QuoteA bonobo demonstrated the ability to track imaginary objects in controlled tests, challenging the belief that imagination is uniquely human and hinting at deep evolutionary roots.
In a set of carefully designed experiments modeled on children's tea parties, researchers at Johns Hopkins University found that an ape could engage in pretend play. The results mark the first controlled demonstration that an ape can imagine objects that are not actually there, a skill long considered uniquely human.
Across three separate tests, the bonobo interacted with invisible juice and imaginary grapes in a consistent and reliable way. The performance challenges longstanding assumptions about the limits of animal cognition.
The researchers conclude that the ability to understand pretend objects falls within the mental capacities of at least one enculturated ape. They suggest this ability could trace back 6 to 9 million years to a common ancestor shared by humans and other apes.
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QuoteAbstract:
Secondary representations enable our minds to depart from the here-and-now and generate imaginary, hypothetical, or alternate possibilities that are decoupled from reality, supporting many of our richest cognitive capacities such as mental-state attribution, simulation of possible futures, and pretense.
We present experimental evidence that a nonhuman primate can represent pretend objects. Kanzi, a lexigram-trained bonobo, correctly identified the location of pretend objects (e.g., "juice" poured between empty containers), in response to verbal prompts in scaffolded pretense interactions. Across three experiments, we conceptually replicated this finding and excluded key alternative explanations.
Our findings suggest that the capacity to form secondary representations of pretend objects is within the cognitive potential of, at least, an enculturated ape and likely dates back 6 to 9 million years, to our common evolutionary ancestors.
QuoteOne of the brightest stars in the Andromeda galaxy quietly collapsed into a black hole without any of the fanfare of a spectacular supernova.
What makes this startling discovery even more remarkable is that the first signs of the transformation were recorded back in 2014 – data that is crucial for understanding the different ways black holes can form after the death of a giant star.
"This has probably been the most surprising discovery of my life," says astronomer Kishalay De of Columbia University in the US, who led the research. "The evidence of the disappearance of the star was lying in public archival data, and nobody noticed for years until we picked it out."
When a massive star many times heavier than the Sun dies, it's not expected to go quietly. Once nuclear fusion in the core can no longer generate sufficient outward pressure against the inward pull of gravity, the core collapses.
This can send a giant shock tearing outward through the star, triggering a supernova explosion that sends the star's outer material flying, while the core transforms into either a neutron star or a black hole.
However, this is not the only way this transformation can take place. In some scenarios, the outward shock stalls. Instead of ripping the star apart, the explosion fizzles out, and the material ends up falling back onto the newly formed black hole. Because this is a much less dramatic process than a supernova, clear evidence of it is relatively rare.
"Unlike finding supernovae, which is easy because the supernova outshines its entire galaxy for a few weeks, finding individual stars that disappear without producing an explosion is remarkably difficult," De explains.
Only one such event had been documented previously, a star recorded vanishing around 2010 in a galaxy 22 million light-years away. Now, by carefully looking over archival observations of the Andromeda galaxy, De and his colleagues have found another, and it's even clearer than the previous example.
M31-2014-DS1 was a supergiant star that started out about 13 times the mass of the Sun and shone brightly, even across the 2.5 million light-year distance between the Milky Way and Andromeda.
Then, in 2014, NASA's NEOWISE telescope recorded it suddenly shining more intensely in infrared, increasing its brightness by about 50 percent over about two years.
Then, between 2016 and 2022, it dimmed dramatically to the point where, by 2023, it completely vanished from view in optical wavelengths.
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QuoteWhen a massive star reaches the end of its lifetime, its core collapses and releases neutrinos that drive a shock into the outer layers (the stellar envelope). A sufficiently strong shock ejects the envelope, producing a supernova. If the shock fails to eject it, the envelope is predicted to fall back onto the collapsing core, producing a stellar-mass black hole (BH) and causing the star to disappear. We report observations of M31-2014-DS1, a hydrogen-depleted supergiant in the Andromeda Galaxy. In 2014, it brightened in the mid-infrared, then from 2017 to 2022, it faded by factors of ≳ 104 in optical light (becoming undetectable) and ≳ 10 in total light. We interpret these observations, and those of a previous event in NGC 6946, as evidence for failed supernovae forming stellar-mass BHs.