KREUZADER (Posts tagged space)

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Where the Solar system meets the solar neighbourhood: patterns in the distribution of radiants of observed hyperbolic minor bodies“Around the same time our ancestors left Africa, a dim red dwarf star came to within 0.8 light-years of our Sun, marking...

Where the Solar system meets the solar neighbourhood: patterns in the distribution of radiants of observed hyperbolic minor bodies

Around the same time our ancestors left Africa, a dim red dwarf star came to within 0.8 light-years of our Sun, marking the closest known flyby of a star to our Solar System. New research suggests Scholz’s Star, as it’s known, left traces of this interstellar encounter by perturbing some comets in the outer Oort Cloud.

[…]

Scholz’s Star, this research suggested, just grazed the outer reaches of the Oort Cloud, that remote bubble of debris that marks the outermost limits of the Sun’s dominant gravitational influence. The red dwarf has been drifting ever since, and it’s now about 20 light-years away. The University of Rochester researchers who conducted the 2015 study said it was unlikely that Scholz’s Star, with a mass around 9 percent of the Sun, and it’s brown dwarf, at about 6 percent the Sun’s mass, were able to disturb or jostle any of the objects in the Oort Cloud to a significant degree.  

But new research published this week in Monthly Notices of the Royal Astronomical Society suggests this interpretation was wrong, and that Scholz’s Star did in fact influence the trajectories of some Oort Cloud objects. In the study, astronomer brothers Carlos de la Fuente Marcos and Raúl de la Fuente Marcos from Complutense University of Madrid, along with Sverre J. Aarseth from the University of Cambridge, identified the movements of dozens of known Oort Cloud objects as having been influenced by this ancient encounter.

Source: Gizmodo
astronomy space
Mission to an Interstellar Asteroid“ A sky map showing the probability that a future interstellar asteroid will approach the Solar System on a trajectory parallel to that direction. The darker colors indicate a higher probability. The axes denote...

Mission to an Interstellar Asteroid

A sky map showing the probability that a future interstellar asteroid will approach the Solar System on a trajectory parallel to that direction. The darker colors indicate a higher probability. The axes denote degrees from a heliocentric point of view and the ecliptic is plotted in black. The sky positions of the constellations Serpens and Lepus, which are close in proximity to the Solar apex and anti-apex respectively, are plotted for context. The black circle indicates the sky location that ‘Oumuamua entered our Solar System, consistent with the prediction that the majority of these objects will approach with velocities parallel to the galactic apex.

Source: centauri-dreams.org
'oumuamua oumuamua asteroid astronomy space
Government Scientists Have A Plan For Blowing Up Asteroids With A Nuke“The Hypervelocity Asteroid Mitigation Mission for Emergency Response (HAMMER) spacecraft — a collaboration between the National Nuclear Security Administration, NASA, and two...

Government Scientists Have A Plan For Blowing Up Asteroids With A Nuke

The Hypervelocity Asteroid Mitigation Mission for Emergency Response (HAMMER) spacecraft — a collaboration between the National Nuclear Security Administration, NASA, and two Energy Department weapons labs — would either steer its 8.8-ton bulk (called an “impactor”) into a small asteroid, or carry a nuclear device to deflect a big one.

“If the asteroid is small enough, and we detect it early enough, we can do it with the impactor,” physicist David Dearborn of the Lawrence Livermore National Laboratory told BuzzFeed News. “The impactor is not as flexible as the nuclear option when we really want to change the speed of the body in a hurry.”

Just because these plans now exist does not mean the spacecraft will ever get built. NASA scientists declined to give a cost estimate for a mission, citing the sensitivity of pricing information, but for comparison, NASA’s more complex OSIRIS-REx mission, now on its way to Bennu, cost $800 million.

Source: BuzzFeed
nasa space asteroid planetary defense
“The Twin Study propelled NASA into the genomics era of space travel. It was a ground-breaking study comparing what happened to astronaut Scott Kelly, in space, to his identical twin brother, Mark, who remained on Earth. The perfect nature versus...

