Showing posts with label NASA. Show all posts
Showing posts with label NASA. Show all posts

Wednesday, April 29, 2020

Possible Life similarities between Jupiter's moon Europa and depths of the Oceans on Earth


I was very happy to read about the continuity of missions Jupiter’s moon Europa " Europa Clipper mission " We can only be very excited and curious to learn more about the depths of the oceans of Jupiter's moon Europe. The eventual life forms can be infinitely varied, the variety of life oceans of moon Europa is still a mystery at the moment. Thanks to NASA and I want to thank them for their efforts in all areas, we will unravel the mystery of this possible extraterrestrial life ocean soon.

Below is a list of 15 strange species from the depths of the planet Earth's oceans, about which we do not have much scientific information and creatures that still continue to amaze us and surrounded in mystery.  

Think of the endless evolutionary possibilities of Jupiter’s moon Europa my friends !


Gulper Eel or Pelican eel

The pelican eel (Eurypharynx pelecanoides) is a deep-sea eel rarely seen by humans, though it is occasionally caught in fishing nets. It is the only known member of the genus Eurypharynx and the family Eurypharyngidae. It belongs to the "saccopharyngiforms", members of which were historically placed in their own order, but are now considered true eels in the order Anguilliformes.

The Gulper Eel - Science-rumors

The pelican eel has been described by many synonyms, yet nobody has been able to demonstrate that more than one species of pelican eel exists. It is also referred to as the gulper eel (which can also refer to members of the related genus Saccopharynx), pelican gulper, and umbrella-mouth gulper. The specific epithet pelecanoides refers to the pelican, as the fish's large mouth is reminiscent of that of the pelican.


Sandra Raredon/Smithsonian Institution - cropped version of File:Eurypharynx pelecanoides X-ray.jpg

Description

Pelican eel specimens can be hard to describe, as they are so fragile that they become damaged when recovered from the immense pressure of the deep sea. The pelican eel's most notable feature is its large mouth, which is much larger than its body.

Gulper Eel Remarkable Large Mouth - Our Breathing Planet

The mouth is loosely hinged, and can be opened wide enough to swallow a fish much larger than the eel itself. The pouch-like lower jaw resembles that of a pelican, hence its name. The lower jaw is hinged at the base of the head, with no body mass behind it, making the head look disproportionately large. Its jaw is so large that it is estimated to be about a quarter of the total length of the eel itself. When it feeds on prey, water that is ingested is expelled via the gills.


Scripps Institution - UC San Diego Photo of the Week

Pelican eels are black or olive and some subspecies may have a thin lateral white stripe. They are ray-finned fish, and only resemble eels in appearance.  source of text wikipedia


Hatchetfish ( Marine hatchetfishes or deep-sea hatchetfishes )

Marine hatchetfishes or deep-sea hatchetfishes are small deep-sea mesopelagic ray-finned fish of the stomiiform subfamily Sternoptychinae. They should not be confused with the freshwater hatchetfishes, which are not particularly closely related Teleostei in the characiform family Gasteropelecidae.

MLTSHP Deep Sea Hatchetfish

Found in tropical, subtropical and temperate waters of the Atlantic, Pacific and Indian Oceans, marine hatchetfishes range in size from Polyipnus danae at 2.8 cm (1.1 in) to the c.12 cm (4.7 in)-long giant hatchetfish (Argyropelecus gigas).


Wild Facts Creepy alien fish

They are small deep-sea fishes which have evolved a peculiar body shape and like their relatives have bioluminescent photophores. The latter allow them to use counter-illumination to escape predators that lurk in the depths: by matching the light intensity with the light penetrating the water from above, the fish does not appear darker if seen from below. They typically occur at a few hundred meters below the surface, but their entire depth range spans from 50 to 1,500 meters deep. source of text wikipedia


Hagfish  ( Not to be confused with Hogfish )

Hagfish, of the class Myxini (also known as Hyperotreti), are eel-shaped, slime-producing marine fish (occasionally called slime eels). They are the only known living animals that have a skull but no vertebral column, although hagfish do have rudimentary vertebrae. Along with lampreys, hagfish are jawless; they are the sister group to jawed vertebrates, and living hagfish remain similar to hagfish from around 300 million years ago.

Hagfish Bizarre prehistoric alien Pinterest

The classification of hagfish had been controversial. The issue was whether the hagfish was a degenerate type of vertebrate-fish that through evolution had lost its vertebrae (the original scheme) and was most closely related to lampreys, or whether hagfish represent a stage that precedes the evolution of the vertebral column (the alternative scheme) as is the case with lancelets. Recent DNA evidence has supported the original scheme.

Hagfish OCEAN TREASURES

The original scheme groups hagfish and lampreys together as cyclostomes (or historically, Agnatha), as the oldest surviving class of vertebrates alongside gnathostomes (the now-ubiquitous jawed vertebrates). The alternative scheme proposed that jawed vertebrates are more closely related to lampreys than to hagfish (i.e., that vertebrates include lampreys but exclude hagfish), and introduces the category craniata to group vertebrates near hagfish.


Snipe Eel

Snipe eels are a family, Nemichthyidae, of eels that consists of nine species in three genera. They are pelagic fishes, found in every ocean, mostly at depths of 300–600 m but sometimes as deep as 4000 m. Depending on the species, adults may reach 1–2 m (39–79 in) in length, yet they weigh only 80-400 g (a few ounces to a pound).


They are distinguished by their very slender jaws that separate toward the tips as the upper jaw curves upward. The jaws appear similar to the beak of the bird called the snipe. Snipe eels are oviparous, and the juveniles, called Leptocephali (meaning small head), do not resemble the adults but have oval, leaf-shaped and transparent bodies.

