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Planet Nine: The black hole theory is a controversial one Image: Getty. Dubbed BP, it attracted attention because of its uniquely unusual orbit.
This orbit could be caused by the gravity of a distant ninth planet. This would need to be four times the size of Earth and 10 times as dense.
Planet Nine: The body was first posited in Image: Getty. Instead, it may be the lingering light from a giant collision between two huge asteroids.
An animation simulating the collision of two huge asteroids. The ring of debris surrounding star Fomalhaut is displayed in yellow, while inset, a simulation shows the fading signal from to The notion Fomalhaut b may not be an exoplanet has been raised since its discovery by Kalas in Although visible in optical light, researchers couldn't find the infrared signature a planet that size should create.
As a result, Fomalhaut b's true identity has remained enigmatic. Alternative hypotheses have been suggested in the past, including in Kalas's original paper.
There have been suggestions Fomalhaut b is a dust-cloud or material captured from the huge disk of debris surrounding Fomalhaut, the star.
The team has already scheduled in almost 50 days of observation time for Fomalhaut b when James Webb gets off the ground in From a pinprick of light in data, Fomalhaut b became a ghost of a planet, the light that appeared in Hubble data began to dissipate and expand before disappearing in Plugging the collision of two gargantuan pre-planets, around miles wide kilometers , into their system, the team discovered the characteristics seen by Hubble matched up neatly.
The model accounts for all of the strangeness seen with Fomalhaut b during its observation history, from Kalas's discovery to some of the last observations seven years ago.
In this version, the soundtrack was replaced and about 6 minutes were cut out. From Wikipedia, the free encyclopedia. DVD cover Krupnyy Plan.
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Download as PDF Printable version. Natalya Orlova [Note 1]. Maksimovich Geliy Arkadyev Gennady Morozov. Kim Nikolai Grabbe Cpt. YLE Nelonen. United States.
English [ citation needed ]. Tallinnfilm Kanal 2. And CB chondrites hold a particularly unique accolade, being the only type of chondrite for which there is near-universal agreement on how they formed.
Because apart from this one anomaly, the exact formation process for chondrules and chondrites remains a mystery—but not for any lack of trying.
For decades scientists have devised and tested myriad different formation models, but a consensus has remained elusive.
We just have to work out what that is. In , at the Lunar and Planetary Science Conference in Houston, a stunned audience watched as John Wood—one of the most revered scientists studying chondrules—appeared to admit defeat in understanding their origin.
Like many before him, Wood had become fascinating by chondrules when he first laid eyes on them. But he was frustrated at the lack of progress that had been made.
A few years later, facing a lack of funding, he opted to retire, turning his attentions to oil painting and spending time with his wife.
The speech was a shock to many. The whole room erupted in applause. Yet one could be forgiven for pessimistically siding with Wood.
Against such magnificent achievements, the stubborn enigma of the lowly chondrule seems to shrink even smaller than its already niche status.
Today there are, the joke goes, as many theories about chondrule formation as there are chondrule scientists themselves—with the acerbic addendum that tomorrow there will inevitably be even more.
The problem of chondrules has from the start been intergenerational, inspiring one cohort after another to try their hand at tackling the issue, with varying success.
The main problem is finding a model that can explain all the different, diverse properties of chondrules. To make chondrules, dust must have been heated to temperatures of up to 2, degrees Celsius by some process in the early solar system, before rapidly cooling over just days or even hours.
This process, whatever it was, likely occurred throughout the solar system, in order to account for the large abundance of chondrules found in chondrites on Earth.
And the chondrules must also have drifted for a time through the dusty environs around our young sun, to account for the telltale rims of accumulated dust that encase their centers.
Most chondrule scientists fall into one of two camps. The first believes that chondrules were among the first solid objects to appear in the solar system, forming directly from the solar nebula—the cloud of dust and gas that surrounded our young sun.
This would make chondrules a key stepping-stone from miniscule dust to larger kilometer-sized planetesimals.
The second camp believes that chondrules were not among the first solids to form, but actually arose after planetesimals—perhaps even after the planets themselves—being instead a by-product of the planet-formation process rather than being actively part of it.
Other models in this camp include magnetohydrodynamics, where huge magnetic fields would trap sheets of electric current to create hot spots tens or hundreds of thousands of kilometers across that melt dust grains to churn out chondrules.
In the other camp, which proposes chondrule formation was post-planetesimal, one of the more prominent models is called impact jetting.
Here, planetesimals would collide at high velocities, creating the necessary heat to produce chondrules.