#acri-st

[sitting-on-me-bum]

NASA’s James Webb Telescope Captures the Fiery Remains of a Dying Star in Unprecedented Detail

Images courtesy of ESA/Webb, NASA, CSA, M. Barlow (University College London), N. Cox (ACRI-ST), R. Wesson (Cardiff University)

[daughter-of-mary]

[wonders-of-the-cosmos]

NASA’s James Webb Space Telescope has observed the well-known Ring Nebula in unprecedented detail. Formed by a star throwing off its outer layers as it runs out of fuel, the Ring Nebula is an archetypal planetary nebula. This new image from Webb’s NIRCam (Near-Infrared Camera) shows intricate details of the filament structure of the inner ring. There are some 20,000 dense globules in the nebula, which are rich in molecular hydrogen. In contrast, the inner region shows very hot gas. The main shell contains a thin ring of enhanced emission from carbon-based molecules known as polycyclic aromatic hydrocarbons (PAHs). 

Credit: ESA/Webb, NASA, CSA, M. Barlow (University College London), N. Cox (ACRI-ST), R. Wesson (Cardiff University)

[thepastisalreadywritten]

The Year’s Most Spectacular Photos from the James Webb Telescope

By Jeffrey Kluger

December 22, 2023

Close to 1,500 light years from Earth lie a pair of baby stellar twins known as Herbig-Haro 46/47 — which are barely a few thousand years old.

A star the size of our sun, by contrast, takes an average of 50 million years to reach even the stellar equivalent of young adulthood It's Herbig-Haro 46/47's extreme youth that gives the formation more of a blob-like appearance than the stellar duo it is.

Young stars are buried in clouds of dust and gas, which they absorb as they grow. Sometimes, however the infant stars ingest too much material too fast.

When that happens, dust and gas erupts from both sides of the formation, giving the young pair their misshapen look.

But if you have patience — 50 million years worth of patience — what is a blob today will be stars tomorrow.

NASA, ESA, CSA. Image Processing: Joseph DePasquale (STScI)

A pair of brilliant stellar nurseries located 1,600 light years from Earth, the Orion Nebula and Trapezium Cluster are home to a relative handful of very young but very bright stars.

Four of the stars are easy to see with a simple, amateur, four-inch telescope.

One of the four — the beast of the young litter — is especially visible, a full 20,000 times brighter than our sun.

Apart from their four main stars, the Orion Nebula and Trapezium cluster contain approximately 700 additional young stars at various stages of gestation.

NASA, ESA, CSA/Science leads and image processing: M. McCaughrean, S. Pearson, CC BY-SA 3.0 IGO

(L): It’s not easy being a Wolf-Rayet star, like this specimen imaged by the Webb telescope at a distance of 15,000 light years.

A rare species of stellar beast — NASA estimates there are only 220 of them in a Milky Way galaxy with at least 100 billion stars — the Wolf-Rayet burns hot and burns fast, with temperatures 20 to 40 times the surface of the sun.

All of that rapidly expended energy causes the star to lose its hydrogen envelope quickly and expose its helium core.

The result: a very early and very violent death.

A star like our sun burns for about 10 billion years. As for a Wolf-Rayet? Just a few hundred thousand before it dissolves into cosmic dust.

NASA, ESA, CSA, STScI, Webb ERO Production Team

(R): If the Wolf-Rayet star dies an ugly and violent death, the celebrated Ring Nebula, photographed by the Webb at a distance of 2,000 light years from Earth, has been expiring beautifully.

The glowing remains of a sun-like star, the nebula was discovered in 1779 by the French astronomer Antoine Darquier de Pellepoix.

As the nebula throws off its outer layers of ionized gas, it reveals its characteristic blue interior, composed of hydrogen and oxygen that have not yet been expelled off by the nebula’s stellar wind.

ESA/Webb, NASA, CSA, M. Barlow (University College London), N. Cox (ACRI-ST), R. Wesson (Cardiff University)

Dwarf galaxy NGC 6822 lives up to to its name — home to just 10 million stars, compared to the minimum of 100 billion in the Milky Way.