A scale diagram of the layers of the pelagic zone. Mature snipe eels generally occupy the Bathypelagic Zone

Spectacular Snipe Eel Sighting Nautilus Live 

Different species of snipe eel have different shapes, sizes and colors. The similarly named bobtail snipe eel is actually in a different family and represented by two species, the black Cyema atrum and the bright red Neocyema erythrosoma.


Giant Isopod


A giant isopod is any of the almost 20 species of large isopods (crustaceans distantly related to shrimp and crabs, which are decapods) in the genus Bathynomus. They are abundant in the cold, deep waters of the Atlantic, Pacific, and Indian Oceans.[1][2] Bathynomus giganteus, the species upon which the generitype is based, is often considered the largest isopod in the world, though other comparably poorly known species of Bathynomus may reach a similar size (e.g., B. kensleyi). The giant isopods are noted for their resemblance to the much smaller common woodlouse (pill bug), to which they are related.

A frontal view of Bathynomus giganteus, showing its large, highly reflective compound eyes wikipedia

French zoologist Alphonse Milne-Edwards was the first to describe the genus in 1879 after his colleague Alexander Agassiz collected a juvenile male B. giganteus from the Gulf of Mexico; this was an exciting discovery for both scientists and the public, as at the time the idea of a lifeless or "azoic" deep ocean had only recently been refuted by the work of Sir Charles Wyville Thomson and others. No females were recovered until 1891.

The underside of Bathynomus giganteus wikipedia

Giant isopods are of little interest to most commercial fisheries, but are infamous for attacking and destroying fish caught in trawls. Specimens caught in the Americas and Japan are sometimes seen in public aquariums.


Sperm Whale or cachalot

The sperm whale (Physeter macrocephalus) or cachalot is the largest of the toothed whales and the largest toothed predator. It is the only living member of the genus Physeter and one of three extant species in the sperm whale family, along with the pygmy sperm whale and dwarf sperm whale of the genus Kogia.

Sperm Whales Clicking You Inside Out — James Nestor at The Interval youtube

The sperm whale is a pelagic mammal with a worldwide range, and will migrate seasonally for feeding and breeding. Females and young males live together in groups, while mature males (bulls) live solitary lives outside of the mating season. The females cooperate to protect and nurse their young. Females give birth every four to 20 years, and care for the calves for more than a decade. A mature sperm whale has few natural predators, although calves and weakened adults are sometimes killed by pods of killer whales (orcas).

The sperm whale's brain is the largest in the world, five times heavier than a human's. wikipedia

Mature males average 16 metres (52 ft) in length but some may reach 20.7 metres (68 ft), with the head representing up to one-third of the animal's length. Plunging to 2,250 metres (7,382 ft), it is the third deepest diving mammal, exceeded only by the Southern elephant seal and Cuvier's beaked whale. The sperm whale uses echolocation and vocalization as loud as 230 decibels (re 1 µPa m) underwater. It has the largest brain on Earth, more than five times heavier than a human's. Sperm whales can live 70 years or more.

Anatomy of the sperm whale's head. The organs above the jaw are devoted to sound generation. wikipedia

Spermaceti (sperm oil), from which the whale derives its name, was a prime target of the whaling industry, and was sought after for use in oil lamps, lubricants, and candles. Ambergris, a solid waxy waste product sometimes present in its digestive system, is still highly valued as a fixative in perfumes, among other uses. Beachcombers look out for ambergris as flotsam. Sperm whaling was a major industry in the 19th century, depicted in the novel Moby-Dick. The species is protected by the International Whaling Commission moratorium, and is listed as vulnerable by the International Union for Conservation of Nature.


Giant Tube Worm Riftia pachyptila

Riftia pachyptila, commonly known as giant tube worms, are marine invertebrates in the phylum Annelida[1] (formerly grouped in phylum Pogonophora and Vestimentifera) related to tube worms commonly found in the intertidal and pelagic zones. Riftia pachyptila live on the floor of the Pacific Ocean near black smokers, and can tolerate extremely high hydrogen sulfide levels. These worms can reach a length of 3 m (9 ft 10 in) and their tubular bodies have a diameter of 4 cm (1.6 in). Ambient temperature in their natural environment ranges from 2 to 30 degrees Celsius.

Photo of one of the largest concentrations of Riftia pachyptila observed, with anemones and mussels colonizing in close proximity. From the 2011 NOAA Galapagos Rift Expedition. The original NOAA image has been modified by increasing brightness. wikipedia

The common name "giant tube worm" is however also applied to the largest living species of shipworm, Kuphus polythalamia, which despite the name "worm" is a bivalve mollusc, rather than an annelid.


Dragon fish known as Stomiidae  other article about Deep-sea dragonfish, one of the most bizarre creatures of the Sea - VIDEO

Stomiidae is a family of deep-sea ray-finned fish, including the barbeled dragonfishes. They are quite small, usually around 15 cm, up to 26 cm. These fish are apex predators and have enormous jaws filled with fang-like teeth. 


Scientists crack secret of dragonfish's deadly 'invisible' teeth New York Post

They are also able to hinge the neurocranium and upper-jaw system, which leads to the opening of the jaw to more than 100 degrees.[1] This ability allows them to consume extremely large prey, often 50% greater than their standard length  



Angler fish

The anglerfish is a fish of the teleost order Lophiiformes It is a bony fish named for its characteristic mode of predation, in which a fleshy growth from the fish's head (the esca or illicium) acts as a lure for other fish.

