It Looks Like the Flu, But Isn’t: What Is Adenovirus?

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It Looks Like the Flu, But Isn’t: What Is Adenovirus?

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It Looks Like the Flu, But Isn't: What Is Adenovirus?

This picture of an adenovirus was taken using a transmission electron microscope (TEM). It has been artifically colorized.

Credit: CDC

The flu isn’t the only virus that could leave you feeling feverish and generally miserable this winter — another virus, called adenovirus, can cause similar symptoms, although doctors don’t routinely test for it.

Adenoviruses are prolific viruses that can cause a variety of illnesses, including upper respiratory infections — such as colds — as well as pneumonia, gastrointestinal illness, conjunctivitis (pink eye) and even urinary tract infections, said Dr. Amesh Adalja, a senior scholar at the Johns Hopkins Center for Health Security. (There are 52 strains of adenovirus, and different strains cause different illnesses.)

When a person has a respiratory infection caused by an adenovirus, “it would be really hard to tell it apart from influenza” just by looking at the patient, Adalja said. Symptoms can include fever, sore throat, cough and runny nose, according to the Centers for Disease Control and Prevention (CDC). [The 9 Deadliest Viruses on Earth]

However, unlike the flu, adenovirus doesn’t have a “striking seasonality,” Adalja told Live Science. Although outbreaks of adenovirus infections are most common in the late winter, spring and early summer, they can occur year-round, the CDC said.

In some cases, adenoviruses can cause severe respiratory symptoms, including pneumonia, particularly in patients whose immune systems are compromised, Adalja said. In 2007, an outbreak of adenovirus sickened about 140 people in four states, killing 10 patients, according to the CDC. But that fatality rate doesn’t compare to that of the flu, which can cause between 12,000 and 56,000 deaths per year, according to the CDC.

Outbreaks of adenovirus in the military led the U.S. Department of Defense to begin vaccinating military recruits against two strains of the virus in 1971, according to Medscape. When vaccine production stopped in 1996, cases of adenovirus in the military increased, as the disease spreads easily in close quarters. This re-emergence of the disease led to the reintroduction of the vaccine among recruits in 2011, Medscape reported. It’s estimated that the vaccine prevents about 15,000 cases of adenovirus infections in U.S. military recruits, according to the U.S. Army Medical Material Development Activity.

A recent study, published in the journal Emerging Infectious Diseases, looked at adenovirus respiratory infections in nonmilitary members and concluded that the vaccine should also be considered for susceptible groups outside the military, such as those living in long-term-care facilities or college dorms.

Adalja agreed that “because [adenovirus] does cause a considerable burden of illness, we want to explore” the ability to use the vaccine outside of the military context.

For example, the vaccine may benefit people at high risk of contracting the virus, such as patients with lung disease and others with compromised immune systems, but it may even benefit the general population, Adalja said. However, future studies would be needed to examine which segments of the population would benefit most, and whether vaccination would be cost-effective, he said.

Original article on Live Science.

Nobody Knows Why These Bees Built a Spiral Nest

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Nobody Knows Why These Bees Built a Spiral Nest

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Nobody Knows Why These Bees Built a Spiral Nest

Top-down view of an Australian stingless bee colony’s brood comb.

Credit: Tim Heard

The Australian stingless bee Tetragonula carbonaria is not your average pollinator. For starters, out of about 20,000 known bee species in the world, T. carbonaria is one of only 500 without stingers.

That’s not to say this bee is defenseless. Invasive beetles that have tried to infiltrate T. carbonaria nests have found themselves suddenly covered in a brew of wax, mud and plant resin — effectively mummified alive by bees.T. carbonaria colonies have also been observed waging days-long territory wars against their stingless neighbors, resulting in hundreds of bee-on-bee casualties and queens unceremoniously dethroned.

