SciNews - H3-30 First launch:

View: https://youtu.be/EFElTQhFrdw


https://global.jaxa.jp/press/2026/06/20260612-1_e.html

Launch Result of H3 Launch Vehicle flight No.6, 30 configuration Test Vehicle

June 12, 2026 (JST)

Japan Aerospace Exploration Agency (JAXA) launched H3 Launch Vehicle flight No.6, 30 configuration Test Vehicle at 09:53:59(JST) on June 12, 2026 from the Tanegashima Space Center. The Launch Vehicle flew as planned, and the second stage of the H3 Launch Vehicle was injected into the predetermined orbit. Approximately 16 minutes and 4 seconds after the liftoff, the separation of the PETREL and STARS-X were confirmed.

Additionally, based on the post-Earth orbit data from the second-stage vehicle, JAXA confirmed that the separation signals were sent to BRO-22, VERTECS, HORN-L and HORN-R.

JAXA appreciates all for the support shown in behalf of the launch.
 
View: https://twitter.com/haya2e_jaxa/status/2053700075315175642?s=20
[May 11]

As Hayabusa2# prepares for the approach to asteroid Torifune, we've launched the second round of "Let's Meet the Petit Prince! Million Campaign 2♯"! Please send us your messages for the team, and a message to deliver to the Hayabusa2# spacecraft ️✒️

https://www.hayabusa2.jaxa.jp/en/topics/2026_TorifuneCamp2s_e/

A complete set of canonical nucleobases in the carbonaceous asteroid (162173) Ryugu [Mar. 16]

Organic molecules delivered from extraterrestrial materials may have played a key role in supplying building blocks for life on Earth. Here we report all five canonical nucleobases—purines (adenine and guanine) and pyrimidines (cytosine, thymine and uracil)—in samples returned from the C-type asteroid (162173) Ryugu by JAXA’s Hayabusa2 mission and compare the results with data from similar extraterrestrial material. Ryugu samples contain nearly equal amounts of purines and pyrimidines, whereas Murchison is enriched in purines and Bennu and Orgueil in pyrimidines. Samples from Ryugu, Bennu and Orgueil, which have a similar mineralogy and elemental composition, show purine-to-pyrimidine ratios negatively correlating with ammonia. These observations indicate that the nucleobases in these samples may have formed via a shared pathway depending on the physicochemical environment of the respective parent bodies. The detection of diverse nucleobases in asteroid and meteorite materials demonstrates their widespread presence throughout the Solar System and reinforces the hypothesis that carbonaceous asteroids contributed to the prebiotic chemical inventory of early Earth.
 
Japan unveils Mars moon sample-return spacecraft ahead of Oct. 19 launch (photos)

Last Thursday (Aug. 13), Japan unveiled the spacecraft that make up its Martian Moons eXploration (MMX) mission, which aims to snag samples of the Mars moon Phobos and haul them to Earth — something that has never been done.

The big reveal came at Tanegashima Space Center, the site from which MMX will launch toward the Red Planet atop an H3 rocket. And we just got some clarity about when that liftoff will take place.

If all goes according to plan, MMX will launch on Oct. 19 at 3:41 p.m. EDT (1941 GMT; 4:41 a.m. on Oct. 20 Japan time), the Japan Aerospace Exploration Agency (JAXA) announced on Thursday (Aug. 20). That's the first day of the mission's launch window, which extends through Nov. 7.
 
DESTINY+ Dust Analyzer Successfully Delivered to JAXA [May 28]

The flight model of the DESTINY+ Dust Analyzer (DDA) arrived in Japan after a journey of just under a week and was handed over to the Japanese space agency JAXA on May 28, 2026. This marks an important milestone for the international instrument project under the supervision of Ralf Srama and led by Heiko Strack of the Institute of Space Systems (IRS) at the University of Stuttgart on the path to the DESTINY+ mission.

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The DDA is a state-of-the-art dust telescope designed for the direct analysis of cosmic dust particles in space. It determines the velocity, mass, direction of travel, electric charge, and chemical composition of individual particles. With nine measurement channels and a newly developed two-axis alignment system, the DDA is among the most complex dust instruments ever developed for space use.

Much More Than Just Dust
Cosmic dust consists of microscopic particles made of silicates, carbon compounds, and metals. “These particles are much more than just dust in space,” explains Ralf Srama, head of dust research at the IRS. “They are fundamental building blocks of the universe and play a central role in the formation of organic molecules, stars, and planets—and thus also in the conditions necessary for life.”

A key scientific goal of the DESTINY+ mission is the flyby of the active asteroid (3200) Phaethon in 2030. During this flyby, the DDA will analyze microparticles from the asteroid’s tail that are released by meteoroid impacts on the asteroid’s surface. Phaethon is also the parent body of the Geminids, a meteor stream that is regularly visible in the night sky in December as a shooting star shower.

However, the DDA will be activated shortly after the spacecraft’s launch, allowing continuous data collection on interplanetary and interstellar dust even while en route to Phaethon. The first scientific milestone for DESTINY+ is the flyby of the asteroid Apophis, which is only 350 meters in size. This near-Earth object will fly past Earth on April 13, 2029, at a distance of just 32,000 km. DESTINY+ will thus have the opportunity to study this small object even before the RAMSES spacecraft.

Seven Years of Development
In 2019, the German Aerospace Center (DLR) commissioned the University of Stuttgart to develop the dust instrument for the bilateral DESTINY+ mission of JAXA and DLR. Over seven years of development, manufacturing, qualification, and validation, the IRS team successfully overcame challenges related to mass requirements for the mechanical structure and the electrical and mechanical interfaces with the spacecraft.

A final functional test in the University of Stuttgart’s globally unique 2-MV dust accelerator in the spring of 2026 confirmed the instrument’s full operational capability under space conditions.

The Stuttgart Dust Group has decades of experience in the development and operation of scientific dust instruments. Among other things, it was responsible for the Cosmic Dust Analyzer on the Cassini–Huygens mission and contributed to LADEE, Europa Clipper, and BepiColombo.

International Collaboration
The DDA was developed in close collaboration with international partners from the scientific and industrial sectors. The electronics were developed by von Hoerner & Sulger GmbH, and quality assurance was handled by Space Works Innovations GmbH. Qualification tests on the flight model—including thermal-vacuum, vibration, and shock tests—were conducted at the DLR in Bremen. An international scientific team led by Harald Krüger from the MPS in Göttingen provided scientific guidance throughout the development process. Regular communication also takes place with Hiroshi Imamura (JAXA Mission Management) and Tomoko Arai from the Planetary Exploration Research Center (PERC) in Tokyo.

Next Steps Leading Up to the 2028 Launch
Following its arrival at JAXA, the ATLO phase (Assembly, Test, and Launch Operations) is now beginning. In the coming months, the instrument’s electronics will first be integrated into the spacecraft and extensively tested with its onboard electronics. This includes, among other things, command and control, telemetry, thermal testing, and the verification of all mechanical and electrical interfaces.

In parallel, flight software, operational concepts, and data processing and archiving are being prepared. The launch of the DESTINY+ mission is scheduled for spring 2028 using a JAXA H3 rocket.
 

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