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Get Outside and Spot June's Strawberry Moon This Week

Get Outside and Spot June's Strawberry Moon This Week

CNET09-06-2025

Not all full moons are created equal, and a great example of this is June's full moon, which you can check out this week. Also known as the strawberry moon, June's full moon will be one of the more interesting full moons of the year. It's a mini-moon, which means the moon is as far away from the Earth as its orbit will allow. It's also part of a major lunar standstill, which will give the moon a unique trajectory across the sky that only occurs every 18.6 years.
Your best chance to see the strawberry moon will be early on June 11, with the fullest possible moon not visible until 3:46 a.m. according to The Farmer's Almanac. It'll be only slightly less full on both June 10 and June 12.
Since it is a mini-moon, it'll also appear to be smaller and dimmer than a normal full moon. Anyone who caught one of four supermoons in 2024 will be able to spot the stark contrast between a supermoon and a mini-moon. During a supermoon, the moon is as close to the Earth as its orbit allows, a phenomenon known as perigee.
For a mini-moon, the moon is as far away from Earth as it can get, a phenomenon called apogee. It's a little less exciting than a supermoon, but for context, it's neat to know how dim and small the moon can get compared to how big and bright it can get during a supermoon.
The major lunar standstill
The strawberry moon is part of what's called a major lunar standstill. This occurs once every 18.6 years when the moon's orbit aligns just right with the Earth's tilt. As most astronomers can tell you, the moon rises and sets from different points of the horizon based on the time of year, the Earth's tilt, and the moon's orbit.
In short, the path the moon is taking through the sky is as long as it's going to get. This phenomenon isn't specific to June 2025. In fact, people will be able to view this phenomenon for most of the year. However, once it's gone, it'll be 18.6 years before it shows up again.
Another interesting tidbit about major lunar standstills is that the moon will be rising and setting on parts of the horizon where the sun will never go. This was noted by researchers at English Heritage, who are currently studying the notion that Stonehenge lines up with this once-in-a-generation event.

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This should have been it for the cosmos, but around 9 billion to 10 billion years after the Big Bang, the universe started to expand again, with this expansion accelerating, leading to the dark-energy dominated epoch. To understand why this is such a worrying puzzle, imagine giving a child on a swing a single push, watching their motion come to a halt, and then, for no discernible reason, they start swinging again, and this motion gets faster and faster. As if dark energy weren't strange enough already, recent results from the Dark Energy Spectroscopic Instrument (DESI) have indicated that this mysterious force is weakening. This is something that seemingly defies the standard model of cosmology or the Lambda Cold Dark Matter (LCDM) model, which relies on dark energy (represented by the cosmological constant or Lambda) being Poplawski theorizes that a spinning universe can both account for dark energy and explain why it is weakening. "Dark energy would emerge from the centrifugal force in the rotating universe on large scales," the theoretical physicist explained. "If the universe were flat, the centrifugal force would act only in directions perpendicular to the preferred axis." However, in Poplawski's black hole theory of cosmology, because the universe created by a black hole is closed, moving away in any direction would eventually lead to coming back from the opposite direction. That would mean the centrifugal force arising from a spinning universe becomes a force acting in all directions away from the universe's parent primordial white hole. "The magnitude of this force is proportional to the square of the angular velocity of the universe and the distance from the white hole," Poplawski said. "This relation takes the form of the force acting on a galaxy due to dark energy, which is proportional to the cosmological constant and the distance from the white hole. Therefore, the cosmological constant is proportional to the square of the angular velocity of the universe."But, how could this explain the DESI observations that seem to indicate that dark energy is getting weaker? "Because the angular momentum of the universe is conserved, it decreases as the universe expands," Poplawski said. "Consequently, the cosmological constant, which is the simplest explanation of dark energy, should also decrease with time. This result is consistent with recent observations by DESI." 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"The next step to advance these ideas is to determine the equation describing how the cosmological constant, generated by the angular velocity of the universe, decreases with time, and to compare this theoretical prediction with the observed decrease of dark energy," Poplawski concluded. "This research might involve searching for the metric describing an expanding and rotating universe."A pre-peer-reviewed version of Poplawski's research appears on the paper repository site arXiv.

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