Representatives of ceratioid families as recognized in this study-1. (A) Centrophrynidae: Centrophryne spinulosa Regan and Trewavas, 136 mm SL, LACM 30379-1; (B) Ceratiidae: Cryptopsaras couesii Gill, 34.5 mm SL, BMNH 2006.10.19.1 (photo by E. A. Widder); (C) Himantolophidae: Himantolophus appelii (Clarke), 124 mm SL, CSIRO H.5652-01; (D) Diceratiidae: Diceratias trilobus Balushkin and Fedorov, 86 mm SL, AMS I.31144-004; (E) Diceratiidae: Bufoceratias wedli (Pietschmann), 96 mm SL, CSIRO H.2285-02; (F) Diceratiidae: Bufoceratias shaoi Pietsch, Ho, and Chen, 101 mm SL, ASIZP 61796 (photo by H.-C. Ho); (G) Melanocetidae: Melanocetus eustales Pietsch and Van Duzer, 93 mm SL, SIO 55-229; (H) Thaumatichthyidae: Lasiognathus amphirhamphus Pietsch, 157 mm SL, BMNH 2003.11.16.12; (I) Thaumatichthyidae: Thaumatichthys binghami Parr, 83 mm SL, UW 47537 (photo by C. Kenaley); (J) Oneirodidae: Chaenophryne quasiramifera Pietsch, 157 mm SL, SIO 72-180. Courtesy of the American Society of Ichthyologists and Herpetologists.


Some anglerfish are notable for extreme sexual dimorphism and sexual symbiosis of the small male with the much larger female, seen in the suborder Ceratioidei. In these species, males may be several orders of magnitude smaller than females.

The Creepy Anglerfish Comes to Light. (Just Don't Get Too Close ...  NYT

Anglerfish occur worldwide. Some are pelagic (dwelling away from the sea floor), while others are benthic (dwelling close to the sea floor). Some live in the deep sea (e.g., Ceratiidae), while others on the continental shelf (e.g., the frogfishes Antennariidae and the monkfish/goosefish Lophiidae). Pelagic forms are most laterally compressed, whereas the benthic forms are often extremely dorsoventrally compressed (depressed), often with large upward-pointing mouths.



Viperfish

A viperfish is any species of marine fish in the genus Chauliodus. Viperfish are characterized by long, needle-like teeth and hinged lower jaws. A typical viperfish grows to lengths of 30 to 60 cm (12 to 23.5 in). Viperfish stay near lower depths in the daytime and shallower depths at night, primarily in tropical and temperate waters. Viperfish are believed to attack prey after luring them within range with light-producing organs called photophores, which are located along the ventral sides of its body, and with a prominent photophore at the end of a long spine in the dorsal fin reminiscent of the illicium of the unrelated deepsea anglerfishes. The viperfish flashes this natural light on and off, at the same time moving its dorsal spine around like a fishing rod and hanging completely still in the water. It also uses the light producing organ to communicate to potential mates and rivals.

Animal Diversity Web Chauliodus sloan

Viperfish vary in color from green, silver, to black. A viperfish uses its fang-like teeth to immobilize prey and would not be able to close its mouth because of their length, if it were not able to fold and curve them behind its head. The first vertebra behind the head of the viperfish absorbs the shock of biting prey. As with other deepsea fish, they are able to endure long periods with minimal food.

Viperfish are believed to live from 30 to 40 years in the wild, but in captivity they rarely live more than a few hours. Some species of dolphins and sharks are known to prey upon viperfish. Scientists believe they can swim at a speed of two body lengths per second, but this is not yet an official speed.

Viper fish zoom photo pinterest

Although it may appear to be covered in scales, it is covered by a thick, transparent coating of unknown substance. Extremely large, fang-like teeth give the fish a slightly protruded lower jaw which makes catching prey easy. The viperfish is lined with three different types of photophores, which some speculate are used to lure prey. They have microscopic spheres without a pigment layer that are scattered over the dorsal side, large spheres with a pigment coat, reflectors, and lens and large, bell-shaped organs with a pigment coat, reflectors, and lens that are grouped together in rows along the dorsal surface. Photophores can also be seen along the ventral and lateral surface of the fish. source wikipedia


Fangtooth


Fangtooths are beryciform fish of the family Anoplogastridae (sometimes spelled "Anoplogasteridae") that live in the deep sea. The name is from Greek anoplo meaning "unarmed" and gaster meaning "stomach". With a circumglobal distribution in tropical and cold-temperate waters, the family contains only two very similar species in one genus, with no known close relatives.

Anoplogaster cornuta - Wikipedia
Description

While understandably named for their disproportionately large, fang-like teeth and unapproachable visage, fangtooths are actually quite small and harmless to humans: the larger of the two species, the common fangtooth, reaches a maximum length of just 16 cm (6.3 in) the shorthorn fangtooth is less than half this size though currently known only from juvenile specimens.

New Scientist Up close with the giant teeth of the deep-sea fangtooth

The head is small with a large jaw and appears haggard, riddled with mucous cavities delineated by serrated edges and covered by a thin skin. The eyes are relatively small, set high on the head; the entire head is a dark brown to black and is strongly compressed laterally, deep anteriorly and progressively more slender towards the tail.

Laboratory News Common Fangtooth alien face

The fins are small, simple, and spineless; the scales are embedded in the skin and take the form of thin plates. As compensation for reduced eyes, the lateral line is well-developed and appears as an open groove along the flanks.