This is all to say, if you had a home like T. carbonaria‘s, you’d probably fight for it, too. As seen in a popular photo posted to Reddit last week, swarms of T. carbonaria rear their young in mesmerizing, spiral-shaped towers called brood combs, linking hundreds of individual egg chambers together into a continuous staircase of unborn baby bees. [Here’s What Wasp Faces Look Like Up-Close]

“The image is just one layer of the brood comb,” entomologist Tim Heard, who took the photo while researching stingless bees for The Commonwealth Scientific and Industrial Research Organisation (CSIRO) in Australia, said in an email.”A fully developed nest consists of 10-20 layers. Each layer is one circle of a continuous spiral.”

The little circular pods you see forming this spiral are called brood cells. Within these cells, individual bees grow from egg to adulthood in the span of about 50 days, Heard wrote in his stingless bee-keeping manual, “The Australian Native Bee Book” (Sugarbag Bees, 2015). To build these cells, worker bees secrete wax from their abdominal glands and mix it with a plant resin derivative, making a sturdy construction material calledcerumen.

“A cell is [then] mass provisioned by nurse workers regurgitating food to about two-thirds of the capacity of the cell, which is sufficient to feed the larva for its entire development to a pupa,” Heard wrote. “The queen lays an egg on the provisions. The cell is then immediately capped so that the larva can develop in a closed cell.”

When one cell is completed, workers move onto another, building new cells outward and upward in a spiral pattern, Heard wrote. Eventually, adult bees start emerging from the oldest cells built in the center of the lowest level of the brood comb, leaving behind a steadily growing cavity of empty husks known as the retreating edge. (You can identify the newly hatched bees in the photo by their silvery sheen — their skin will darken to its mature color a few days after the bees leave their cells.)

As this cavity of empty cells grows from the bottom up, workers begin building a brand new brood inside it, continuing the cycle. A single colony could potentially live indefinitely in this fashion, Heard and his colleaguestheorized, so long as it had a queen to lay new eggs.

So, why the spiral shape? Researchers have tried (and sort of failed) to explain the bee’s construction guidelines as an algorithm that every worker bee innately knows. But Heard, for one, would as soon leave it to mystery.

“It may be unwise to attempt to explain the adaptive significance of why this form may have evolved,” Heard told Live Science. “Perhaps, it is just the outcome of some random behavior or perhaps it is adaptive. A possible adaptive advantage of this form is that it is efficient use of space and also facilitates the circulation of air between the layers. But then one has to ask, why it is not more common.”

Originally published on Live Science.

The Phases of the Super Blue Blood Moon of 2018 Explained

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The Phases of the Super Blue Blood Moon of 2018 Explained

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No enthusiastic skywatcher ever misses a total eclipse of the moon. The spectacle of the lunar disk slipping into Earth’s shadow and turning a deep shade of red is often more striking and engaging than one might think. What’s more, when the moon is entering into and later emerging out of Earth’s shadow, secondary phenomena may be overlooked, but these additional features of the eclipse are worth looking out for.A total lunar eclipse occurs when the moon is completely submerged in Earth’s dark, inner shadow, called the umbra. If the moon is only partly covered by the umbra, or only enters the outer shadow (called the penumbra), it is considered a partial lunar eclipse. The total eclipse is said to “begin” when the moon is fully covered by the umbra; this phase is also called “totality.” [Super Blue Blood Moon 2018: When, Where and How to See It]

Stages of the Jan. 31, 2018 "super blue blood moon" are depicted in Pacific Time with "moonset" times for major cities across the U.S., which affect how much of the event viewers will see. While viewers along the East Coast will see only the initial stages of the eclipse before moonset, those in the West and Hawaii will see most or all of the lunar eclipse phases before dawn.

Stages of the Jan. 31, 2018 “super blue blood moon” are depicted in Pacific Time with “moonset” times for major cities across the U.S., which affect how much of the event viewers will see. While viewers along the East Coast will see only the initial stages of the eclipse before moonset, those in the West and Hawaii will see most or all of the lunar eclipse phases before dawn.

