The Ouna spacecraft, also called VRAD (right), was released on Friday. This image was taken from a camera on the mothership (Image: JAXA) Part of South America is visible in this image of Earth taken by the Kaguya spacecraft from a distance of 110,000 kilometres (Image: JAXA/NHK)

Japan’s Kaguya spacecraft has released its second mini-probe into orbit around the Moon. The two ‘baby’ probes will work in concert with their mothership to reveal the Moon’s internal structure by making sensitive measurements of its gravity field.
Formerly known as SELENE, for SELenological and ENgineering Explorer, Kaguya is named after a character from a Japanese legend who travels to the Moon. It blasted into space on 14 September and entered lunar orbit on 4 October.
The two mini-spacecraft are each just 1 metre long with a mass of about 50 kilograms, while the main spacecraft, which weighs in at nearly 3 tonnes and measures about 5 metres long.
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They clung to the main spacecraft during launch, but detached on 9 and 12 October. They are called Okina and Ouna, after the foster parents of princess Kaguya in the legend.
Guardian angels
“[The two] satellites are flying in a higher orbit than the main satellite, Kaguya, as if they are watching over the Kaguya as its guardians,” a statement from the Japan Aerospace Exploration Agency (JAXA) says. “Therefore, we selected Okina and Ouna as their nicknames.”
Okina will travel in an elongated orbit that is 100 kilometres from the Moon at one end and 2400 kilometres at the other, while Ouna’s path will take it from 100 to 800 kilometres from the Moon.
Using just 70 watts of power each, about what is needed to power a light bulb, the two probes, together with the main spacecraft, will measure the Moon’s gravity field to probe the distribution of mass in its interior.
Far side
The motions of the three spacecraft, which are sensitive to variations in the gravity field, will be measured from Earth by tracking their radio signals. Okina and Ouna will beam radio signals directly to Earth, and Okina will also relay signals to Earth from Kaguya while the main spacecraft is out of contact on the far side of the Moon.
The Moon has a much “lumpier” gravity field than Earth because its mass is not as smoothly distributed inside. These variations cause spacecraft orbits to change over time, a problem better gravity maps may help solve, says Paul Spudis of Johns Hopkins University in Laurel, Maryland, US.
“If people go, or even [for] future unmanned spacecraft, the better you know the gravity field, the better you can find stable orbits,” he told New ¾«¶«´«Ã½ before the launch.
High-definition videos
It may also help scientists figure out the events that made the Moon’s crust uneven in thickness, with the thickest part on the far side, he says, something that would have been set early in the Moon’s early history.
The mission will start collecting science data in a couple of months, says Kaguya project manager Yoshisada Takizawa. “The checkout of the mission instruments will be finished in December,” he told New ¾«¶«´«Ã½. “After the mission instruments’ checkout, the planned observation of the Moon will be started.”
Between now and then, the main spacecraft also needs to finish adjusting its orbit from the current elliptical one into a circular orbit 100 kilometres above the lunar surface.
Since reaching space, Kaguya has recorded some high-definition videos of Earth. JAXA has released a still frame from the footage, showing Earth from 110,000 kilometres away (see image at right).
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