Vampire Squid

The vampire squid (Vampyroteuthis infernalis, lit. "vampire squid from Hell") is a small cephalopod found throughout temperate and tropical oceans in extreme deep sea conditions. Unique retractile sensory filaments justify the vampire squid's placement in its own order, Vampyromorphida, as it shares similarities with both octopuses and squid. As a phylogenetic relict, it is the only known surviving member of its order. The first specimens were collected on the Valdivia Expedition and they were originally described as an octopus in 1903 by German teuthologist Carl Chun, but later assigned to a new order together with several extinct taxa.

Vampire Squid (Vampyroteuthis infernalis) – Our Wild World

Description

The vampire squid can reach a maximum total length around 30 cm (1 ft). Its 15-centimetre (5.9 in) gelatinous body varies in colour from velvety jet-black to pale reddish, depending on location and lighting conditions. A webbing of skin connects its eight arms, each lined with rows of fleshy spines or cirri; the inner side of this "cloak" is black.



Only the distal halves (farthest from the body) of the arms have suckers. Its limpid, globular eyes, which appear red or blue, depending on lighting, are proportionately the largest in the animal kingdom at 2.5 cm (1 in) in diameter. The name of the animal was inspired by its dark colour, cloaklike webbing, and red eyes, rather than habit—it feeds on detritus, not blood.


Oarfish

Not to be confused with Paddlefish.

Oarfish are large, greatly elongated, pelagic lampriform fish belonging to the small family Regalecidae. Found in all temperate to tropical oceans yet rarely seen, the oarfish family contains three species in two genera. One of these, the giant oarfish (Regalecus glesne), is the longest bony fish alive, growing up to 8 m (26 ft) in length.

Sea Serpent - Can the Giant Oarfish Predict Earthquakes? The Vintage News

The common name oarfish is thought to be in reference either to their highly compressed and elongated bodies, or to the now discredited belief that the fish "row" themselves through the water with their pelvic fins. The family name Regalecidae is derived from the Latin regalis, meaning "royal". The occasional beachings of oarfish after storms, and their habit of lingering at the surface when sick or dying, make oarfish a probable source of many sea serpent tales.


Although the larger species are considered game fish and are fished commercially to a minor extent, oarfish are rarely caught alive; their flesh is not well regarded for eating due to its gelatinous consistency

United States Navy SEALS holding a 23-foot (7.0 m) giant oarfish, found washed up on the shore near San Diego, California, in September 1996 wikipedia

Anatomy and morphology

The dorsal fin originates from above the (relatively large) eyes and runs the entire length of the fish. Of the approximately 400 dorsal fin rays, the first 10 to 13 are elongated to varying degrees, forming a trailing crest embellished with reddish spots and flaps of skin at the ray tips. The pelvic fins are similarly elongated and adorned, reduced to one to five rays each. The pectoral fins are greatly reduced and situated low on the body.


The anal fin is completely absent and the caudal fin may be reduced or absent, as well, with the body tapering to a fine point. All fins lack true spines. At least one account, from researchers in New Zealand, described the oarfish as giving off "electric shocks" when touched.


Nautilus

The nautilus (from the Latin form of the original Ancient Greek: ναυτίλος, 'sailor') is a pelagic marine mollusc of the cephalopod family Nautilidae, the sole extant family of the superfamily Nautilaceae and of its smaller but near equal suborder, Nautilina.

It comprises six living species in two genera, the type of which is the genus Nautilus. Though it more specifically refers to species Nautilus pompilius, the name chambered nautilus is also used for any of the Nautilidae. All are protected under CITES Appendix II.

Nautilus, Palau wikipedia

Nautilidae, both extant and extinct, are characterized by involute or more or less convolute shells that are generally smooth, with compressed or depressed whorl sections, straight to sinuous sutures, and a tubular, generally central siphuncle. Having survived relatively unchanged for hundreds of millions of years, nautiluses represent the only living members of the subclass nautiloidea, and are often considered "living fossils".

Diagram of the anatomical structure of a female N. pompilius including most of its internal organs. wikipedia

The first and oldest fossil of Chambered Nautilus displayed at Philippine National Museum.
The word nautilus is derived from the Greek ναυτίλος nautílos and originally referred to the paper nautiluses of the genus Argonauta, which are actually octopuses. The word nautílos literally means "sailor", as paper nautiluses were thought to use two of their arms as sails



Coelacanth 

Latimeria chalumnae "fish with legs from Indian Ocean" the mysterious living fossil reveals its secrets

The coelacanths (/ˈsiːləkænθ/ (About this soundlisten) SEE-lə-kanth) constitute a now-rare order of fish that includes two extant species in the genus Latimeria: the West Indian Ocean coelacanth (Latimeria chalumnae) primarily found near the Comoro Islands off the east coast of Africa and the Indonesian coelacanth (Latimeria menadoensis). They follow the oldest-known living lineage of Sarcopterygii (lobe-finned fish and tetrapods), which means they are more closely related to lungfish and tetrapods than to ray-finned fish. They are found along the coastlines of the Indian Ocean and Indonesia. The West Indian Ocean coelacanth is a critically endangered species.

Preserved Latimeria menadoensis, Tokyo Sea Life Park, Japan wikipedia

Coelacanths belong to the subclass Actinistia, a group of lobed-finned fish related to lungfish and certain extinct Devonian fish such as osteolepiforms, porolepiforms, rhizodonts, and Panderichthys. Coelacanths were thought to have become extinct in the Late Cretaceous, around 66 million years ago, but were rediscovered in 1938 off the coast of South Africa.