The Twin Study propelled NASA into the genomics era of space travel. It was a ground-breaking study comparing what happened to astronaut Scott Kelly, in space, to his identical twin brother, Mark, who remained on Earth. The perfect nature versus nurture study was born.

The Twins Study brought ten research teams from around the country together to accomplish one goal: discover what happens to the human body after spending one year in space. NASA has a grasp on what happens to the body after the standard-duration six-month missions aboard the International Space Station, but Scott Kelly’s one-year mission is a stepping stone to a three-year mission to Mars.

[…]

Another interesting finding concerned what some call the “space gene”, which was alluded to in 2017. Researchers now know that 93% of Scott’s genes returned to normal after landing. However, the remaining 7% point to possible longer term changes in genes related to his immune system, DNA repair, bone formation networks, hypoxia, and hypercapnia.

Source: nasa.gov
nasa space

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In this composite image, derived from data collected by the Jovian Infrared Auroral Mapper (JIRAM) instrument aboard NASA’s Juno mission to Jupiter, shows the central cyclone at the planet’s north pole and the eight cyclones that encircle it. JIRAM collects data in infrared, and the colors in this composite represent radiant heat: the yellow (thinner) clouds are about 9 degrees Fahrenheit (-13° Celsius) in brightness temperature and the dark red (thickest) are around -181 degrees Fahrenheit (-118.33° Celsius).

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This computer-generated image shows the structure of the cyclonic pattern observed over Jupiter’s south pole. Like in the North, Jupiter’s south pole also contains a central cyclone, but it is surrounded by five cyclones with diameters ranging from 3,500 to 4,300 miles (5,600 to 7,000 kilometers) in diameter. Almost all the polar cyclones (at both poles), are so densely packed that their spiral arms come in contact with adjacent cyclones. However, as tightly spaced as the cyclones are, they have remained distinct, with individual morphologies over the seven months of observations detailed in the paper.

Source: jpl.nasa.gov
jupiter juno space nasa

For hundreds of years, this gaseous giant planet appeared shrouded in colorful bands of clouds extending from dusk to dawn, referred to as zones and belts.

[…]

The bands were thought to be an expression of Jovian weather, related to winds blowing eastward and westward at different speeds.   This animation illustrates a recent discovery by Juno that demonstrates these east-west flows, also known as jet-streams penetrate deep into the planet’s atmosphere, to a depth of about 1,900 miles (3,000 kilometers).  Due to Jupiter’s rapid rotation (Jupiter’s day is about 10 hours), these flows extend into the interior parallel to Jupiter’s axis of rotation, in the form of nested cylinders. Below this layer the flows decay, possibly slowed by Jupiter’s strong magnetic field. 

jupiter nasa space juno
lordtableshark
itsfullofstars:
“ AI HEADING TO THE ISS What could possibly go wrong, Dave?
“ The crew on board the International Space Station (ISS) will soon welcome a new member — one that is 3D-printed from metal and plastic and is described by its creators as...
itsfullofstars

AI HEADING TO THE ISS

What could possibly go wrong, Dave?

The crew on board the International Space Station (ISS) will soon welcome a new member — one that is 3D-printed from metal and plastic and is described by its creators as “a kind of flying brain.”

It goes by the name CIMON, short for “Crew Interactive Mobile Companion.” Built by the aerospace design company Airbus in collaboration with IBM, CIMON houses artificial intelligence (AI) in an autonomous, spherical body that would “float” in the space station’s microgravity environment, with a screen that can display data readouts for astronauts — or present an image of a friendly face — as well as a voice shaped by IBM’s AI technology.

kreuzaderny

love 2 be trapped in space with my floating face friend h̸͕̜̰̘͖̺͙̠͎͍̞̦̀͑̇̑̾͗̈́̒̓͌͘͘ͅͅe̷̹̰̹̜̩̦̎̇̃̈́́̏̇͂̾͗̚l̷̼͙̗̮̖͍̹͍̘̞̻͚̫̜̰̀̂͆̾͆̅̆̀́͝p̶͖͓̬̲͖̫̮̱̗̝͓͖͍̮̟͋̋͛̂̎̚͠ ̶͙͇͔̝͂ͅu̸̧̹̔͜s̸̯͎̒̋̌̾̂̇̅͜͝

space artificial intelligence international space station robot
Direct Multipixel Imaging and Spectroscopy of an Exoplanet with a Solar Gravity Lens Mission“ The remarkable optical properties of the solar gravitational lens (SGL) include major brightness amplification (~1e11 at wavelength of 1 um) and extreme...