But what NGC 6822 lacks in numbers, it makes up in spectacle — which the keen eye of the Webb telescope has revealed.

Discovered in 1884 by American astronomer E.E Barnard, NGC 6822, is now known to have a prodigious dust tail measuring 200 light years across..

What's more, it's home to a dense flock of stars that glow 100,000 times brighter than our sun.

ESA/Webb, NASA & CSA, M. Meixnev

Spiral galaxies are often defined by uneven — and even ragged — arms.

But not galaxy M51, which lies 27 million light years from Earth and is defined by the tautness of its arms and the compactness of its structure.

M51 isn't alone in space. Nearby lies the companion galaxy NGC 5195.

The two galaxies are engaged in something of a gravitational tug of war — one that the NGC 5195 is winning.

NGC's constant gravitational pull is thought to account for both the tightly woven structure of M51's arms and for tidal forces that are thought lead to the creation of new stars in the arms.

ESA/Webb, NASA & CSA, A. Adamo (Stockholm University) and the FEAST JWST team

Just below Orion’s belt lies one of the most celebrated objects in the night sky: the Orion Nebula, a stellar nursery that is home to about 700 young stars.

This Webb image focuses not on the entirety of the nebula but on a structure in the lower left-hand quadrant known as the Orion Bar.

So named because of its diagonal, ridge-like appearance, the bar is shaped by the powerful radiation of the hot, young stars surrounding it.

ESA/Webb, NASA, CSA, M. Zamani (ESA/Webb), and the PDRs4All ERS Team

A baby by stellar standards, the IC 348 Star cluster is just five million years old and located about 1,000 light years from Earth.

Composed of an estimated 700 stars, IC 348 has a structure similar to wispy curtains, created by dust that reflects the light of the stars.

The conspicuous loop in the right hand side of the image is likely created by the gusting of solar winds blowing in the direction that, from Earth, would be west to east.

NASA, ESA, CSA, STScI, Kevin Luhman (PSU), Catarina Alves de Oliveira (ESA)

When it comes to galaxies, there's big and then there's huge and by any measure, Pandora's Cluster — more formally, known as Abell 2744 — qualifies as the latter.

Not just a galaxy, and not even a cluster of galaxies, Abell 2744 is a cluster of four clusters, which long ago collided with one another.

Located 3.5 billion light years from Earth, Pandora's Cluster measures a staggering 350 million years across.

The cluster's massive collective gravity allows astronomers to use it as a gravitational lens, bending and magnifying the light of foreground objects, making them easier to study.

NASA, ESA, CSA, I. Labbe (Swinburne University of Technology) and R. Bezanson (University of Pittsburgh). Image processing: Alyssa Pagan (STScI)

Webb was built principally to look at the oldest and most distant objects in the universe, some of 13.4 billion light years away.

But doesn't prevent the telescope from peering into its own back yard.

This image of Saturn and some of its 146 moons, rivals the images obtained by the Pioneer and Voyager probes.

NASA, ESA, CSA, STScI, Matt Tiscareno (SETI Institute), Matt Hedman (University of Idaho), Maryame El Moutamid (Cornell University), Mark Showalter (SETI Institute), Leigh Fletcher (University of Leicester), Heidi Hammel (AURA). Image processing: J. DePasquale (STScI)

Infant stars are born all over the universe, but the closest stellar birthing suite to Earth is the Rho Ophiuchi cloud complex, located just 460 light years distant.

A turbulent — even violent — place, Rho Ophiuchi is defined by jets of gas roaring from young stars.

Most of the stars in this comparatively modest nursery are more or less the size of the sun.

But one, known as S1, is far bigger — so much so that it is self-immolating, carving a great cavity around itself with its stellar wind, the storm of charged particle's all stars emit, though few with the gale-force power of S1.