Pectoral fin of a West Indian Ocean coelacanth wikipedia

The coelacanth was long considered a "living fossil" because scientists thought it was the sole remaining member of a taxon otherwise known only from fossils, with no close relations alive,[5] and that it evolved into roughly its current form approximately 400 million years ago. However, several recent studies have shown that coelacanth body shapes are much more diverse than previously thought.


Other articles on the same theme:









Text source wikipedia

Tuesday, April 28, 2020

Divine warning or just a coincidence? A potentially dangerous asteroid will pass tomorrow near Earth "the steroid appears to be wearing a face mask"

Asteroid (52768) 1998 OR2 Spalding Today


An asteroid with an estimated size of 2 kilometers will pass near Earth tomorow on April 29, at 9.56 GMT dont worry the risk of collision being excluded.

As a unique detail in the images captured by astronomers, the asteroid appears to be wearing a face mask. 

Asteroid 52768 (1998 OR2), discovered by NASA in 1998 will travel at a distance of about 6.2 million kilometers from Earth, at a speed of about 31,300 kilometers per hour.If it collided with Earth, the asteroid would cause "global effects," NASA officials said after discovering the cosmic object.

Radar image of asteroid 1998 OR2 acquired April 18, 2020, by astronomers at Arecibo Observatory. The radar data confirm that 1998 OR2 is at least 2 km in diameter [a little over a mile wide]. These radar images suggest it is spherical. It rotates once every 4.1 hours. Image via Arecibo Observatory in Puerto Rico.

In a completely unique way, in the images captured by the specialists from the Arecibo Astronomical Observatory in Puerto Rico, the asteroid seems to be wearing a face protection mask, according to CNN. The asteroid was included by NASA in the "potentially dangerous" category, like any other spacecraft approaching Earth at less than 7,480,000 kilometers.  descopera

The Arecibo Observatory wikipedia


According to information available to specialists to date, the largest asteroid that has passed Earth is 3122 Florence (1981 ET3). The object with a size of about 4-9 kilometers passed our planet on September 1, 2017 and is still expected to "visit" us on September 2, 2057.

3122 Florence is a stony trinary asteroid of the Amor group. It is classified as a near-Earth object and potentially hazardous asteroid. It measures approximately 5 kilometers in diameter. It orbits the Sun at a distance of 1.0–2.5 AU once every 2 years and 4 months (859 days); the orbit has an eccentricity of 0.42 and an inclination of 22° with respect to the ecliptic. Florence was discovered on 2 March 1981 by American astronomer Schelte J. "Bobby" Bus at Siding Spring Observatory.[3] Its provisional designation was 1981 ET3. It was named in honor of Florence Nightingale, the founder of modern nursing the naming citation was published on 6 April 1993 wiki



Other articles on the same theme:






Friday, December 7, 2018

US researchers succeeded in creating elementary particles using quantum computers with 512 qubits

Quantum computing has long dangled the possibility of superfast, super-efficient processing, and now search giant Google has jumped on board that future. popsci.com 



US researchers  succeeded in creating elementary particles using quantum computers with 512 qubits quantum bit. They estimate that 10 are needed at the power of 500 qubits or 1, e + 500 qubits to simulate the entire universe with all its fundamental particles. Each atom is composed of electrons, protons and neutrons, and each of these particles consists of 1 (electron) or 3 quartz

In quantum computing, a qubit or quantum bit (sometimes qbit) is the basic unit of quantum information—the quantum version of the classical binary bit physically realized with a two-state device. A qubit is a two-state (or two-level) quantum-mechanical system, one of the simplest quantum systems displaying the weirdness of quantum mechanics. Examples include: the spin of the electron in which the two levels can be taken as spin up and spin down; or the polarization of a single photon in which the two states can be taken to be the vertical polarization and the horizontal polarization. In a classical system, a bit would have to be in one state or the other. However, quantum mechanics allows the qubit to be in a coherent superposition of both states/levels at the same time, a property that is fundamental to quantum mechanics and thus quantum computing.

Autodesk qubits-explained


Each quark consists of 6 fundamental particles with different spin In particle physics, an elementary particle or fundamental particle is a subatomic particle with no substructure, thus not composed of other particles. Particles currently thought to be elementary include the fundamental fermions (quarks, leptons, antiquarks, and antileptons), which generally are "matter particles" and "antimatter particles", as well as the fundamental bosons (gauge bosons and the Higgs boson), which generally are "force particles" that mediate interactions among fermions. A particle containing two or more elementary particles is a composite particle.

Everyday matter is composed of atoms, once presumed to be matter's elementary particles—atom meaning "unable to cut" in Greek—although the atom's existence remained controversial until about 1910, as some leading physicists regarded molecules as mathematical illusions, and matter as ultimately composed of energy. Soon, subatomic constituents of the atom were identified. As the 1930s opened, the electron and the proton had been observed[citation needed], along with the photon, the particle of electromagnetic radiation. At that time, the recent advent of quantum mechanics was radically altering the conception of particles, as a single particle could seemingly span a field as would a wave, a paradox still eluding satisfactory explanation

The energy behind them is the same, only the mathematical equations that are those smells and spins are different

Therefore, this universal simulation is made up of immense energy and intense computational effort

Scientists simulate the Universe's birth (Credit: Patrick Landmann/Science Photo Library)


They believe that most of the characters in the local universe containing 7 trillions of galaxies, of which 250 billion stars, the rest being in the nebula;

Each galaxy is composed of a central black hole and between 100 and 1,000 billion stars
each star has between 10 and 100 planets

Each planet can have hundreds of natural satellites (Jupiter in our solar system as a gas giant)
and on every planet or satellite that meets the conditions can live billions of intelligent beings and trillions of beings in total

tecreview.tec


Well most of the characters are simulated they do not have the spirit of being outside the universe
however, the purpose of this gigantic simulation is historical, the purpose being to find out how the universe would evolve if some key characters would have done other things in life
that is, if a political leader like myself would live in poverty, he would not join a political party and would not become a president ...

