Astronomers were first alerted<\/a> to the mysterious cloud’s presence in September 2024, when they detected a surprise dimming event surrounding the star J0705+0612 (sometimes referred to as ASASSN-24fw) \u2014 a sun-like, main sequence star around 3,000 light years from Earth. The star’s brightness suddenly fell 40-fold, to around 3% of its original luminosity, and remained that way for just over eight and a half months before returning to full brightness in May 2025.<\/p>\n You may like<\/p>\n “Stars like the sun don’t just stop shining for no reason,” study lead author Nadia Zakamska<\/a>, an astrophysicist at Johns Hopkins University, said in a statement<\/a>. “So dramatic dimming events like this are very rare.”<\/p>\n In the study, published Jan. 21 in The Astronomical Journal<\/a>, Zakamska and her team analyzed this strange event using data captured by the Gemini South telescope and the Magellan Telescopes in Chile, and found that a massive object had passed in front of, or occulted, J0705+0612. After ruling out things like giant planets and asteroid belts, which were either too small or too diffuse to block out so much light for so long, the researchers concluded that the occulting object was a thick cloud of molecular gas.<\/p>\n The unnamed cloud is approximately 125 million miles (200 million kilometers) across and is positioned around 13.3 astronomical units (or roughly 13.3 Earth-sun distances) from J0705+0612. For context, that would put it around halfway between Saturn<\/a> and Uranus<\/a> if it were located in our solar system<\/a>. At this distance, it takes about 44 years for the cloud to fully orbit its home star.<\/p>\n Gemini South’s newly operational Gemini High-resolution Optical Spectrograph<\/a> (GHOST) instrument, which captures specific wavelengths of light given off by different molecules, played a key role in the study. It peered deeper into the cloud than other telescopes can, enabling the researchers to probe exactly what the cloud was made of.<\/p>\n The results “exceeded all expectations,” revealing an abundance of metals, such as iron and calcium, Zakamska said. The GHOST data also enabled the team to track subtle movements within the cloud, which is “something we’ve never been able to do before in a system like this,” she added.<\/p>\n \n (Image credit: International Gemini Observatory\/NOIRLab\/NSF\/AURA\/Kwon O Chul)<\/p>\n After reviewing the cloud’s movements, it quickly became clear that the metallic mass was being held together by a hefty object at its center. Based on the size of the cloud, this could either be a gas giant several times larger than Jupiter<\/a>, a low-mass star in a binary pair with J0705+0612, or a brown dwarf \u2014 a sort of planet-star hybrid<\/a> that’s more massive than Jupiter but not massive enough to sustain nuclear fusion in its core.<\/p>\n If the cloud surrounds a star, then it would be classified as a circumsecondary disk because its host star is the secondary, or smaller, star in its binary pair. But if it is being held together by a planet, then it would be dubbed a circumplanetary disk. The researchers suggest the cloud is more likely held together by a star, due to high levels of infrared radiation glowing from the cloud. However, it is too early to tell for sure.<\/p>\n You may like<\/p>\n The next mystery is how the cloud formed. The researchers predict that the cloud is around 2 billion years old, hinting that it is younger than J0705+0612, which is likely closer in age to the sun<\/a> (around 4.6 billion years old). This would mean that it is not left over from the star system’s creation, like most other similar disks.<\/p>\n![\"A](\"https:\/\/www.newsbeep.com\/au\/wp-content\/uploads\/2026\/01\/6oBKjNQtshaA9tvmiksfcc.jpg\")
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