Credit: NASA

To help prepare for the upcoming eclipse Wednesday morning (Jan. 31), which NASA has dubbed a “Super Blue Blood Moon” eclipse due to its occurance near perigee and during the second full moon of January, has prepared a step-by-step chronology of the eclipses’ major phases and some of the secondary phenomena you might expect to see. Not all of the events mentioned in the chronology will necessarily occur, because no two eclipses are the same. But many will, and those who know what to look for have a better chance of seeing them!

1 5:51 4:51 3:51 2:51 1:51 12:51
2 6:31 5:31 4:31 2:31 1:31 1:31
3 6:48 5:48 4:48 3:48 2:48 1:48
4 6:35 5:35 4:35 3:35 2:35
5 6:46 5:46 4:46 3:46 2:46
6 6:51 5:51 4:51 3:51 2:51
7 6:29 5:29 4:29 3:29
8 7:07 6:07 5:05 4:05
9 6:23 5:23 4:23
10 7:11 6:11 5:11
11 6:28 5:28
12 7:08 6:08

In the above timetable, all times are for a.m. on Jan. 31. When dashes are provided, it means that the moon has set and is no longer visible. Below are the numbered stages listed above, fully described:

1. Moon enters Earth’s penumbra: The shadow cone of the Earth has two parts: a dark, inner umbra, surrounding by a lighter penumbra. The penumbra is the pale outer portion of Earth’s shadow. Although the eclipse begins officially when the moon enters the penumbra, this is, in essence, an academic event. You won’t see anything unusual happening to the moon — at least not just yet. The Earth’s penumbral shadow is so faint that it remains invisible until the moon is deeply immersed in it. We must wait until the penumbra has reached about 70 percent across the moon’s disk. So for about 40 minutes after the “start” of the partial eclipse, the full moon will continue to appear to shine normally, although with each passing minute it is progressing ever deeper into Earth’s outer shadow.

2. Penumbral shadow begins to appear: Now the moon has progressed far enough into the penumbra that the shadow should be evident on the moon’s disk. Start looking for a very subtle, light shading to appear on the moon’s left portion. This will become increasingly evident as the minutes pass, with the shading appearing to spread and deepen. Just before the moon begins to enter Earth’s dark umbral shadow, the penumbra should appear as an obvious smudge or tarnishing of the moon’s left portion.

Areas of the world that will see the Jan. 31, 2018, total lunar eclipse. The eclipse will be visible Jan. 31 in the morning before sunrise for North America, Alaska and Hawaii. Observers in the Middle East, Asia, eastern Russia, Australia and New Zealand will see it during moonrise the evening of Jan. 31.

Areas of the world that will see the Jan. 31, 2018, total lunar eclipse. The eclipse will be visible Jan. 31 in the morning before sunrise for North America, Alaska and Hawaii. Observers in the Middle East, Asia, eastern Russia, Australia and New Zealand will see it during moonrise the evening of Jan. 31.

Credit: NASA


3. Moon enters Earth’s umbra: The moon now begins to cross into the Earth’s dark central shadow, called the umbra. A small dark scallop begins to appear on the moon’s left-hand (eastern) limb, or it’s apparent edge. The partial phases of the eclipse begin; the pace quickens and the change is dramatic. The umbra is much darker than the penumbra and fairly sharp-edged. As the minutes pass, the dark shadow appears to slowly creep across the moon’s face. At first the moon’s limb may seem to vanish inside of the umbra, but much later, as it moves in deeper you’ll probably notice it glowing dimly orange, red or brown. Notice also that the edge of the Earth’s shadow projected on the moon is curved. Here is visible evidence that the Earth is a sphere, as deduced by Aristotle from lunar eclipses he observed in the fourth century B.C. Almost as if a dimmer switch was slowly being turned down, the surrounding landscape and deep shadows of a brilliant moonlit night begin to fade away.

4. 75 percent coverage: With three-quarters of the moon’s disk now eclipsed by the umbra, the part of it that is immersed in shadow should begin to very faintly light up— like a piece of iron heated to the point where it just begins to glow. It now becomes obvious that the umbral shadow does not create complete darkness on the lunar surface. Using binoculars or a telescope, the shadow’s outer part is usually light enough to reveal lunar maria and craters, but the central part is much darker, and sometimes no surface features are recognizable. Colors in the umbra vary greatly from one eclipse to the next, reds and grays usually predominate, but sometimes browns, blues and other tints are encountered.

