China launches another set of satellites for one of its giant internet constellations

China earlier today successfully launched the sixth set of satellites for the Thousand Sails internet constellation, its Long March 6A rocket lifting off from its Taiyuan spaceport in northern China.

Very little information appears available about this specific payload. No word also was released about where the rocket’s lower stages and four strap-on boosters crashed inside China.

The leaders in the 2025 launch race:

69 SpaceX
33 China
7 Rocket Lab
6 Russia

SpaceX still leads the rest of the world in successful launches, 69 to 53.

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June 5, 2025 Quick space links

Courtesy of BtB’s stringer Jay. This post is also an open thread. I welcome my readers to post any comments or additional links relating to any space issues, even if unrelated to the links below.

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Landing of Ispace’s Resilience lander uncertain

Resilence landing

The landing of Ispace’s Resilience lander on the Moon at present appears uncertain, and could be a failure. Though the announcers of the live stream had warned beforehand that it might take awhile after the planned touchdown time to confirm a successful landing, the circumstances just before landing did not appear to go as expected.

At T-1:45 minutes, with the spacecraft at an altitude of 32 feet and still moving at a speed of 116 miles per minute, all telemetry disappeared from the broadcast. Mission controllers did then indicate the spacecraft was “pitching up”, which means it was re-orienting itself for landing. At that point however no further updates were provided. Moments later we could see the engineer in mission control in the lower left of the screen capture to the right, obviously disturbed by something.

In ending the live stream a few minutes later, with no further information, the announcers added that a full report will be made during a press conference later today.

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Scientists discover another exoplanet that theories say should not exist

The uncertainty of science: Scientists using telescopes both in orbit and on the ground have discovered a small red dwarf star with only 20% the mass of our Sun with a gas giant exoplanet with about half the mass of Saturn but a bit larger in size.

The problem is that the theory for the formation of such gas giants predicts that they should not form around small red dwarfs such as this star.

The most widely held theory of planet formation is called the core accretion theory. A planetary core forms first through accretion (gradual accumulation of material) and as the core becomes more massive, it eventually attracts gases that form an atmosphere. It then gets massive enough to enter a runaway gas accretion process to become a gas giant.

In this theory, the formation of gas giants is harder around low-mass stars because the amount of gas and dust in a protoplanetary disc around the star (the raw material of planet formation) is too limited to allow a massive enough core to form, and the runaway process to occur.

Yet the existence of TOI-6894b (a giant planet orbiting an extremely low-mass star) suggests this model cannot be completely accurate and alternative theories are needed.

You can read the paper here. The exoplanet orbits the star every 3.37 days, and each transit across the face of the star has been easily detected by numerous telescopes. Further spectroscopic observations using the Webb Space Telescope will be able to characterize the exoplanet’s atmosphere more fully.

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Scientists release the first year’s data from the Pace orbiter

Pace global data, August 2024
Click for original movie.

Launched in early 2024, the Pace orbiter was designed to track the evolution of the leaves of trees globally throughout the entire year. NASA has now released the data from the first twelve months, showing the seasonal changes of trees as the Earth rotates the Sun and the seasons change globally.

The map to the right is a screen capture from one of many videos showing these changes. The green indicates the global spread of tree cover in the middle of August in the northern hemisphere as well as in the equatorial regions of South America and Africa. Other movies focusing on North America, South America, Europe, India, etc, can be viewed here.

PACE measurements have allowed NASA scientists and visualizers to show a complete year of global vegetation data using three pigments: chlorophyll, anthocyanins, and carotenoids. That multicolor imagery tells a clearer story about the health of land vegetation by detecting the smallest of variations in leaf colors.

…Anthocyanins are the red pigments in leaves, while carotenoids are the yellow pigments โ€“ both of which we see when autumn changes the colors of trees. Plants use these pigments to protect themselves from fluctuations in the weather, adapting to the environment through chemical changes in their leaves. For example, leaves can turn more yellow when they have too much sunlight but not enough of the other necessities, like water and nutrients. If they didnโ€™t adjust their color, it would damage the mechanisms they have to perform photosynthesis.

In the visualization, the data is highlighted in bright colors: magenta represents anthocyanins, green represents chlorophyll, and cyan represents carotenoids. The brighter the colors are, the more leaves there are in that area. The movement of these colors across the land areas show the seasonal changes over time.

