We live inside the Milky Way galaxy which is joined as it drifts through space by two satellite galaxies, the Magellanic Clouds. A star cluster in the Large Magellanic Cloud known as R136 has been the subject of a fascinating discovery. A team of astronomers have discovered 55 high-speed stars that have been ejected from the cluster. The discovery was made using the Gaia satellite and it seems up to a third of stars from the cluster have been ejected in the last century.
R136 is a massive star cluster in the Tarantula Nebula inside the Large Magellanic Cloud (LMC.) The LMC is a satellite galaxy of ours at a distance of around 160,000 light years. The cluster is among the most massive known and it contains some of the most massive stars ever observed. The stars are young at just a few million years old having formed out of the gas in the nebula.
This is a Hubble Space Telescope image of a star-forming region containing massive, young, blue stars in 30 Doradus, the Tarantula Nebula. Located within the Large Magellanic Cloud, this is one of the regions observed by a newly-completed survey named ULLYSES. Image Credit: NASA, ESA, STScI, Francesco Paresce (INAF-IASF Bologna), Robert O’Connell (UVA), SOC-WFC3, ESOWhen clusters form, the random movement of gas is transferred to the forming stars. With the movement of stars, crisscrossing the cluster it is not uncommon for stars to be ejected out. This was exactly what the team of astronomers observed using Gaia. The Gaia space observatory was launched back in 2013 by the European Space Agency and has been precisely mapping stellar positions since.
Artist’s impression of the ESA’s Gaia Observatory. Credit: ESAThe team of astronomers led by University of Amsterdam PhD student Mitchel Stoop discovered the ejected stars travelling at speeds above 100,000 km/hr. You may have heard the saying ‘live fast, die young!’ Whether it’s true for humans is an interesting debate but it certainly seems true for stars. The most massive stars in the Universe fuse elements deep in their core at an alarming rate so will reach the end of their lives in just a few million years. Stars like those in R136 are a great example of this and, after being ejected to distances of around 1,000 light years, explode as supernova producing a neutron star or a black hole.
The measurements showed too that the stars have not been ejected over one particular period of the cluster’s history. The first event seems to have taken place 1.8 million years ago just when the cluster formed. Another event seems to have occurred around 200,000 years ago. Comparing the two events revealed an interesting difference. In the first event during the formation of the cluster, the stars shot off in almost random directions but in the second event, the stars moved in one general direction.
The co-author of the paper which was published in Nature, Alex de Koter said “We think that the second episode of shooting away stars was due to the interaction of R136 with another nearby cluster (that was only discovered in 2012). The second episode may foretell that the two clusters will mix and merge in the near future.”
The discovery that a third of the stars have been ejected from their point of origin shows that, through the ejection, they can influence other regions of the galaxy. It is even possible that ejected stars through the history of the evolution of the Universe could have contributed to the reionization of the universe by ultraviolet light. In this era, the universe transitioned from being filled with ionised gas to a more neutral era with electrons and protons combining to form neutral hydrogen atoms.
Source : Dozens of massive stars launched from young star cluster R136
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Jupiter is well known for its Great Red Spot, a feature that was discovered by Galileo over 400 years ago! Astronomers have been tracking the size and shape of it for over a century but the most accurate measurements have come from the Hubble Space Telescope. Every time Earth and Jupiter are at their closest, Hubble takes a series of images and it’s these images that have detected that the spot jiggles from day to day. Not only does it change size but length and width too leaving astronomers baffled.
Jupiter is the largest planet in the Solar System and, like the other outer planets is a giant ball of gas. It’s so large all the other planets in the Solar System can be fitted inside with plenty of room to spare. Composed mostly of hydrogen and helium it can be seen as a colourful disk through amateur telescopes with belts, storms and of course the Great Red Spot. The spot was first discovered by Galileo in around 1610 when he became the first person to turn a telescope on the distant planet.
Side-by-side images show the opposite faces of Jupiter. The largest storm, the Great Red Spot, is the most prominent feature in the left bottom third of this view. Credit: NASA, ESA, Amy Simon (NASA-GSFC).The Great Red Spot is a storm which has been raging for over 400 years. It’s large enough that Earth could easily fit inside more than once and is an anticyclone system similar to those seen here on Earth. It rotates in a counterclockwise direction with speeds reaching in excess of 640 km per hour. Over the years, it seems to have been generally decreasing in size albeit not as quickly as expected.