NASA, ESA, CSA, STScI, Klaus Pontoppidan (STScI)

[mutant-distraction]

The Ring Nebula captured by Webb’s near-infrared camera (NIRCam). ESA/Webb, NASA, CSA, M. Barlow (University College London), N. Cox (ACRI-ST), R. Wesson (Cardiff University)

[askdreemurkids]

Ranunculus bulbosus, commonly known as bulbous buttercup or St. Anthony's turnip,[1] is a perennial flowering plant in the buttercup family Ranunculaceae. It has bright yellow flowers, and deeply divided, three-lobed long-petioled basal leaves.

The stems are 20–40 cm tall, erect, branching, and slightly hairy, with a swollen corm-like base.[2]: 120 [3] There are alternate and sessile leaves on the stem. The flower forms at the apex of the stems, with 5–7 petals,[3] the sepals strongly reflexed.[2] The flowers are glossy yellow and 1.5–3 cm wide. The plant blooms from April to July.

The native range of Ranunculus bulbosus is Western Europe between about 60°N and the Northern Mediterranean coast. It grows in both the eastern and western parts of North America as an introduced weed.[4] Bulbous buttercup grows in lawns, pastures and fields in general, preferring nutrient-poor, well-drained soils. Although it doesn't generally grow in proper crops or improved grassland, it is often found in hay fields[5] and in coastal grassland.

The bulbous buttercup gets its name from its distinctive perennating organ, a bulb-like swollen underground stem or corm, which is situated just below the soil surface. After the plant dies in heat of summer, the corm survives underground through the winter.[6][7] Although the presence of a corm distinguishes Ranunculus bulbosus from some other species of buttercup such as Ranunculus acris, the species also has distinctive reflexed sepals.

Other names for the bulbous buttercup are "Goldcup" because of the colour and shape of the leaves, and "Frogs-foot" from their form.[8]

This plant, like other buttercups, contains the toxic glycoside ranunculin, which gives it a bitter, acid taste, so cases of poisoning in humans are rare.[9] It is also avoided by livestock when fresh, but when the plant dries the toxin is lost, so hay containing the plant is safe for animal consumption.[3] Pigs are unaffected by the toxin and eat bulbous buttercups avidly, being prepared to travel long distances to find them;[10] hence the folk name of the plant, St Antony's Turnip, after the patron saint of swineherds.

[visualpoett]

JWST’s mid-infrared view of the Ring Nebula.ESA/WEBB, NASA, CSA, M. BARLOW (UNIVERSITY COLLEGE LONDON), N. COX (ACRI-ST), R. WESSON (CARDIFF UNIVERSITY)

[skycrorg]

James Webb capturó impresionantes imágenes de la nebulosa del Anillo

El Telescopio Espacial James Webb (JWST) de la NASA ha registrado nuevas imágenes impresionantes de la icónica Nebulosa del Anillo, también conocida como Messier 57. Las imágenes, publicadas hoy por un equipo internacional de astrónomos dirigido por el profesor Mike Barlow (UCL, Reino Unido) y el Dr. Nick Cox (ACRI-ST, Francia), con el profesor Albert Zijlstra de la Universidad de Manchester,…

[zehub]

Méduses : vous devriez consulter cette carte avant de partir à la plage

Comment savoir si des méduses sont présentes sur votre plage avant de vous déplacer ? Le laboratoire ACRI-ST, spécialisé dans l'étude de la Terre grâce aux outils satellites, a lancé un

[mwapatecapsulehire]

Mwapate Capsule Hire Oakleigh

Professional and accredited baby capsule hire, Holiday hire for baby car seats, with safe and trusted Baby seat installation along Bayside Melbourne, south East Suburbs and Select Eastern Suburbs. We are ACRI accredited updated with Kidsafe training. Established in 2012 and trusted by local councils and family day car centres across Melbourne

Website: https://babycarseathire.com

Address: 6 Elizabeth St, Oakleigh East, VIC, 3166

Phone Number: 0479 168 579

Business Hours: Mon - Fri : 09:00 am - 05:00 pm

[astroblogs]

