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annarita ruberto
Worked at Ministry of National Education
Attended University of Salento
Lives in Ravenna (Italy)
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annarita ruberto

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charly avital's profile photoStephen Fletcher's profile photoAli Faisol's profile photoLandy Ortiz's profile photo
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Looks like some type of free energy device. Very nice. Thank you
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annarita ruberto

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The Sombrero Galaxy in Infrared

(This image was shared by APoD on January 21, 2007.)

This floating ring is the size of a galaxy. In fact, it is part of the photogenic Sombrero Galaxy, one of the largest galaxies in the nearby Virgo Cluster of Galaxies.

The dark band of dust that obscures the mid-section of the Sombrero Galaxy in optical light actually glows brightly in infrared light.
The below image shows the infrared glow, recorded by the orbiting Spitzer Space Telescope, superposed in false-color on an existing image taken by NASA's Hubble Space Telescope in optical light.

The Sombrero Galaxy, also known as M104, spans about 50,000 light years across and is located 28 million light-years from Earth at the southern edge of the rich Virgo cluster of Galaxies. Equivalent to 800 billion suns, Sombrero is one of the most massive objects in that group.

The hallmark of Sombrero is a brilliant white, bulbous core encircled by the thick dust lanes comprising the spiral structure of the galaxy.
As seen from Earth, the galaxy is tilted nearly edge-on. We view it from just six degrees north of its equatorial plane. This rich system of globular clusters is estimated to be nearly 2,000 in number which is 10 times as many as in our Milky Way galaxy.

Similar to the clusters in the Milky Way, the ages range from 10-13 billion years old. Embedded in the bright core of M104 is a smaller disk, which is tilted relative to the large disk.
The HST paired with the Spitzer infrared telescope, offers this striking composite capturing the magnificence of the Sombrero galaxy.
In the Hubble view, the galaxy resembles a broad-rimmed Mexican hat, whereas in the Spitzer striking infrared view, the galaxy looks more like a bulls eye.

The full view provided by Spitzer shows the disk is warped, which is often the result of a gravitational encounter with another galaxy, and clumpy areas spotted in the far edges of the ring indicate young star forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy as well, where there is a huge black hole believed to be a billion times more massive than our Sun.

M104 can be seen with a small telescope in the direction of the constellation Virgo.

Credit: R. Kennicutt (Steward Obs.) et al., SSC, JPL, Caltech, NASA

Further reading and references

► The Sombrero Galaxy in Infrared >> http://go.nasa.gov/2ivw2WM

► Sombrero Galaxy (M104) in Infrared Light>> http://bit.ly/2j2n7Z6

#Universe, #HubbleSpaceTelescope, #SombreroGalaxy, #M104, #MilkyWayGalaxy, #Astronomy, #Space
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collins ijessei's profile photoannarita ruberto's profile photonima alizadeh's profile photoLuis Fernandez's profile photo
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BEAUTIFUL
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Crescent Jupiter with the Great Red Spot

This image of a crescent Jupiter and the iconic Great Red Spot was created by a citizen scientist (Roman Tkachenko) using data from Juno's JunoCam instrument.
You can also see a series of storms shaped like white ovals, known informally as the "string of pearls."
Below the Great Red Spot a reddish long-lived storm known as Oval BA is visible.

The image was taken on Dec. 11, 2016 at 2:30 p.m. PST (5:30 p.m. EST), as the Juno spacecraft performed its third close flyby of Jupiter. At the time the image was taken, the spacecraft was about 285,100 miles (458,800 kilometers) from the planet.

► JunoCam's raw images are available, for the public to peruse and process into image products, at>> www.missionjuno.swri.edu/junocam.

► More information about Juno is online at>> http://www.nasa.gov/juno and http://missionjuno.swri.edu.