“Great Red Spot from P7 Flyover”. Credit: NASA / SwRI / MSSS / Jason Major © public domainImages taken by Hubble of the storm were collected over a 90 day period between December 2023 and March 2024 when the Jupiter was at its closest to Earth. Its high resolution cameras showed that it is jiggling like a bowl of jelly and certainly not as stable as we once thought. Previous studies showed that there is an amount of movement along the longitudinal axis but no suggestion it’s changing in size.
The team of astronomers led by Amy Simon of NASA’s Goddard Space Flight Centre in Maryland published their findings in the Planetary Science Journal. Simon’s said “This is really the first time we’ve had the proper imaging cadence of the GRS. With Hubble’s high resolution we can say that the GRS is definitively squeezing in an out at the same time as it moves faster and slower. That was very unexpected, and at present there are no hydrodynamic explanations.”
The study was a part of NASA’s Outer Planet Atmospheres Legacy program (OPAL) whose aim is to obtain a long time series of observations of the outer planets to understand their evolution and atmosphere. These recent observations though were purely to explore and analyse the GRS. Extrapolating forward in time the team think that the GRS will keep shrinking before it stabilises in a less elongated shape than we see today. Currently it’s particularly ‘wide’ in latitude but once it shrinks it will likely stabilise with the winds holding it in place.
The team hope that to understand the GRS was to understand the mechanisms of the largest storms in the Solar System which would ultimately help us to learn more about hurricane systems on Earth.
Source : NASA’s Hubble Watches Jupiter’s Great Red Spot Behave Like a Stress Ball
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China’s space program has advanced considerably since the turn of the century. In addition to developing heavy-launch vehicles like the Long March 5 and building a modular space station in orbit, China has also embarked on an ambitious program of lunar exploration (Chang’e) – which has launched six robotic missions to explore the Moon’s surface since 2007. These missions are paving the way for crewed missions to the Moon by 2030 and creating a permanent habitat around the Moon’s southern polar region – the International Lunar Research Station (ILRS).
They also plan to send crewed missions to Mars by 2033, which will culminate in the creation of a permanent base there too. Earlier today, the Chinese Academy of Sciences (CAS), the China National Space Administration (CNSA), and the China Manned Space Agency (CMSE) jointly released the country’s first long-term scheme for space science and exploration. Titled “National Medium—and Long-Term Development Plan for Space Science (2024-2050),” this plan elaborated on the basic principles, development goals, and roadmap for the country’s space science and exploration through 2050.
Tiangong Chinese space station. Credit: China Manned Space Agency.The plan revealed five major scientific themes it hopes to accomplish in three developmental stages between now and mid-century. These five themes contain 17 priority areas for future breakthroughs, outlined by CAS Vice President Ding Chibiao at a press conference earlier today. According to statements released by The State Council of the People’s Republic of China and shared via the China Global Television Network (CGTN), they include:
The plan also outlined a three-stage development roadmap between 2024 and 2050. For the first stage (2024-2027), China will focus on maintaining the operation of the Tiangong space station, carrying out crewed missions to the Moon, and commencing the fourth phase of its Chang’e program – which includes the launch of the Chang’e-7 and -8 missions in 2026 and 2028, respectively – as well as its planned missions to Mars. According to the program, five to eight space science satellite missions will also be approved during the period.
Visualization of the ILRS from the CNSA Guide to Partnership (June 2021). Credit: CNSAThe second stage (2028 to 2035) will consist of the continued operation of the Tiangong space station (and expanding it to twice its current size), crewed missions to the Moon, and the construction of the ILRS. China is also expected to deploy about 15 space satellite missions during this phase. The third and final stage (2036 to 2050) calls for more than 30 space science missions to be implemented, with the intention of achieving “significant advancements in key areas reaching a world-leading level.”