[eurovisionsocialnewswire]

SPACE: Manchester astronomer captures stunning images of the Ring Nebula [PHOTOS]

NASA’s James Webb Space Telescope (JWST) has recorded breath-taking new images of the iconic Ring Nebula, also known as Messier 57. The images, released today by an international team of astronomers led by Professor Mike Barlow (UCL, UK) and Dr Nick Cox (ACRI-ST, France), with Professor Albert Zijlstra of The University of Manchester, showcase the nebula’s intricate and ethereal beauty in…

[tinyshe]

‘We crush the head of the serpent when we scorn and trample underfoot the glory of the world, the praises the vanities, and all the other pomps of pride.’

Bl. Marie of The Incarnation

Also known as Madame Barbe Acrie.         1566 – 1618

She was born Barbe Avrillot on February 1st 1566 and baptised the next day.  Her father, Nicholas Avrillot, was accountant general in the Chamber of Paris and chancellor to Queen Margaret of Valois.  Her mother, Marie Lhuillier was also from the upper class of Parisian society.   Barbe was educated by the Franciscan nuns of Longchamp.  The girls were taught to read and to sing and they joined in most of the Divine Office with the nuns.  Barbe always felt drawn to religious life but in obedience to her parents’ wishes she married Pierre Acarie in 1582.  He was a rich young man from Parisian high society but he was also a committed Catholic.  They had six children and Barbe proved to be an excellent wife and mother.

After the birth of her second child Barbe read some words of St. Augustine which made a great impression on her, ‘He is indeed a miser to whom God is not enough’.  It was after this that she began to have mystical experiences, which worried her a great deal at first, but gradually she gained more control and could be resting in God at the same time as she was involved with her family or her other works.

Barbe’s husband Pierre Acarie became an active member of the Catholic League which opposed the Huguenots and although he never joined in the violent activities of some of the members, when Henri IV took possession of Paris, he, like many others in the League, was ordered to leave the city.  However, he was able to choose his place of residence and went to the charterhouse in Bourgfontaine.   Unfortunately his zeal for his faith had outstripped his prudence and he had recklessly lent money to other members of the League.  As Pierre was 45 miles from Paris, Barbe found herself faced with sudden debts and had to hand over most of her possessions to pay them off.  She sent her four eldest children away to school and the two youngest to stay with relatives while she went to stay with her cousin Mme Bérulle mother of the future cardinal, who was then a student at the Sorbonne.He was nine years younger than Barbe and although they already knew each other they grew closer and found mutual support and encouragement, as each became more completely dedicated in their spiritual paths.

Barbe never criticised her husband for his reckless ways and her love for him never faltered in spite of all the hardship he had caused her. She travelled the 45 miles to  Bourgfontaine to see him.  While there he was captured by bandits and she raised the ransom to free him and also arranged his transfer to the Chateau at Luzarches, which was much closer to Paris.  There she was able to see him far more frequently until on returning from one of these visits her horse stumbled and left her with a broken hip. The next year she fell on a step and fractured her thigh, and a third fall of a similar nature followed soon afterwards. These accidents caused her to remain lame for the rest of her life.  Meanwhile, after many legal struggles she had sorted out Pierre’s affairs and soon afterwards the family was reunited in their old home.

Barbe became known all over Paris for her great charity to the sick and poor. Her works were many and varied, among other things she opened a refuge for prostitutes who wanted to make a new start in life and she made vestments for missionaries.

By the beginning of the seventeenth century the Acarie home was a gathering place for clergy and devout laity alike.  Many came to ask Barbe’s advice.  She always accommodated clergy who wanted to stay for convalescence after an illness. Her cousin, Cardinal Pierre Bérulle, was a frequent visitor, others included St. Francis de Sales, who was Barbe’s spiritual director for a short time, and St. Vincent de Paul. High society ladies, including Mme. Jourdain, Mme de Bréauté and others who later became Carmelites, were also visitors to the Acarie household.