The voice in the brain tells me that I have accomplished 93% of what I had to do until now, although only 20% of my real life has been respected it's actually pretty boring to follow your life's schedule as it's already just you know what you've done or suspect.


Other articles on the same theme:





Friday, April 28, 2017

Astronomers have discovered a new planet named LHS 1140b with the greatest chances of sustaining life. '' It's the most exciting planet ''

This artist's impression shows the exoplanet LHS 1140b, which orbits a red dwarf star 40 light-years from Earth and may be the new holder of the title 'best place to look for signs of life beyond the Solar System'. Using ESO's HARPS instrument at La Silla, and other telescopes around the world, an international team of astronomers discovered this super-Earth orbiting in the habitable zone around the faint star LHS 1140. This world is a little larger and much more massive than the Earth and has likely retained most of its atmosphere. Credit: ESO/spaceengine.org
An exoplanet orbiting a red dwarf star 40 light-years from Earth may be the new holder of the title 'best place to look for signs of life beyond the solar system.' Using ESO's HARPS instrument, and other telescopes, astronomers discovered a 'super-Earth' orbiting in the habitable zone around the star LHS 1140. This world is larger and more massive than the Earth and has likely retained most of its atmosphere. This makes it one of the most exciting targets for atmospheric studies.

The newly discovered super-Earth LHS 1140b orbits in the habitable zone around a faint red dwarf star named LHS 1140, in the constellation of Cetus (The Sea Monster). Red dwarfs are much smaller and cooler than the Sun and, although LHS 1140b is ten times closer to its star than the Earth is to the Sun, it only receives about half as much sunlight from its star as the Earth and lies in the middle of the habitable zone. The orbit is seen almost edge-on from Earth and as the exoplanet passes in front of the star once per orbit it blocks a little of its light every 25 days.

"This is the most exciting exoplanet I've seen in the past decade," said lead author Jason Dittmann of the Harvard-Smithsonian Center for Astrophysics (Cambridge, USA). "We could hardly hope for a better target to perform one of the biggest quests in science -- searching for evidence of life beyond Earth."

"The present conditions of the red dwarf are particularly favourable -- LHS 1140 spins more slowly and emits less high-energy radiation than other similar low-mass stars," explains team member Nicola Astudillo-Defru from Geneva Observatory, Switzerland.

For life as we know it to exist, a planet must have liquid surface water and retain an atmosphere. When red dwarf stars are young, they are known to emit radiation that can be damaging for the atmospheres of the planets that orbit them. In this case, the planet's large size means that a magma ocean could have existed on its surface for millions of years. This seething ocean of lava could feed steam into the atmosphere long after the star has calmed to its current, steady glow, replenishing the planet with water.

The discovery was initially made with the MEarth facility, which detected the first telltale, characteristic dips in light as the exoplanet passed in front of the star. ESO's HARPS instrument, the High Accuracy Radial velocity Planet Searcher, then made crucial follow-up observations which confirmed the presence of the super-Earth. HARPS also helped pin down the orbital period and allowed the exoplanet's mass and density to be deduced .

The astronomers estimate the age of the planet to be at least five billion years. They also deduced that it has a diameter 1.4 times larger than the Earth -- almost 18,000 kilometres. But with a mass around seven times greater than the Earth, and hence a much higher density, it implies that the exoplanet is probably made of rock with a dense iron core.

This super-Earth may be the best candidate yet for future observations to study and characterise its atmosphere, if one exists. Two of the European members of the team, Xavier Delfosse and Xavier Bonfils both at the CNRS and IPAG in Grenoble, France, conclude: "The LHS 1140 system might prove to be an even more important target for the future characterisation of planets in the habitable zone than Proxima b or TRAPPIST-1. This has been a remarkable year for exoplanet discoveries!" [4,5].

In particular, observations coming up soon with the NASA/ESA Hubble Space Telescope will be able to assess exactly how much high-energy radiation is showered upon LHS 1140b, so that its capacity to support life can be further constrained.

Further into the future -- when new telescopes like ESO's Extremely Large Telescope are operating -- it is likely that we will be able to make detailed observations of the atmospheres of exoplanets, and LHS 1140b is an exceptional candidate for such studies.

Notes

[1] The habitable zone is defined by the range of orbits around a star, for which a planet possesses the appropriate temperature needed for liquid water to exist on the planet's surface.

[2] Although the planet is located in the zone in which life as we know it could potentially exist, it probably did not enter this region until approximately forty million years after the formation of the red dwarf star. During this phase, the exoplanet would have been subjected to the active and volatile past of its host star. A young red dwarf can easily strip away the water from the atmosphere of a planet forming within its vicinity, leading to a runaway similar to that on Venus.

[3] This effort enabled other transit events to be detected by MEarth so that the astronomers could nail down the detection of the exoplanet once and for all.

[4] The planet around Proxima Centauri is much closer to Earth, but it probably does not transit its star, making it very difficult to determine whether it holds an atmosphere.

[5] Unlike the TRAPPIST-1 system, no other exoplanets around LHS 1140 have been found. Multi-planet systems are thought to be common around red dwarfs, so it is possible that additional exoplanets have gone undetected so far because they are too small.