Image Credit: NASA/JPL-Caltech/SwRI/MSSS/Roman Tkachenko

► Source>> http://photojournal.jpl.nasa.gov/catalog/PIA21376

#SolarSystem #Jupiter, #GreatRedSpot, #NASA, #JunoMission
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Tulus Sitorus's profile photoJesula Cherenfant's profile photoEdna Peters's profile photoHemal Amratlal's profile photo
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Jupiter is nice planet
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annarita ruberto

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Eurasian Jay (Garrulus glandarius)

The Eurasian jay (Garrulus glandarius) is a species of bird occurring over a vast region from Western Europe and north-west Africa to the Indian Subcontinent and further to the eastern seaboard of Asia and down into south-east Asia. Across its vast range, several very distinct racial forms have evolved to look very different from each other, especially when forms at the extremes of its range are compared.

The bird is called jay, without any epithets, by English speakers in Great Britain and Ireland. It is the original 'jay' after which all others are named.

Eurasian Jay feeds primarily on invertebrates such as caterpillars and beetles during the breeding and nesting seasons. It gleans from foliage in trees. But as other Corvidae, it also takes eggs and nestlings of several bird species.
During autumn and winter, it feeds on seeds and berries, chestnuts and acorns. One jay often caches acorns in winter (up to 3000 a month), by burying each acorn in the leaf litter or beneath low vegetation. It has learnt to know the green shoots of oak produced by the buried acorns. The next summer, it easily finds them and feeds the germinated acorn. It is a prolific planter of oaks!

Eurasian Jay usually flies fairly low and between trees. In flight, the white rump is very conspicuous. It performs undulating flight.
During migrations or movements in flocks, they climb high and move out with steady wing beats.

Breeding season varies according to the range.
Eurasian Jays have long-term pair-bonds and are solitary nesters.

Photo credit: Conny Lundström >> http://bit.ly/2jnOAVD

Further reading and references

► Eurasian Jay>> http://bit.ly/2jopHJA

► Eurasian Jay>> http://bit.ly/1XQnSm1


#Biodiversity, #EurasianJay, #Birds, #Animals, #Garrulusglandarius
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avinash jadhav's profile photoJohnnilmini Gomez's profile photoYoussef فديوRiahi's profile photoOlga Kalmuk's profile photo
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Wow super
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Mars Then and Now

Two images of Mars taken over 100 years apart. The first was drawn by Eugene Antoniadi in 1894, the second is from Hubble during the close approach of Mars in 2003. It's interesting to see what they got right and what they got wrong.
Notably the extensive system of 'Martian Canals', which Percival Lowell was so adamant existed and proved the presence of Martians.

Actually, a hot debate topic of the late 1800s, several prominent astronomers including Percival Lowell not only claimed to see an extensive system of long straight canals on Mars, but used them to indicate that intelligent life exists there.

The relatively close opposition of 1894 was used to make drawings like the one digitally re-scaled on the below left.

In more modern times, the latest Mars opposition has allowed the Hubble Space Telescope to capture a picture of similar orientation. Comparison of the two images shows that large features were impressively recorded, but that an extensive system of long and straight canals just does not exist.

Satellites orbiting Mars have now shown conclusively that the red planet does indeed have surface features similar to canals, but that these are usually smaller, curved, and less extensive than that previously claimed. Real canyon systems like Noctis Labyrinthus are most likely cracks caused by surface stress.

► Image source>> https://apod.nasa.gov/apod/ap031112.html

Credit & Copyright: Tom Ruen, Eugene Antoniadi, Lowell Hess, Roy A. Gallant, HST, NASA

Further reading

► Great Debates in Astronomy>> https://apod.nasa.gov/debate/debate.html

► Mars Exploration>> http://mars.jpl.nasa.gov/

► Percival Lowell>> http://www.daviddarling.info/encyclopedia/L/LowellP.html

► Eugène Antoniadi>> http://www.daviddarling.info/encyclopedia/A/Antoniadi.html

► Canals of Mars>> http://www.daviddarling.info/encyclopedia/M/Marscanals.html

#MartianCanals, #Mars, #SolarSystem, #Hubble, #NoctisLabyrinthus
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Talha Abbasi's profile photoDinah Masango's profile photoRohit Kr Sharma's profile photoPatricia Williams's profile photo
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Amazing
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The Vortex at Saturn's North Pole from Cassini

Close up of the central part of the hexagonal cloud system that surrounds the north pole of Saturn.

