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Emily LakdawallaJune 21, 2018

Hayabusa2 update: New views of Ryugu and corkscrew course adjustments

Ryugu has continued to grow in Hayabusa2's forward view, resolving into a diamond-shaped body with visible bumps and craters!

Ryugu approach images from 220 km to 100 km

JAXA, University of Tokyo, Koichi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, University of Aizu and AIST

Ryugu approach images from 220 km to 100 km
These 16 images of Ryugu were captured by Hayabusa2's ONC-T (Optical Navigation Camera - Telescopic) on June 18, 19 and 20. Image processing was used to interpolate between the pixels during enlargement and emphasize light and dark regions.

Optical navigation camera principal investigator Seiji Sugita described the images on the JAXA website:

"The varied geography of Ryugu"

As we approached Ryugu and were able to distinguish individual features in the asteroid's topology, it became clear that Ryugu has a land of rich terrain. Numerous clusters of rock roll on the surface. Among these, a large rocky mass (about 150m across) stands out on the upper part of Ryugu due to its brighter color (higher reflectivity). The belt-shaped ring of peaks that surround the equator are also slightly brighter than their surroundings. This color difference may reflect a difference in material composition and the size of the particles that form the rock. We can also see many sunken regions that look like craters. These depressions may have been made in collisions with other celestial bodies. A structure that looks like a grove is also visible.

The existence of such varied topographies is an indication that Ryugu has undergone a complex evolutionary history. It is generally believed that small asteroids that are less than 1km, such as Ryugu, were created fairly recently in the Solar System's history (within several hundred million years) during the fragmentation of a larger parent body. Ryugu's terrain will tell us about the division from the parent body and the asteroid's subsequent evolution.

The spacecraft is now experiencing Ryugu's gravitational tug, accelerating it toward its destination. Hayabusa2 has adjusted its course six times to brake its motion with respect to the asteroid and to do optical navigation. In the final stages of the approach, navigators weaved the spacecraft's path back and forth slightly, to create parallax between Ryugu in the foreground and the stars in the background. The optical navigation images they took has dramatically increased the accuracy of their estimation of the range to Ryugu, necessary for planning the final approach.

Optical navigation on Hayabusa2


Optical navigation on Hayabusa2
Taken from the 14 June 2018 press conference slides (PDF).

While at a distance of 2100 kilometers, they conducted a thorough search for satellites in the space around Ryugu, both for science and for spacecraft safety. Ryugu's gravity is small, so its gravitational influence (its Hill sphere) extends only out to 90 kilometers' altitude. No satellites were found, ruling out the existence of satellites larger than 50 centimeters in diameter. As they approach the asteroid, they'll continue doing hazard searches to make sure the space around the asteroid is safe for space flight; they'll have to perform another search before getting closer than 50 kilometers, where hazards could've been hiding in Ryugu's glare during the previous search.

On June 7, Hayabusa2 pointed its thermal infrared imager at Ryugu for 8 hours (from 08:30 to 16:30), taking 37 images. The double-humped light curve they measured matched Earth-based estimates of Ryugu's rotation rate of about 7.6 hours. As Hayabusa2 approaches, they'll refine the rotation rate.

The current plan for Hayabusa2 activities is as follows, with all future dates being subject to change:

EventDate (JST)Range to
Ryugu (km)
Ion engine operation ends 3 Jun 2018 3100 Complete
Asteroid approach begins, enter optical-radio combined navigation phase 3 Jun 2018 3100 Complete
Trajectory correction maneuver 1 (rel. speed now 2.35 m/s) 8 Jun 2018 1900 Complete
Trajectory correction maneuver 2 (rel. speed now 2.1 m/s) 11 Jun 2018 1320 Complete
Trajectory correction maneuver 3 (rel. speed now 1.7 m/s) 14 Jun 2018 750 Complete
Trajectory correction maneuver 4 (rel. speed now 1.3m/s) 15 Jun 2018 470 Complete
Trajectory correction maneuver 5 (rel. speed now 0.7 m/s) 18 Jun 2018 220 Complete
Trajectory correction maneuver 6 (rel. speed now 0.4 m/s) 20 Jun 2018 110 Complete
Trajectory correction maneuver 7 22 Jun 2018    
Trajectory correction maneuver 8 24 Jun 2018    
Trajectory correction maneuver 9 26 Jun 2018    
Ryugu arrival 27 Jun 2018 20  
Medium altitude observations #1 end July 2018 5  
Descent to measure gravity August 2018 1  
Touchdown operation & rover deployment #1 Sep-Oct 2018    
Solar conjunction Nov-Dec 2018    
Medium altitude observations #2 January 2019 5  
Touchdown operation #2 February 2019    
Impactor & crater generation Mar-Apr 2019    
Touchdown operation #3 Apr-May 2019    
Rover deployment #2 July 2019    
Remain near asteroid Aug-Nov 2019    
Depart asteroid Nov-Dec 2019    

JAXA also announced a schedule for future press briefings on July 19, August 2, and August 23.

Finally, here's a fun new way to keep on top of Hayabusa2: an aggregated browser feed of multiple information sources assembled by user mcmcmc.

Ryugu from 100 km

JAXA, University of Tokyo, Koichi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, University of Aizu and AIST.

Ryugu from 100 km
This image of Ryugu was as captured by Hayabusa2's ONC-T (Optical Navigation Camera - Telescopic) on June 20 from a distance of about 100 kilometers.

Read more: asteroid 162173 Ryugu, Hayabusa2, mission status, asteroids

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Emily Lakdawalla

Solar System Specialist for The Planetary Society
Read more articles by Emily Lakdawalla

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