orbit around the Earth-Sun L2 Lagrange point, and commissioning of its science instruments has commenced.

As I noted in Space Sunday: a “dark” mission, recycling water and a round-up, Euclid is a mission intended to aid understanding of both dark matter and dark energy – neither of which should be confused with the other. Euclid will do this by creating a “3D” map of the cosmos around us, plotting the position of some two billion galaxies in terms of their position relative to the telescope and the redshift evident in their motion.

Animation of Euclid (purple) in a halo orbit around the the Earth-Sun L2 position (light blue), as seen from “above” and following launch from Earth (dark blue). Credit: Phoenix777 utilising data from ESA / NASA

From this, astronomers will be able to study the clustering effects of dark matter, the cosmic expansion of dark energy, and how cosmic structure has changed over time. It will be the largest and most detailed survey of the deep and dark cosmos ever done.

Following a 30-day transit from Earth, Euclid entered into orbit around the Earth-Sun L2 Lagrange point, 1.5 million km from Earth, at the end of July, and commissioning of its instruments – which had undergone power tests whilst en-route – commenced almost at once, with early result being released.

Over the next 6 years, Euclid will observe the extragalactic sky (the sky facing away from the bulk of our own galaxy) in what is called a “step and stare” method: identifying a section of sky and training both of its camera systems, one of which images in visible wavelengths and the other in infrared, before moving on to the next, generating “strips” on imaged squares.

The grid-like “step and stare” observation method Euclid will use to survey the extragalactic sky. Credit: NASA

In doing so, Euclid will capture light from galaxies that has taken up to 10 billion of the universe’s estimated 13.8 billion-year lifespan to reach us. In doing so, it will measure their shape and the degree of red shift evident, whilst also using the effects of gravitational lensing on some to reveal more data about them.

The data gathered is intended to help astrophysicists construct a model to explain how the universe is expanding which might both explain the nature and force of dark energy and potentially offer clues as to the actual nature of dark matter – the mass of which must be having some impact on dark energy as it pushes a the galaxies.

Commissioning images for Euclid’s near-infrared camera. Credit: ESA

In all, it is anticipated that Euclid will produce more than 170 petabytes of raw images and data during its primary 6-year mission, representing billions of stars within the galaxies observed. This data will form a huge database that will be made available globally to astronomers and researchers to help increase our understanding of the cosmos and in support for current and future missions studying the universe.

Curiosity Celebrates 11 Years on Mars by Completing Tough Challenge

Since arriving on Mars in February 2021, the Mars 2020 mission with Perseverance and Ingenuity has tended to overshadow NASA’s other operational rover mission on Mars, that of the Mars Science Laboratory Curiosity, which arrived within Gale Crater on August 6th, 2011.

In that time, the mission has scored success after success, doing much to reveal the water-rich history of the crafter – and the history of Mars as a whole. For the last several years the rover has been slowly climbing “Mount Sharp” – the 5 km tall mound at the centre of the crater – and officially called Aeolis Mons – revealing how it is the result of the crater being the home of several lakes during Mars’ ancient history.

With lower slopes at the top and upper sloped at the bottom, this image of Aeolis Mons (from NASA’s Mars Reconnaissance Orbiter) charts Curiosity’s climb to the ridge which caused it so much trouble (white lines, the dots showing individual Sols), with the multiple attempts to drive over it (the collection of dots in the middle of the image) and the eventually diversion around it which allowed the rover to enter the “Jau” crater field. Credit: NASA/JPL

Most recently, the rover has faced its toughest challenge yet: attempting to ascend a ridgeline setting between it and an area of geological interest dubbed “Jau”. From orbit, the ridge appeared to be difficult, but not impossible for the rover. However, it combined three obstacles which proved troublesome: a steep slope averaging 23o and which comprises a mix of sand dunes and boulders large enough to pose a threat to the rover’s already battered wheels.

Initial attempts to get over this ridge in April and June resulted in the rover hitting “faults”:  stoppages triggered automatically as the wheels start slipping, either as a result of the ground beneath them being too soft to offer traction meeting a resistance such as a too-large boulder they could not overcome. These forced the mission team to take a chance on a 300 metre diversion to try a point on the ridge which appeared to be less challenging.