Direct Multipixel Imaging and Spectroscopy of an Exoplanet with a Solar  Gravity Lens Mission

The remarkable optical properties of the solar gravitational lens (SGL) include major brightness amplification (~1e11 at wavelength of 1 um) and extreme angular resolution (~1e-10 arcsec) in a narrow field of view. A mission to the SGL carrying a modest telescope and coronagraph opens up a possibility for direct megapixel imaging and high-resolution spectroscopy of a habitable Earth-like exoplanet at a distance of up to 100 light years. The entire image of such a planet is compressed by the SGL into a region with a diameter of ~1.3 km in the vicinity of the focal line. The telescope, acting as a single pixel detector while traversing this region, can build an image of the exoplanet with kilometer-scale resolution of its surface, enough to see its surface features and signs of habitability. We report here on the results of our initial study of a mission to the deep outer regions of our solar system, with the primary mission objective of conducting direct megapixel high-resolution imaging and spectroscopy of a potentially habitable exoplanet by exploiting the remarkable optical properties of the SGL. Our main goal was to investigate what it takes to operate spacecraft at such enormous distances with the needed precision. Specifically, we studied i) how a space mission to the focal region of the SGL may be used to obtain high-resolution direct imaging and spectroscopy of an exoplanet by detecting, tracking, and studying the Einstein ring around the Sun, and ii) how such information could be used to detect signs of life on another planet. Our results indicate that a mission to the SGL with an objective of direct imaging and spectroscopy of a distant exoplanet is challenging, but possible. We composed a list of recommendations on the mission architectures with risk and return tradeoffs and discuss an enabling technology development program.
Source: arxiv.org
astronomy space
Mistakes in the Drake Equation“There are 400 billion other solar systems in our galaxy, and it’s been around for 10 billion years. Clearly it stands to reason that there must be extraterrestrial civilizations. We know this, because the laws of nature...

Mistakes in the Drake Equation

There are 400 billion other solar systems in our galaxy, and it’s been around for 10 billion years. Clearly it stands to reason that there must be extraterrestrial civilizations. We know this, because the laws of nature that led to the development of life and intelligence on Earth must be the same as those prevailing elsewhere in the universe.

Hence, they are out there. The question is: how many?

Source: centauri-dreams.org
drake equation seti space
Proxima’s orbit around Alpha Centauri“Proxima and Alpha Centauri AB have almost identical distances and proper motions with respect to the Sun. Although the probability of such similar parameters is in principle very low, the question as to whether...

Proxima’s orbit around Alpha Centauri

Proxima and Alpha Centauri AB have almost identical distances and proper motions with respect to the Sun. Although the probability of such similar parameters is in principle very low, the question as to whether they actually form a single gravitationally bound triple system has been open since the discovery of Proxima one century ago. Owing to HARPS high precision absolute radial velocity measurements and the recent revision of the parameters of the Alpha Cen pair, we show that Proxima and Alpha Cen are gravitationally bound with a high degree of confidence. The orbital period of Proxima is approximately 550 000 years. With an excentricity of 0.50 (+0.08 -0.09), Proxima comes within 4.3 (+1.1 -0.9) kau of Alpha Cen at periastron. Its orbital phase is currently close to apastron (13.0 +0.3 -0.1 kau). This orbital motion may have influenced the formation or evolution of the recently discovered planet orbiting Proxima as well as circumbinary planet formation around Alpha Cen.

Source: arxiv.org
alpha centauri proxima centauri astronomy space