False color composite from red, CB2 and MT2 filters images.

Original image data dated on or about December 30, 2013.

► Source>>
http://www.planetary.org/multimedia/space-images/saturn/vortex-at-saturns-north-pole-from-cassini.html

► Credit: NASA / JPL-Caltech / Space Science Institute / Alexis Tranchandon / Solaris

Related posts

► In the Center of Saturn's North Polar Vortex>>
https://plus.google.com/+annaritaruberto/posts/HPzbYH9F1NP

► Enter the Vortex ... in Psychedelic Color>> https://plus.google.com/+annaritaruberto/posts/8K68p51GPhq

#Saturn, #Vortex, #Cassini, #SolarSystem, #NASA, #Space
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Grażyna Domagalska's profile photoStefano Muccinelli's profile photoBhanu pratap singh's profile photoRichard “Bkat Dahgz” Shane's profile photo
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+Bhanu pratap singh​ why I practice Christianity sir, folly to those who believe in themselves to explain our existence without acknowledging a master Creator of total Mass! 

annarita ruberto

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It holds Peace and Harmony
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Our Ability to Recognize Faces Improves from Infancy to Adulthood

A comparison of kid brains and grown-up brains may explain why our ability to recognize faces keeps getting better until about age 30.

Brain scans of 25 adults and 22 children showed that an area devoted to facial recognition keeps growing long after adolescence, researchers report in the journal Science.

The area didn't acquire more neurons, says Jesse Gomez, a graduate student in neurosciences at Stanford University and the study's lead author. Instead the brain region became more densely populated with the structures that connect and support neurons.

Understanding how facial recognition develops throughout childhood could make it easier to figure out why some people have difficulty recognizing faces, researchers say.

Gomez hopes to scan the brains of people with "face blindness," a disorder that can leave a person unable to recognize even familiar faces.

And Suzy Scherf, an assistant professor of psychology at Penn State University, wants to know whether people with autism, who often struggle to recognize faces, have abnormal development in the facial recognition area of their brains.

► The study "Microstructural proliferation in human cortex is coupled with the development of face processing" published in the journal Science>> http://science.sciencemag.org/content/355/6320/68

► Image source>> http://bit.ly/2juzHAP

Further reading and references

► Brain Area That Recognizes Faces Gets Busier And Better In Young Adults>> http://n.pr/2hXcLvq

► Brain’s face recognition area grows much bigger as we get older>> http://bit.ly/2jjja5q


#Neuroscience, #Brain, #BrainScans, #FacialRecognition, #Research, #HumanCortex
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Re analyzed
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Great Rift Near the Center of the Milky Way

On November 10, 2016, APoD shared this stunning image about the Great Rift.

Let's try to learn more.

Over 100 telescopic image panels in this amazing vertical mosaic span about 50 degrees across the night sky.
They follow part of the Great Rift, the dark river of dust and molecular gas that stretches along the plane of our Milky Way Galaxy.
More precisely, the Great Rift (sometimes called the Dark Side, Dark Rift, or, less commonly, Dark River) is a series of overlapping, non-luminous, molecular dust clouds that are located between the Solar System and the Sagittarius Arm of the Milky Way Galaxy at a distance of about 100 parsecs or about 300 light years (2×10^15 miles or 3×10^15 kilometers) from Earth. The clouds are estimated to contain about 1 million solar masses of plasma and dust.

Start at top center and you can follow the galactic equator down through brighter stars in constellations Aquila, Serpens Cauda, and Scutum.
At the bottom is Sagittarius near the center of the Milky Way. Along the way you'll encounter many obscuring dark nebulae hundreds of light-years distant flanked by bands of Milky Way starlight, and the telltale reddish glow of starforming regions.

