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And such a Planet Nine will be exceptionally difficult to actually spot it, as it is so far away that one year would last thousand Earth years. Planet Nine: Astrophysicist reveals surprising find.
Capture of a free-floating planet is a leading explanation for the origin of Planet Nine and we show that the probability of capturing a primordial black hole instead is comparable Jakub Scholtz, James Unwin.
Although their black hole theory is a controversial one, it could one day be testable. Planet Nine: Might the hypothetical body actually be a black hole Image: Getty.
This, he says, could validate the collision hypothesis. The mystery of Fomalhaut b seems mostly settled, but now researchers await the launch of the James Webb Telescope in Kalas says the telescope will "probably give the next big leap in understanding the planetary system around Fomalhaut.
Be respectful, keep it civil and stay on topic. We delete comments that violate our policy , which we encourage you to read.
Discussion threads can be closed at any time at our discretion. Astronomers solve mystery of the vanishing planet with new NASA data Fomalhaut b was discovered 16 years ago but then it disappeared.
Jackson Ryan. April 20, p. Fomalhaut b As luck would have it An animation simulating the collision of two huge asteroids. He noticed something weird with Fomalhaut b: Its light was fading.
A suspicious fat man, Merry Fellow Oo, tries to steal a bird. Having listened to the speech of the Chatterer, the crew of "Pegas" heads for the Jellyfish system.
On the road, the heroes rescue robots of the planet Shelezyaka from diamond dust, mixed into machine oil. On the third planet of the Jellyfish system Alisa finds "mirrors" — the flowers which are memorable and displaying everything that occurred before them.
By means of mirrors the heroes find out that on the planet there are Verkhovtsev and the Merry Fellow. In attempt to fly in a safe place of "Pegas" falls in a trap.
Seleznyov and Green are captured by pirates, Alisa manages to run away. On the planet the captain Buran, and with him — the real Verkhovtsev lands.
Alisa asks them for help. Meanwhile, the Merry Fellow threatening to murder the captives, demands from captain Kim locked in the ship, a formula of absolute fuel.
Buran's invasion rescues the heroes. The double Verkhovtsev, Glot, is exposed. The Merry Fellow in attempt to escape falls into the clutches a bird of prey, Krok.
The captains and researchers return home. Pyotr Vishnyakov Prof. Verhovtsev, Glot Vladimir Druzhnikov Cpt. Nikolai Grabbe Cpt.
The film was adapted twice for the US market. It was first brought over as a video release in , with dubbed voices. The second time, it was released in the s as part of Mikhail Baryshnikov 's "Stories from My Childhood" series.
This series consisted of films that were bought by California-based company Films by Jove from Soyuzmultfilm for the international market.
The film has been released on DVD several times the latest release, which featured rather misleading cover art, was in October .
The original Russian version with English subtitles is here: . 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. A variant of this, called splashing, would have involved collisions between molten objects at lower velocities, releasing droplets into space that solidified into chondrules.
The nebula shock model, meanwhile, posits that Mars-sized planetary embryos moving through the nebula could act like boats sailing through water, fusing dust into chondrules.
Other ideas include radiative heating, a relatively new idea that suggests planetesimals flying low over molten bodies could have been roasted and then cooled to produce chondrules.
Against this rising theoretical tide, some wilder notions have already been ruled out. Events from outside the solar system such as gamma-ray bursts—enormously energetic explosions from sources such as merging neutron stars or black holes—were once considered a possibility, but now seem implausible owing to the great distances involved.
Even so, many models still remain, complicated by the fact that chondrules are not really predicted by planet formation at all.
Narrowing down which of the remaining theories is correct is hard, and arguments can get heated. At stake is what role chondrules played in our solar system.
If they were among the first solids to form, then some inescapable process took place around our young sun that could explain how planet formation begins around most any star.
But if not, are they less vital to the process than once thought? Most of our ideas on chondrule formation come from modeling of the early solar system and performing experiments on Earth to replicate different formation methods.
Meteorite scientist Aimee Smith from the University of Manchester and her colleagues are one of several teams around the world that perform such experiments, mixing chemicals into a powder to resemble different types of known chondrule compositions.