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Исследование космоса (в научных целях)

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After troubleshooting communications, flight controllers have confirmed Odysseus is upright and starting to send data.
Right now, we are working to downlink the first images from the lunar surface
А на этом сайте охуительная история как все висело на волоске и пришлось написать программный патч в последний час перед приземлением
 

Hubble Telescope witnesses a new star being born in a stunning cosmic light show (image)​

The infant star FS Tau B is blasting out a powerful jet of matter that is slamming into sounding material.

A bright point of light shines near center-right with diffraction spikes, surrounded by glowing clouds against black space. A blue jet of material extends roughly throughout the center of the image, partially obscured by the clouds.

A Hubble image of the FS Tau systen with a bright four pointed light at its center representing the infant star FS Tau B(Image credit: NASA, ESA, K. Stapelfeldt (NASA JPL), G. Kober (NASA/Catholic University of America))

The Hubble Space Telescope has imaged a powerful jet erupting from a natal envelope of gas and dust that represents a newly born star announcing itself to the cosmos.
Hubble spotted the infant star slicing its way out of the nebula that birthed it when it zoomed in on the youthful multi-star system FS Tau. Located 450 light years from Earth, FS Tau is part of the Taurus-Auriga region. This region of space houses a stellar nursery of dark clouds of gas and dust, or "molecular clouds," that are home to numerous newly forming protostars and young stars.

Astronomers had previously discovered binary infant stars in this 2.8 million-year-old nebula, and now a second infant star, designated FS Tau B, has made itself known.
Related: Hubble Space Telescope discovers 'failed stars' are bad at relationships too

Both FS Tau B and the previously discovered infant stars in the FS Tau stellar nursery, a binary named FS Tau A (Haro 6-5A), are shrouded in illuminated gas and dust. This represents what is left of the matter in which overdense patches formed and collapsed to birth these stars.

A bright point of light shines near center-right with diffraction spikes, surrounded by glowing clouds against black space. A blue jet of material extends roughly throughout the center of the image, partially obscured by the clouds



A Hubble image of the FS Tau systen with a bright four pointed light at its center representing the infant star FS Tau B (Image credit: NASA, ESA, K. Stapelfeldt (NASA JPL), G. Kober (NASA/Catholic University of America)f)
As the Hubble image shows FS Tau B is partially obscured by a dark, vertical lane of dust. This is believed to be the edge of a pancake-shaped gathering of gas, and dust called a protoplanetary disk that surrounds the infant star. As the name suggests, this material left over from the formation of FS Tau B will eventually coalesce to form planets.
FS Tau B isn't a fully-fledged star just yet. This protostar is currently gathering material from its surroundings. Once it has accumulated enough mass, the pressure at the heart of FS Tau B will be so great that hydrogen begins to undergo nuclear fusion to create helium in its stellar core. That is the nuclear process that defines the main sequence lifetime of a star.
 
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