In 1601 Abbé de Brétigny’s translation of Ribera’s life of St. Teresa was published.  After Barbe had begun reading this St. Tesesa appeared to her and told her that God had chosen her to found Carmels in France.   Barbe consulted with her friends and advisers but they felt that the time was not right and advised her to abandon the idea or at least leave it aside for a time.  She tried to do that but eight months later St. Teresa appeared to her again and assured her that the difficulties would be overcome. Barbe approached the Duchess of Longueville asking her to be the foundress which in fact meant financing the project and also getting the necessary letters patent from the king.  She eventually succeeded in this and Barbe persuaded her friends and advisers to support her.  St. Francis de Sales wrote to Pope Clement VIII to obtain his permission to found monasteries of Discalced Carmelite nuns in France under the jurisdiction of secular clergy as there were no Carmelite Friars in France at that time.  They all considered it essential to bring nuns from Spain who had known St. Teresa, so that the French Carmels would be authentically Teresian.   Gradually the difficulties were overcome as St. Teresa had predicted.   The Pope sent authorisation for the new monastery which was built  in Paris and Barbe gathered a group of future postulants together. Abbé de Brétigny travelled to Spain to bring back Spanish Carmelites who had known St. Teresa, but he was initially refused, so he called on Barbe for advice, she sent her cousin, Pierre de Bérulle to help him and together with some ladies of the nobility they returned with six of Teresa’s best nuns including Anne of St. Bartholomew and Anne of Jesus.  Two Spanish Carmelite friars accompanied them and gave the habit to the first French novices. The Spanish nuns all went to the newly built Paris Carmel in 1604 but more foundations followed and Barbe was much involved in those at  Pontoise in1605, Dijon in 1605 and Amiens in1606. By the time of her death 12 years later there were fourteen Carmels in France.  Barbe’s three daughters all became Carmelites. Among the young women Barbe had gathered together to train as future Carmelites she found that some  clearly did not have a Carmelite vocation, yet they were dedicated women sincerely seeking to serve God.  It occurred to Barbe that they would make excellent teaching sisters, so she set about founding the Ursulines in Paris convinced that if girls were taught their faith well they could reform morality in the country, as most of these girls would go on to be mothers and would pass on the teaching to their children.

Very soon after her husband, Pierre Acarie, died in 1613,  Barbe settled her affairs and asked to enter Carmel as a lay sister, she wanted to go to the poorest monastery and entered at Amiens where her eldest daughter was sub-prioress.  She took the name Sr. Mary of the Incarnation and made her solemn profession on April 8th  1615, but her health had deteriorated a great deal.  She only lived five years after Pierre’s death.  Barbe was sent to the Carmel at Pontoise,  as the superiors thought it might be beneficial for her health, but she died there on the Wednesday of Easter week, April 18th 1618. Sister Mary of the Incarnation was beatified on June 5th 1791. Her Feast Day is kept on April 18th  in Paris and in the Carmelite order.

text source

[sciencespies]

Observing phytoplankton via satellite

https://sciencespies.com/nature/observing-phytoplankton-via-satellite/

Observing phytoplankton via satellite

Thanks to a new algorithm, researchers at the AWI can now use satellite data to determine in which parts of the ocean certain types of phytoplankton are dominant. In addition, they can identify toxic algal blooms and assess the effects of global warming on marine plankton, allowing them to draw conclusions regarding water quality and the ramifications for the fishing industry.

The tiny phytoplankton found in the world’s oceans are tremendously productive, and create half the oxygen we need to breathe. Just like land-based plants, they use photosynthesis to produce carbohydrate, which they use as an energy source. They grow, divide and produce enormous quantities of biomass, the basis of all marine life. In addition, they are an essential food source for small crustaceans, fish and mussel larvae, which are themselves staples for larger fish. When phytoplankton are in short supply, it jeopardises the food web for all other marine organisms.

