Planetary Radio: Space Exploration, Astronomy and Science
Planetary Radio: Space Exploration, Astronomy and Science

Hayabusa2 Reaches a Dark Diamond in Space

Japan’s Hayabusa2 is just 6 kilometers from asteroid Ryugu as it prepares to snatch samples of the space rock for return to Earth. ISAS/JAXA Director General and former Hayabusa Mission Project Manager Hitoshi Kuninaka joins us for a conversation about the spacecraft and what’s ahead. Then we hear f

Featured Speakers

The Planetary Society HostHitoshi Kunanaka GuestHans-Jorg Didas Guest

Topics Discussed

Episode Summary

Executive Summary: This episode of Planetary Radio centers on Hayabusa2’s imminent asteroid Ryugu operations, featuring mission leader Hitoshi Kunanaka and DLR’s Hans-Jorg Didas on the science and engineering of sample return and the Mascot lander. It also highlights Emily Lochtawala’s new role leading The Planetary Report and closes with Mars opposition, eclipse notes, and space trivia with Bruce Betts.

Main Topics: Emily Lochtawala and The Planetary Report: Emily discusses becoming editor of the Planetary Society’s 40-year-old member magazine, its legacy, and plans to keep it focused on mission voices, imagery, and undercovered worlds while better aligning it with the website. Hayabusa2 mission status and mission design: Hitoshi Kunanaka describes Hayabusa2’s approach to Ryugu, the transition into proximity operations, and the careful autonomous procedures required for landing, sampling, and return. Ion propulsion and lessons from Hayabusa1: Kunanaka explains how the mission’s ion engines, improved after Hayabusa1’s technical issues, made deep-space travel possible for Japan’s limited launch capability and enabled a highly reliable cruise phase. Sampling Ryugu with impactor and return capsule: The transcript details the plan to create a crater using a copper impactor, collect subsurface material, and later return the sample capsule to Australia and then Japan for curation and analysis. Mascot and international collaboration: Hans-Jorg Didas explains the DLR-CNES Mascot lander, its passive hopping design, short battery-limited life, scientific instruments, and the importance of Japanese-European cooperation. Mars opposition and skywatching with Bruce Betts: Bruce Betts previews the 2018 Mars opposition, notes the total lunar eclipse in some regions, debunks the 'Mars as big as the Moon' myth, and answers listener trivia about Mars’ orbital eccentricity.

Key Arguments: Hayabusa2’s success depends on highly cautious autonomous operations because Earth-based control is impossible at the asteroid’s distance and light-time delay. Ion propulsion was essential for Japan’s deep-space missions because its rockets cannot loft enough mass for large chemical-propulsion spacecraft. Lessons from Hayabusa1 directly improved Hayabusa2, especially through extensive simulation, better engineering margins, and more reliable engine operation. Sampling below Ryugu’s weathered surface should produce fresher material, improving the chance of finding organic compounds and clues to early solar system history. Mascot was intentionally built as a tiny passive lander with a very limited lifespan to fit within strict mass constraints and to operate in Ryugu’s low gravity. International partnerships are treated as mutually beneficial, allowing agencies to share hardware, expertise, and mission roles across exploration programs. Mars appears dramatically different from the Moon because its orbit is more eccentric, which leads to stronger variations in distance and brightness across oppositions.

Data Points: Planetary Report circulation: about 50,000 people - Emily Lochtawala describes the member magazine’s readership Age of The Planetary Report: 40 years old - Magazine founded in 1980 by Carl Sagan Hayabusa2 distance from Ryugu: 20 kilometers (12.5 miles) - Kunanaka describes the spacecraft’s proximity during the interview Communication delay to Ryugu: about 40 minutes one way - Explains why spacecraft autonomy is necessary Ion engine thrust (Hayabusa1): 8 milliNewtons - Baseline engine performance referenced by Kunanaka Ion engine thrust (Hayabusa2 improved): 10 milliNewtons - Improved propulsion system used on Hayabusa2 Thrust increase: 25% - Improvement over the Hayabusa1 engine Hayabusa2 cruise reliability: 3.5 years with no interruption - Kunanaka says the improved ion engine operated continuously during cruise Mascot lander mass limit: 10 kilograms maximum - Didas describes the extreme mass constraint for the lander Ryugu surface albedo: 1.5% - Didas notes the asteroid is exceptionally dark Expected surface temperature: about 90°C - Predicted by first images and used to inform landing-site selection Mars closest approach in 2018: July 31, 2018 - Bruce Betts discusses the Mars opposition/close approach Mars opposition date: July 27, 2018 - Mars is opposite the Sun in the sky Mars apparent diameter at closest approach: 24.31 arcseconds - Bruce’s random space fact Full Moon apparent diameter: about 1800 arcseconds - Used to debunk the Mars-hoax comparison Ratio of Moon to Mars apparent size: about 74 times larger - Calculated from the angular diameters Contest deadline extension: Wednesday, August 8, at 8 a.m. Pacific Time - Bruce extends the trivia entry deadline

Pivotal Quotes: "Asteroid is the fossil of the solar system." — Hitoshi Kunanaka: Used to explain why samples from Ryugu matter scientifically "We have to be lucky." — Hans-Jorg Didas: Describing the passive landing challenge for Mascot on Ryugu "Space exploration will stimulate human beings, I believe." — Hitoshi Kunanaka: On the motivational and inspirational value of exploration

Implications: The episode shows how asteroid sample-return science depends on precision engineering, international partnership, and public engagement. Hayabusa2 and Mascot may reveal pristine solar-system material, while the magazine and skywatching segments broaden participation in exploration.

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