From Seeker: “Quest to Reveal Asteroid’s Mysteries Before Japanese Spacecraft’s Visit”

Seeker bloc


Dec 5, 2016

Artist’s concept of Hayabusa-2 approaching asteroid 162173 Ryugu (1999 JU3). Image Credit: JAXA

A Japanese spacecraft is on its way to some daring work at an asteroid. Hayabusa 2 is expected to reach Asteroid Ryugu in June or July 2018 and will drop several tiny landers on to its surface. The spacecraft itself will scoop up a sample of asteroid material for return back to Earth, just as its predecessor Hayabusa did at asteroid Itokawa a decade ago.

It’s clear that a lot of engineering and precision is needed to achieve these maneuvers, far from home and in a zone that doesn’t easily give second chances. So as Hayabusa 2 moves towards its target, astronomers on Earth are looking at Ryugu as much as they can to learn about its properties.

“Before you can send an interplanetary mission to a small body, it is important to know its orbit with the best possible accuracy, but you also have to know the object’s properties,” said Thomas Mueller, co-investigator for Hayabusa’s thermal infrared imager instrument, in an email to Seeker. He is also leading the efforts to do a characterization of Ryugu before Hayabusa 2’s arrival.

The latest research is based on analyzing results from the European Herschel Space Observatory (in April 2012) and the NASA Spitzer Space Telescope (between January and May 2013). The astronomers attempted to map the rotation of the object using its light curve (the change in light as seen from Earth), which in turn led to estimating its spin and surface composition. A paper based on the research was recently published on the prepublishing site arXiv, and has been accepted in the journal Astronomy & Astrophysics.

ESA/Herschel spacecraft

NASA/Spitzer Telescope
NASA/Spitzer Telescope

The shadow of Hayabusa, along with a target marker (circled, at left), is shown on asteroid Itokawa in November 2005. Credit: JAXA

Mueller, who works with the Max Planck Institute for Extraterrestrial Physics in Garching, Germany, has been interested in learning about small bodies in the solar system since his Ph.D. thesis, which he completed in 1997 — where he tried to apply infrared measurements of well-known targets to objects that were less well known, but still scientifically interesting. He’s been working to characterize Ryugu (in collaboration with the Japan Aerospace and Exploration Agency, or JAXA) since 2008.

“Mission targets like Itokawa (Hayabusa mission in 2005) or Ryugu (Hayabusa-2 mission) always attracted my attention for many reasons,” Mueller added, providing a list: “(1) The possibility to compare my model predictions with ‘ground-truth’ at some point; (2) the relation to space projects (I worked in the European Space Agency for several years); (3) the connection between near-Earth objects and Earth (NEAs as a risk for Earth, but also as the origin of life, water and heavy element supply); (4) to find out more about the building blocks of the planets.”

Specifically for Ryugu, Mueller says the latest research will help engineers adjust their instrument settings, do risk assessments and develop plans for what the spacecraft will do when it gets there. Some of the things they have covered include Ryugu’s estimated size, brightness (known as albedo), rotation period and spin axis, thermal properties and where grains of different sizes are distributed.

But there are challenges with observing a small object from so far away. The new paper notes that because Ryugu is nearly spherical, it made it hard to get a light curve. So the astronomers combined radiometric and lightcurve inversion techniques to come up with an estimation of Ryugu’s physical and thermal properties.

A view of asteroid Itokawa based on data from the Hayabusa spacecraft. Credit: JAXA

“In all our observations, we see Ryugu as a perfect point source (we cannot resolve the target from Earth distance),” Mueller added. “However, we are able to derive not only the size, shape, spin properties, but also things like the (most-likely) surface material (carbonaceous, complex organics?) or predominant grain sizes on the surface (1-10 mm).”

He added that both Itokawa and Ryugu are “fantastic opportunities” to see how well models hold up against ground truth. The astronomers are lucky to have this opportunity, as only a fraction of small bodies are visited by spacecraft, he said.

“Other experts in the field of small-body characterization/modelling will very likely pick up our published observations to make their own predictions,” he added. “It is very exciting for us to see who gets closest to the truth.”

See the full article here .

Please help promote STEM in your local schools.


Stem Education Coalition