There are various groups of phytoplankton around the globe, and they fulfil different functions in marine ecosystems. Some are favourite food sources; others form specific chemical compounds or serve as nutrient fixers in the water, which can have a major influence on marine flora and fauna. On the other hand, certain groups of phytoplankton can grow to dense masses and produce toxic substances; when there are too many of them in the water, it can be lethal for some marine organisms, especially fish. Marine phytoplankton are also extremely important in their role as a CO2 sink. Accordingly, researchers are keen to learn how the populations of the respective phytoplankton groups are developing around the world.

More than chlorophyll

However, until recently it was virtually impossible to estimate these populations in detail. Granted, researchers have been collecting water samples from on board research vessels for decades, in order to identify and quantify the plankton present. But these are only random samplings. And even satellites, which have been scanning the oceans with their sensors for the past three decades, were an imperfect solution at best: though they could certainly be used to gauge the amount of the plant pigment chlorophyll in the water — as an indicator of how high the general concentration of phytoplankton was — distinguishing between the different types of phytoplankton remained extremely difficult. Moreover, there was no way to use satellite data to predict algal growth in specific regions.

But now an international team led by Hongyan Xi and Astrid Bracher from the Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research (AWI) have for the first time managed to glean far more from satellite data: as they report in the journal Remote Sensing of Environment, working in close cooperation with the French company ACRI-ST and with the support of the European-based satellite data provider Copernicus Marine Environment Monitoring Service, they have developed a new algorithm that can be used to distil the data into key information on five main phytoplankton groups.

Reflectance as a key parameter

Satellite sensors register light at various wavelengths; normally, those wavelengths are used which are capable of picking up the colour of the chlorophyll. But Hongyan Xi and her colleagues have found a way to put this wavelength information to better use. More specifically, this involves analysing an aspect known as reflectance (or coefficient of reflection), which represents the amount of sunlight striking the Earth that is reflected back into space. This reflection is due to numerous optical processes: the light is scattered, bent and altered by water molecules and particles in the ocean and atmosphere alike. “And the plankton, which itself contains certain pigments, has an influence on the reflectance,” Hongyan Xi explains. “The reflectance can differ, depending on which types of plankton and which pigments are dominant in the water.” In fact, each of the five types leaves its own fingerprint on the reflected light — and the new algorithm can recognise them all.

Painstaking comparisons of ship-based and satellite data

This breakthrough was only possible thanks to a tremendous amount of hard work. First the team had to determine which reflectance pattern was characteristic of each plankton type. They then had to compare the satellite readings with plankton samples collected at the same time and place from on board research vessels. Fortunately, the findings of many ship-based expeditions are now available in publicly accessible databases. Thanks to these archives, the experts were able to determine where and when the water samples had been collected, and which species and types of plankton were present. Xi and her colleagues analysed ca. 12,000 of these datasets — and then mapped each and every one to satellite scans taken of the same place at the same time. Doing so allowed them to deduce how the reflectance changed in certain plankton types.

Water quality and toxic algal blooms

Armed with these findings, they were then ready to develop the algorithm. Today, it can be used to determine which types of phytoplankton are dominant in any given marine region worldwide, based on its reflectance information. This is important e.g. to identify toxic “harmful algal blooms” (HABs). The presence of certain types of phytoplankton is also an indicator of water quality; information that is particularly relevant for the fishing industry. According to Hongyan Xi: “In addition, in the future we’ll be able to determine whether or not the distribution of phytoplankton is affected by climate change — an important aspect in terms of predicting the impacts on ecosystems.”

#Nature

[spaceexp]

Sentinel-3 flies tandem

ESA - Sentinel-3 Mission logo. 19 June 2018 The key to monitoring Earth’s changing environment and to guaranteeing a consistent stream of satellite data to improve our daily lives is to take the same measurements over the course of decades. But how do you know that measurements from successive satellites, even though identical in build, are like for like? The answer, for the Copernicus Sentinel-3 mission, is to engage in some nifty orbital flying.