The diversion proved worthwhile; despite taking several weeks to plan and execute, Curiosity managed to reach “Jau” – an area of multiple impact craters in close proximity to one another – in early July, and has been studying it at length.

Overcoming the ridge is a significant achievement for the rover, and clearly it means Curiosity should have something of a smoother passage to its next destination.

Voyager 2 Loses and Regains Communications

NASA’s veritable Voyager 2 spacecraft, launched in 1977 19.9 billion kilometres from Earth as part of the twin Voyager mission, suffered a slight glitch on July 28th after an incorrect command sent from Earth swung its communications antenna 2o out of alignment, breaking contact with Earth.

The news caused some excitement on solar media, although calmer heads, such as Carolyn Porco, herself once a member of the Voyager mission team pointed out, Voyager 2 knows where it is relative to Earth and, failing the receipt of updates, would perform a routine “safing” manoeuvre the re-align its antenna with Earth on October 15th.

Even so, the mission team set about trying to contact the vehicle to re-establish contact sooner rather than later. On August 1st, they obtained Voyager 2’s “heartbeat” signal – a “pulse” intended to indicate all is well with the craft. As a result, a signal commanding Voyager 2 to re-orient itself was sent from the Deep Space Network facility in Canberra, Australia, although it took 37 hours for the command to be received, acted upon and a confirmation sent back to Earth, followed by a resumption of science and telemetry data.

A 2018 illustration showing the approximate positions of the Voyager craft as they mov through the interstellar medium beyond the Sun’s influence. Credit: NASA/JPL

Both Voyager 1 and Voyager 2 are moving through the interstellar medium beyond the direct influence of our Sun, but both are running out or power from their “nuclear batteries”. Over the last several years steps have been taken to try to preserve their power capabilities for science and communications, but it is currently anticipated Voyager 2’s power reserves are liable to be unable to power the remaining science instruments much beyond the end of 2026.

Chandrayaan-3 Achieves Initial Lunar Orbit

India’s latest lunar mission, Chandrayaan-3, entered its initial orbit around the Moon on August 5th. The mission, which I outlined on July 16th, following its successful launch, will now commence a series of orbital corrections through until August 17th, gradually settling its elliptical orbital into a circular one some 100 km above the lunar surface.

At this point, the lander will separate from the propulsion module and manoeuvre itself into a 35x100km orbit and undergo landing check-outs. The final descent and the soft landing attempt are set for August 23rd, with the primary landing site is in the vicinity of the lunar South Pole region, located at 69.37 degrees south latitude and 32.35 degrees east longitude. No previous Moon mission has landed at such a low latitude.

If successful, Chandrayaan-3 will make India only the fourth country in the world to achieve a lunar landing, joining the U.S., the former Soviet Union and China. The lander will then deploy a small rover for a 15-day surface mission independent of the lander.

Ingenuity Flies Again

NASA’s Mars helicopter drone Ingenuity has completed its 53rd flight, confirming all is well with the little vehicle after it losing contact with Earth for 63 days after its 52nd flight carried it out of line-of-sight communications with the Mars 2020 rover, Perseverance  – which acts as a relay between the drone and Earth.

A GIF released by NASA on August 3rd, 2023, showing Ingenuity landing within Jezero Crater at the end of its 53rd flight. Credit: NASA/JPL

The 53rd flight actually took place on July 22nd, around a month after Perseverance had trundled to a point where it could once again “see” Ingenuity and allow communication between the done and Earth to be re-established– but NASA opted not to release all of the data for the flight until August 4th. However, keen-eyed Ingenuity watchers speculated the flight had occurred prior to August 2nd, when it was noted images returned by the drone appeared to show a change in terrain.

Overall, the flight covered a distance of 142 metres at an altitude of 5 metres. The flight lasted a total of 75 seconds, including both horizontal flight and vertical transition / hovering while the craft imaged its surroundings prior to landing at the end of its flight.

Plans are now in progress for the 54th flight.