Other articles on the same theme:





Story source: 
 
The above post is reprinted from materials provided by Sciencedaily . Note: Materials may be edited for content and length.

Monday, January 30, 2017

Researchers have found another planet (Wolf 1061c) that can sustain life: Located just 14 light-years away

Credit: The Wolf 1061 system. Credit: UNSW Sydney
An exoplanet with the prime conditions for life could be located just 14 light-years away, scientists report, in one of the closest neighbouring solar systems to our own.

New research suggests that a planet circling the star Wolf 1061 falls within what's called the star's habitable zone - making it one of the most likely neighbouring candidates for a planet that supports life.


This artist's concept illustrates a young, red dwarf star surrounded by three planets. Credit: wikipedia

"The Wolf 1061 system is important, because it is so close, and that gives other opportunities to do follow-up studies to see if it does indeed have life," says lead researcher Stephen Kane from San Francisco State University.

There are three planets orbiting Wolf 1061, but the planet Wolf 1061c is of particular interest.

Discovered in 2015, and with an estimated mass that's more than four times Earth's mass, Wolf 1061c is located right in the middle of Wolf 1061's habitable zone: the region where a planet's distance from its host star makes conditions suitable for liquid water and other life-supporting elements.

Our own Solar System runs by the same rules: conditions on Earth are just right for liquid water, whereas Mars is too cold.

To investigate whether Wolf 1061c might offer the same kind of habitability, the researchers analysed seven years of luminosity data from its host star and ran calculations of the exoplanet's orbit to figure out what the temperature and pressure on the surface could be.


The findings add weight to previous speculation that Wolf 1061c could be habitable – but just because the exoplanet is within a habitable zone, that doesn't necessarily mean it's one like Earth's.

The new data suggest that Wolf 1061c could have an atmosphere similar to what Venus had in its earliest days, meaning that any liquid water on the planet might not stick around for long. 

Previous research has suggested that high temperatures caused excessive water evaporation on Venus, and the newly formed water vapour in the atmosphere increased temperatures even further - a process known as a runaway greenhouse effect.

Now, the team thinks the same thing could be happening on Wolf 1061c, which is "close enough to the star that it's looking suspiciously like a runaway greenhouse", says Kane.

In addition, Wolf 1061c's orbit of its star varies much more quickly than Earth's orbit of the Sun, which would lead to chaotic climate changes such as a rapidly encroaching ice age (or warm phase).

So, is there life on Wolf 1061c?

We don't yet know, and to find out, we'll need more detailed measurements than what we have so far. To that end, Kane says NASA's James Webb telescope is one of the ways we'll be able to learn more about the exoplanet in the future.

Wolf 1061c Credit: Centauri Dreams

The telescope is launching next year, and its advanced optics should be able to reveal the atmospheric conditions on Wolf 1061c, and give us a better idea about whether water (and life) could really exist there.

Meanwhile, scientists from METI - the Messaging Extraterrestrial Intelligence organisation - are also interested in Wolf 1061c, and have been keeping a close eye on the exoplanet as they try to reach out to any alien life that might exist beyond our Solar System.

"I'm not holding my breath that we'll ever find evidence of life on Wolf 1061c," METI president Doug Vakoch told Rae Paoletta at Gizmodo.

"But the fact that there's a roughly Earth-like planet in the habitable zone of a star so close to our own Solar System is a good omen as we continue our search for life on other planets."

Other articles on the same theme:




Story source: 
The above post is reprinted from materials provided by Sciencealert . Note: Materials may be edited for content and length.

Sunday, January 15, 2017

2017 in Review: NASA’s Space Technology Mission Directorate (STMD) Pioneering Progress

Solar Electric Propulsion work is underway, sponsored by NASA's Space Technology Mission Directorate and managed by NASA's Glenn Research Center. A prototype 13-kilowatt Hall thruster, shown here, is tested to demonstrate the technology readiness needed for industry to continue the development of high-power solar electric propulsion into a flight-qualified system. Credits: NASA
NASA’s Space Technology Mission Directorate (STMD) is dedicated to pushing the technological envelope, taking on challenges not only to further space agency missions near Earth, but also to sustain future deep space exploration activities.

“In 2016, we completed several major program milestones,” explains Steve Jurczyk, NASA associate administrator for STMD.

During the year, STMD focused upon and made significant progress in advancing technologies and capabilities in the following areas:

Space Power and Propulsion;




Enabling engine 

Jurczyk points to areas of notable progress in fiscal year 2016, particularly work on high-power Solar Electric Propulsion (SEP) – an enabler for cost-effective deep space exploration.


Asteroid Redirect Mission makes use of solar electric propulsion. The vehicle’s solar arrays collect power from the sun and convert it to energy to ionize and accelerate xenon propellant, resulting in the bright blue plume at the rear of the vehicle. Credits: NASA

SEP makes use of large solar cell arrays that convert collected sunlight energy to electrical power. That energy is fed into extremely fuel-efficient thrusters that provide gentle but nonstop thrust throughout the mission. SEP thrusters are designed to use far less propellant than comparable, conventional chemical propulsion systems.

“We completed the development and testing of a prototype SEP engine at NASA’s Glenn Research Center. Also, we have contracted with Aerojet Rocketdyne to develop the SEP flight system for the Asteroid Redirect Robotic Mission,” Jurczyk notes.

Furthermore, SEP solar array technology is being transitioned into commercial application, Jurczyk adds, by both Space Systems Loral and Orbital ATK.