Tandem in images

Sentinel-3 is a two-satellite mission to supply the coverage and data delivery needed for Europe’s Copernicus environmental monitoring programme. Launched in 2016, Sentinel-3A has been measuring our oceans, land, ice and atmosphere to monitor and understand large-scale global dynamics and to provide critical information for marine operations, and more. Its twin, Sentinel-3B, was launched in April 2018 and is having its instruments calibrated and being commissioned for service. Once Sentinel-3B is operational, the two satellites will orbit Earth 140° apart.

Sentinel-3 spacecraft

Now, however, the satellites have been positioned much closer together, flying a mere 30 seconds apart. Travelling at 7.4 km per second, the separation equates to a distance of 223 km. The reason for this is to see how their instruments compare. Even though the two Sentinel-3 satellites are identical, each carrying a radar altimeter, a radiometer and an imaging spectrometer, there’s a chance that their instruments could behave slightly differently. It is important that any differences are carefully accounted for otherwise the information they deliver could be misinterpreted as changes happening on Earth’s surface. Given the satellites’ current brief separation, their measurements should be virtually the same.

Sentinel-3 going tandem

This tandem phase is also important for the future Sentinel-3 satellites. ESA’s ocean scientist, Craig Donlon, explains, “Our Sentinel-3 ocean climate record will eventually be derived from four satellites because we will be launching two further Sentinel-3s in the future. “We need to understand the small differences between each successive satellite instrument as these influence our ability to determine accurate climate trends. “The four-month Sentinel-3 tandem phase is a fantastic opportunity to do this and will provide results so that climate scientists can use all Sentinel-3 data with confidence.” ESA’s Sentinel-3 project manager, Bruno Berruti, said, “Following liftoff and the usual checks, the operations team has been expertly flying Sentinel-3B so that it gradually flies closer to Sentinel-3A.

Sentinel-3 comparison

“We recently reached the magic separation of 30 seconds and I am happy to say that we are now officially in the tandem phase. “This will last around four months, after which the two satellites will be gently moved apart until they reach their operational separation of 140°. This is different to the other Sentinel missions, but for our mission it is better to measure ocean features such as eddies as accurately as possible.” ESA’s Sentinel-3 mission manager, Susanne Mecklenburg, added, “So far, we are really happy with the results of the tandem phase. Measurements from the satellites’ instrument packages seem to be very much aligned, but we will be analysing the results very carefully over the next months to make sure we account for any minor differences.” Related links: Sentinel-3: http://www.esa.int/Our_Activities/Observing_the_Earth/Copernicus/Sentinel-3 Sentinel data access: https://scihub.copernicus.eu/ Images, Text, Credits: ESA/contains modified Copernicus Sentinel data (2018), processed by ESA/S3MPC/ACRI-ST/ESA, CC BY-SA 3.0 IGO. Best regards, Orbiter.ch Full article

[julie1971]

Acco, Ptolemais, Acre Also known as Tel 'Akko/Acco, Tel/Tell el-Fukhkhar, Tell el-Fukhar, Acca, Accho, Acon, Acre, Acri, Ake, 'Akka, Akko, Antiochenes, Antiochia Ptolemais, Ptolemais Antiochenes, Ocina, St. Jean d'Acre

Acco, Ptolemais, Acre Also known as Tel ‘Akko/Acco, Tel/Tell el-Fukhkhar, Tell el-Fukhar, Acca, Accho, Acon, Acre, Acri, Ake, ‘Akka, Akko, Antiochenes, Antiochia Ptolemais, Ptolemais Antiochenes, Ocina, St. Jean d’Acre

Port City of Acco Acco is only referenced once in the Bible by this name. In Judges 1:31, it is referred to as one of the places the Israelites failed to hold. In the New Testament, Acco was known as Ptolemais and was one of the stops on Paul’s final return to Jerusalem (Acts 21:7). Ptolemais was situated on the main sea and land route in ancient times. It served as the main port of the region…