You can read the full paper describing the first year’s data here.

The Trump budget presently funds Pace for two more years of observations, at about $26 million per year. This is an obvious example of a satellite whose life should be extended for as long as possible. This long term data would likely confirm other data that indicates the increase in CO2 in the atmosphere is greening the Earth, helping plant life that provides us oxygen to breath and food to eat.

To do so, however, other cuts in NASA will have to be found to pay for that extension. I once again wonder about the half a billion NASA spends for its “Mission Enabling Services”, which covers NASA’s human resources division, public relations department, and its equal opportunity division, as well as other more useful departments. Surely some money from these bureaucratic divisions could be found to finance this actual useful research.

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Watch the landing attempt of Ispace’s Resilience lunar lander

Map of lunar landing sites
Landing sites for both Firefly’s Blue Ghost and
Ispace’s Resilience

I have embedded the live stream below of the landing of the Japanese startup Ispace’s Resilience lunar lander, presently scheduled to occur at 3:17 pm (Eastern) today (June 6, 2025 in Japan).

The live stream goes live at about 2:00 pm (Eastern).

Resilience will attempt to land on the near side of the Moon at 60.5 degrees north latitude and 4.6 degrees west longitude, in the region dubbed Mare Frigoris (Latin for “the Sea of Cold”), as shown on the map to the right. That map also shows a number of other landings on this quadrant of the Moon, including Ispace’s previous failed attempt with its first lander, Hakuto-R1, in Atlas Crater in 2023.

For Ispace, today’s landing is critical for its future. It has contracts for future three landers with NASA, with Japan’s space agency JAXA, and with the European Space Agency, but a failure today could impact whether those contracts proceed to completion.
» Read more

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SpaceX launches more Starlink satellites

SpaceX this afternoon successfully launched another 27 Starlink satellites, its Falcon 9 lifting off from Vandenberg Space Force Base in California.

The first stage completed its 26th flight, landing on a drone ship in the Pacific. Also, as noted by regular reader Richard M, this was also the 500th orbital launch of a Falcon rocket, including the Falcon 1, the Falcon 9, and the Falcon Heavy. And the company has done this in only a bit over fifteen years. Quite amazing.

The leaders in the 2025 launch race:

69 SpaceX
32 China
7 Rocket Lab
6 Russia

SpaceX now leads the rest of the world in successful launches, 69 to 52.

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June 4, 2025 Quick space links

Courtesy of BtB’s stringer Jay. This post is also an open thread. I welcome my readers to post any comments or additional links relating to any space issues, even if unrelated to the links below.

  • New paper speculates alternative to the Big Bang
    Fun stuff only a tiny bit different than fantasy. The author does however provide a nice summary of some of the basic problems with the Big Bang theory itself, problems that until recently it was generally considered inappropriate for any cosmologist to mention.
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Two giant clusters of galaxies on target for second collision

Colliding galaxy clusters
Click for full image.

Using telescopes both on Earth and in space, astronomers now think two giant clusters of galaxies that had collided previously have now stopping flying from each other and are on target for second collision.

The annotated image to the right shows what we can see today. The two blue blobs near the center are the two galaxy clusters.

The galaxy cluster PSZ2 G181.06+48.47 (PSZ2 G181 for short) is about 2.8 billion light-years from Earth. Previously, radio observations from the LOw Frequency ARray (LOFAR), an antenna network in the Netherlands, spotted parentheses-shaped structures on the outside of the system. In this new composite image, X-rays from Chandra (represented in purple) and ESAโ€™s XMM-Newton (blue) have been combined with LOFAR data (red) and an optical image from the Pan-STARRS telescope of the stars in the field of view.

These structures are probably shock fronts โ€” similar to those created by jets that have broken the sound barrier โ€” likely caused by disruption of gas from the initial collision about a billion years ago. Since the collision they have continued traveling outwards and are currently separated by about 11 million light-years, the largest separation of these kinds of structures that astronomers have ever seen.

Now, data from NASAโ€™s Chandra and ESAโ€™s XMM-Newton, a mission with NASA contributions, is providing evidence that PSZ2 G181 is poised for another collision. Having a first pass at ramming each other, the two clusters have slowed down and begun heading back toward a second crash.

When such giant object collide what really interacts the most is the gas and dust between the stars. The motions of the stars and galaxies of course get distorted by the pull of gravity, but there are almost never any crashes.

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