Green propellant 

Another 2016 spotlight on progress, Jurczyk observes, is the integration and testing of the Green Propellant Infusion Mission (GPIM). Now ready for launch in 2017, GPIM will test the distinctive quality of a high-performance, non-toxic, “green” fuel in orbit.

STMD worked with Aerojet Rocketdyne in Redmond, Washington and GPIM prime contractor Ball Aerospace & Technologies Corp. in Boulder, Colorado, to develop the spacecraft capable of using the unique propellant. It will fly on the U.S. Air Force’s Space Test Program (STP-2) mission.

Given the term “green” propellant, Jurczyk points out that the Air Force-developed fuel is a hydroxyl ammonium nitrate-based fuel/oxidizer mix, also known as AF-M315E. GPIM will flight demonstrate this fuel designed to replace use of highly toxic hydrazine and complex bi-propellant systems now in common use today.

“GPIM’s green propellant is less toxic than hydrazine. It will reduce spacecraft processing costs and it has 40 percent higher performance by volume than hydrazine,” Jurczyk says.

Aerojet Rocketdyne, builder of GPIM’s set of thrusters, is now marketing the novel thrusters as a product. The aerospace firm is also working with NASA’s Glenn Research Center to further enhance the thrusters, looking to reduce cost and add to their reliability, Jurczyk adds. “So we’re collaborating with the aerospace company to further advance this technology and I’m pleased with the progress.”

Push the technology 

Jurczyk reports that STMD-supported work on the Deep Space Atomic Clock, DSAC for short, is ongoing.

DSAC is a small, low-mass atomic clock based on mercury-ion trap technology that will be demonstrated in space, providing unprecedented stability needed for next-generation deep space navigation and radio science. NASA’s Jet Propulsion Laboratory oversees project development of DSAC, which offers the promise of 50 times more accuracy than today’s best navigation clocks.


STMD’s Flight Opportunities program includes use of Masten Space Systems’ XA-0.1B “Xombie” vertical-launch, vertical-landing reusable rocket as a risk-reduction activity, testing science experiments and hardware before long duration spaceflight. Vehicle is shown soaring above Mojave Air and Space Port in California. Credits: NASA Photo/Tom Tschida

The task of designing DSAC has not been trouble-free, but it represents a tenant of STMD “to push the technology,” Jurczyk responds. Taking on the challenges of space-rating terrestrial based atomic clock technology is not easy. However, the path forward has been outlined with launch of DSAC now eyed for next year.

The DSAC demonstration unit and payload is to be hosted on a spacecraft provided by Surrey Satellite Technologies U.S. of Englewood, Colorado, lofted spaceward as part of the U.S. Air Force Space Test Program 2 mission aboard a Space X Falcon 9 Heavy booster.

Tipping point partnerships 

In 2016, STMD entered into their first set of public-private partnerships, a solicitation that proved very beneficial – to both industry and NASA. Called “Utilizing Public-Private Partnerships to Advance Tipping Point Technologies,” Jurczyk is pleased with this facilitated collaborative effort with industry. These partnerships require companies to contribute at least 25 percent of the funding; NASA contributes up to $20 million for ground-based efforts.

With the recent increase of the U.S. private sector interest in space applications, NASA is seeking commercial space technologies that are at a “tipping point” in their development.

“We do many one-on-one discussions with companies about their interests. For NASA, we want to help advance technologies that boost commercial products and services,” he points out. The Tipping Point partnerships have led to contracts, for example, in space robotic manufacturing and small spacecraft technologies.

Similarly, Jurczyk adds that in 2016, STMD saw collaborative opportunity for industry to tap into NASA expertise, allowing companies to use space agency talent and facilities. This collaboration is made possible through non-reimbursable, no-exchange-of-funds Space Act Agreements. Those types of agreements, he emphasizes, have enabled private-sector advancements in technologies such as small launch vehicle rocket engines and advanced structures for small boosters.

Flight opportunities

“It has been a good and productive year for STMD’s Flight Opportunities program,” Jurczyk advises.

That program provides affordable access to relevant space-like environments for NASA payloads. This activity makes use of a variety of flight platforms, such as Blue Origin’s New Shepard suborbital vehicle, Masten Space Systems’ XA-0.1B “Xombie” vertical-launch, vertical-landing reusable rocket, as well as the UP Aerospace SpaceLoft sounding rocket.


STMD’s lineup of smallsat launches in 2017 includes the CubeSat Proximity Operations Demonstration (CPOD) project that will demonstrate rendezvous, proximity operations and docking using two CubeSats. Credits: NASA/Ames/Tyvak Nano-Satellite Systems, Inc.

“We can ‘ring out’ experiments and technologies in short duration exposure to relevant flight conditions before they go onto longer duration flight on space missions,” Jurczyk explains. “It’s a risk reduction activity,” he continues, for example, in life science research or shaking out various robotic technologies.

Big year ahead 

Looking into 2017, STMD’s Jurczyk highlights the launch of the Green Propellant Infusion Mission and the Deep Space Atomic Clock. “Those are two major flight demonstrations and are very important.”

Among a host of STMD-supported activities, next year will see flight of small satellites to showcase, for instance, optical laser communications. Then there’s the Integrated Solar Array and Reflectarray Antenna (ISARA) for advanced communications and the CubeSat Proximity Operations Demonstration (CPOD). The function of CPOD is to trial-run autonomous rendezvous and docking, Jurczyk says.

“There’s going to be a lot going on,” Jurczyk concludes. “It’ll be a big year for small satellites and space technology.”


Other articles on the same theme:





Story source: 
The above post is reprinted from materials provided by NASA. Note: Materials may be edited for content and length.