Notable Messier objects include The Eagle (M16) and Omega (M17) nebulae, the Sagittarius Star Cloud (M24), the beautiful Trifid (M20) and the deep Lagoon (M8).

Image Credit & Copyright: Rogelio Bernal Andreo (Deep Sky Colors)

► Source>> https://apod.nasa.gov/apod/ap161110.html

Further reading and references

► Near the core of the Milky Way>> https://roundme.com/tour/85245/view/214717/

► Great Rift>> https://en.wikipedia.org/wiki/Great_Rift_(astronomy)

► Paddle the Milky Way’s Dark River>> http://www.skyandtelescope.com/observing/a-trip-down-the-great-rift/

► Galactic equator>> http://www.atlasoftheuniverse.com/galchart.html

► Messier object>> https://en.wikipedia.org/wiki/Messier_object

► Dark nebula>> https://en.wikipedia.org/wiki/Dark_nebula

#Universe, #GreatRift, #MilkyWay, #DarkNebulae, #Astronomy, #Space
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Paul Houchin's profile photoMaruf Islam's profile photoDiamonddds Back's profile photoRunveer Sooraj's profile photo
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Amazing
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Two New Missions to Explore the Early Solar System

NASA has selected two missions that have the potential to open new windows on one of the earliest eras in the history of our solar system – a time less than 10 million years after the birth of our sun.

The missions, known as Lucy and Psyche, were chosen from five finalists and will proceed to mission formulation, with the goal of launching in 2021 and 2023, respectively.

Lucy, a robotic spacecraft, will visit a target-rich environment of Jupiter’s mysterious Trojan asteroids. Scheduled to launch in October 2021, the spacecraft is slated to arrive at its first destination, a main asteroid belt, in 2025.
Then, from 2027 to 2033, Lucy will explore six Jupiter Trojan asteroids.

The Psyche mission will explore one of the most intriguing targets in the main asteroid belt – a giant metal asteroid, known as 16 Psyche, about three times farther away from the sun than is the Earth. The asteroid measures about 130 miles in diameter and, unlike most other asteroids that are rocky or icy bodies, it is thought to be comprised of mostly metallic iron and nickel, similar to Earth’s core.
The Psyche robotic mission is targeted to launch in October of 2023, arriving at the asteroid in 2030, following an Earth gravity assist spacecraft maneuver in 2024 and a Mars flyby in 2025.

Learn more>> https://www.nasa.gov/press-release/nasa-selects-two-missions-to-explore-the-early-solar-system

► Gif source>> http://nasa.tumblr.com/page/2


#Planets, #SolarSystem, #SpaceExploration, #NASA
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charly avital's profile photoHari Prasad's profile photoFreddie Loyie's profile photoCarlos Miller's profile photo
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sound good and wonderfull
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NGC 1977: Running Man Nebula

NGC 1977 is one of the most-recognized highlights in the constellation of Orion.
Although classified as an open cluster embedded within nebulosity, this area just north of the Orion Nebula is generally recognized as the Running Man Nebula owing to the emission nebulosity at the center which is in the formation of a running man.

The cluster is approximately 1,500 light-years away and spans approximately 20' in diameter. It is dominated by a number of bright stars ranging from mag 4 to mag 6 and whose light reflects off gas in the immediate vicinity and thus leading to reflection nebulosity.

Two other reflection nebulae sitting on the shoulders of the humanoid figure have classifications within the NGC catalog, namely NGC 1975 to the east and NGC 1973 to the west. Also, an area of protostar formation to the south is known as Herbig-Haro 45.