Through this program, China hopes to address some of the most challenging fundamental questions and scientific issues of our time. This includes the nature of Dark Matter and Dark Energy, the origins of the Universe, extraterrestrial life (aka astrobiology), the evolution of the Solar System and its Planets, and the connections of the Sun-Earth system. Given the ambitious nature of the program and some of the wording used (“reaching a world-leading level”), it could also be seen as a declaration of intent.
For years, China has indicated its intentions to rival NASA as a major power in space. With this first-ever roadmap, it is clear that China’s long-term intentions are to replace NASA as a leader in space exploration and science.
Further Reading: CGTN, The State Council of the People’s Republic of China
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The X-37B Orbital Test Vehicle (OTV) has been shrouded in mystery since its maiden flight in 2011. Designed by Boeing and operated by the U.S. Space Force (USSF), this remotely operated, reusable space plane is designed to operate in Low-Earth Orbit (LEO), 240 to 800 km (150 to 500 mi) above the Earth, and test reusable vehicle technologies that support long-term space objectives. On December 29th, 2023, the X-37B began its seventh mission (OTV-7) and has reportedly been conducting experiments on the effects of space radiation and testing Space Domain Awareness (SDA) technologies.
As part of this mission, the X-37B will soon begin executing a series of novel maneuvers to change its orbit around Earth. These maneuvers will consist of the spacecraft brushing against Earth’s upper atmosphere to shed speed and lower its orbit without expending much fuel—a technique known as “aerobraking.” This is the first time the X-37B has performed such a maneuver, which will help it evade detection by potentially hostile nations and perform undetected low passes over Earth during future missions.
According to a statement by the USSF, this latest maneuver leverages six successful missions in LEO and decades of lessons learned from missions to the Moon and Mars. In 1997, the Mars Global Surveyor (MGS) orbiter used its solar panels as “wings” to control its passage through Mars’ tenuous upper atmosphere and lower its orbit over several months. More recently, aerobraking has been used by the Mars Odyssey in 2001, the Mars Reconnaissance Orbiter in 2006, and the ESA’s ExoMars Trace Gas Orbiter in 2017-2018.
The X-37B Orbital Test Vehicle taxiing on the flightline on March 30th, 2010, at the Astrotech facility in Titusville, Florida. Credit: USAF“This novel and efficient series of maneuvers demonstrates the Space Force’s commitment to achieving groundbreaking innovation as it conducts national security missions in space,” said Secretary of the Air Force Frank Kendall. “This first-of-a-kind maneuver from the X-37B is an incredibly important milestone for the United States Space Force as we seek to expand our aptitude and ability to perform in this challenging domain,” added Chief of Space Operations Gen. Chance Saltzman. “The success is a testament to the dedication and perseverance of the team.”
Beyond these experiments, very little is known about the X-37B’s capabilities and purpose. However, during the Aspen Security Forum in 2019, former U.S. Air Force (USAF) Secretary Heather Wilson explained how the X-37B capabilities allow it to avoid detection, saying:
“[The X-37B is] fascinating [because it] can do an orbit that looks like an egg and, when it’s close to the Earth, it’s close enough to the atmosphere to turn where it is. Which means our adversaries don’t know – and that happens on the far side of the Earth from our adversaries – where it’s going to come up next. And we know that that drives them nuts. And I’m really glad about that.”
As Jonathan McDowell – an astronomer and astrophysicist at the Harvard-Smithsonian Center for Astrophysics – told Military.com in an interview at the time:
“[Wilson’s comments may shed light on] a previously secret orbit-related capability. The dip into the atmosphere causes a change in the timing of when it next comes overhead. So [trackers’] predictions are off, and [they] have to search for it all over again. Even a timing change makes more work for [adversaries] than just being able to use the existing orbital prediction.”
Once the aerobrake maneuver is complete, the X-37B will resume its tests and experiments until they are fulfilled. As the USSF indicated before the launch of the OTV-7 mission, these tests include operating in new orbital regimes, experimenting with future SDA technologies, and investigating the radiation effects on plant seeds provided by NASA – the “Seeds-2” experiment. The spacecraft will also eject some of its service module components in accordance with recognized standards for space debris mitigation. At this point, the vehicle will de-orbit and return to Earth as it has during its six previous missions.
Further Reading: Live Science, USSF
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