► Source>> http://www.perseus.gr/Astro-DSO-NGC-1977.htm

► This view of the nebula NGC 1977 was acquired in November–December 2015. >>
http://www.adamblockphotos.com/ngc-1977.html
Credit: Adam Block / Mount Lemmon SkyCenter / University of Arizona

Further reading

► NGC 1973, NGC 1975 and NGC 1977>> https://en.wikipedia.org/wiki/NGC_1973,_NGC_1975_and_NGC_1977

► The Orion Nebula and Running Man Nebula>>
http://www.skyandtelescope.com/online-gallery/the-orion-nebula-and-running-man-nebula/

► 'Running Man' Races in Spectacular Nebula Photo>>
http://www.space.com/21520-running-man-nebula-photo.html

#Universe, #RunningManNebula, #NGC1977, #OrionNebula, #OrionConstellation, #Space, #Astronomy
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+Akbar Hussain thanks 
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Asteroid (226514) 2003 UX34 Is a Binary System

Arecibo and Goldston planetary radar observations of 250 m asteroid (226514) 2003 UX34 reveal it is a binary system!

The Minor Planet Center has classified 2003 UX34 as a "Potentially Hazardous Asteroid."

This gif demonstrates the orbit of the secondary object about the primary; each frame is a sum of 3 minutes of data.

NEA 2003 UX34 was discovered in October 2003 by Spacewatch at Kitt Peak. At its closest approach on January 2, 2017, it was within a distance 19 times the Earth-Moon distance.

► Source>> http://www.naic.edu/~pradar/

Further reading

► Goldstone Radar Observations Planning: 2003 UX34>>
http://echo.jpl.nasa.gov/asteroids/2003UX34/2003UX34_planning.2017.html


#SolarSystem, #Asteroid , #AreciboPlanetaryRadar , #2265142003UX34, #NearEarthAsteroids
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Very kool. 👽
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annarita's Collections
Work
Occupation
I teach mathematics and science and work at educational research.
Skills
Science communication and e-learning. Scientific blogging
Employment
  • Ministry of National Education
    Tenured teacher at secondary school
  • "Scuola & Didattica" - Educational fortnightly magazine in Italian
    Freelance journalist of scientific and educational articles
  • Collaboration with various educational websites
Places
Map of the places this user has livedMap of the places this user has livedMap of the places this user has lived
Currently
Ravenna (Italy)
Previously
Lecce - Firenze
Story
Tagline
We can achieve what strongly we want!
Introduction
I teach mathematics and science and I wrote (2000-2013) for "Scuola e Didattica"- Educational fortnightly magazine in Italian (Editrice La Scuola).

I'm a member of Google+ Create w/verified Google+ Account

I'm also interested in web 2.0, social network and much more. I love reading, writing, painting, photography, good music, and more.

My posts are prevalently about Science and Mathematics for a general audience, but also about Art, beautiful images/photos and interesting  gifs. I share often scientific news that can be useful to many people.

I would like to look at the profiles of everyone who circles me, but there are too many. ;)
Anyway, I will definitely look at your profile if you engage with my posts.

Furthermore, I am interested in following people who post quality original content, regardless of the number of their followers. 

Instead I am not interested in following people if they never engage with my own content.

If you consider interesting my posts, you can circle me:). I'd like to read your posts and to interact with you here on Googleplus
Bragging rights
I experimented at school a research scholarship in Science, producing approximately over 200 pages of Materials for Science, published by IRRE- ER (Institute of Educational Research Emilia-Romagna, Italy). I was also part, along with 50 teachers selected nationwide, of The SENIS Project, a pilot project from Ministry of National Education for improving the scientific formation of teachers at secondary school. This Project has collected a lot of educational resources, published in a book by Ministry of National Education.
Education
  • University of Salento
    Master's Degree in Physics
  • Classical Lyceum
    Watch: http://en.wikipedia.org/wiki/Liceo_classico
  • University of Florence
    Advanced course in methods of communication and networked learning
  • University of Tuscia
    1. Advanced course on assessment/evaluation and managing portfolio. 2. Master in elearning and Learning Object
Basic Information
Gender
Female
Relationship
Married