5. Less than 5 minutes to totality: Several minutes before (and after) totality, the contrast between the remaining pale-yellow sliver of the moon’s surface and the ruddy-brown coloration spread over the rest of the disk may produce a beautiful phenomenon known to some as the “Japanese Lantern Effect.”

The moon during totality. The color of the moon in this phase varies from eclipse to eclipse.

The moon during totality. The color of the moon in this phase varies from eclipse to eclipse.

Credit: NASA

6. Total eclipse begins: When the last of the moon enters the umbra, the total eclipse begins. How the moon will appear during totality is not known. Sometimes the fully eclipsed moon is such a dark gray-black that it nearly vanishes from view. But it can also glow a bright orange. The reason the moon can be seen at all when totally eclipsed is that sunlight is scattered and refracted around the edge of Earth by our atmosphere. To an astronaut standing on the moon during totality, the sun would be hidden behind a dark Earth outlined by a brilliant red ring consisting of all the world’s sunrises and sunsets. The brightness of this ring around Earth depends on global weather conditions and the amount of dust suspended in the air. A clear atmosphere on Earth means a bright lunar eclipse. If a major volcanic eruption has injected particles into the stratosphere during the previous couple of years, the eclipse is very dark.

7. Middle of totality: The moon is now shining anywhere from 10,000 to 100,000 times fainter than it was just a couple of hours ago. Since the moon is moving to the south of the center of Earth’s umbra, the gradation of color and brightness across the moon’s disk should be such that its upper portion should appear darkest, with hues of deep copper or chocolate brown. Meanwhile, its lower portion — that part of the moon closest to the outer edge of the umbra — should appear brightest, with hues of reds, oranges and even perhaps a soft bluish-white.

Observers away from bright city lights will notice a much greater number of stars than were visible before the eclipse began. The moon will be in the dim constellation of Cancer, the Crab, and positioned almost midway between the backward question-mark pattern of stars known as the Sickle of Leo well to its east (upper left) and the “twin stars,” Pollux and Castor of Gemini well to the west (the moon’s lower right). The darkness of the sky is impressive. The surrounding landscape has taken on a somber hue. Before the eclipse, the full moon looked flat and one-dimensional. During totality, however, it will look smaller and three-dimensional — like some weirdly illuminated ball suspended in space.

Before the moon entered Earth’s shadow, the temperature on its sunlit surface hovered at about 266 degrees Fahrenheit (130 degrees Celsius). Since the moon lacks an atmosphere, there is no way this heat could be prevented from escaping into space as the shadow sweeps by. Now, in shadow, the temperature on the moon has dropped to minus 146 degrees F (minus 99 C); a drop of 412 degrees F, or 229 degrees C, in less than 150 minutes!

8. Total eclipse ends: The emergence of the moon from the umbral shadow begins. The first small segment of the moon begins to reappear, followed again for the next several minutes by the Japanese Lantern Effect.

9. 75 percent coverage: Any vestiges of coloration within the umbra should be disappearing now. From here on, as the dark shadow methodically creeps off the moon’s disk, it should appear black and featureless.

10. Moon leaves umbra: The dark central shadow clears the moon’s right-hand (western) limb.

11. Penumbra shadow fades away: As the last, faint shading vanishes off the moon’s right portion, the visual signs of the eclipse come to an end.

12. Moon leaves penumbra: The eclipse “officially” ends, as it is completely free of the penumbral shadow.

Editor’s note: If you capture an amazing photo of video of the Jan. 31 total lunar eclipse and would like to share it with for a story or gallery, send images and comments to:

Joe Rao serves as an instructor and guest lecturer at New York’s Hayden Planetarium. He writes about astronomy for Natural History magazine, the Farmers’ Almanac and other publications, and he is also an on-camera meteorologist for Verizon Fios1 News, based in Rye Brook, N.Y. Follow us@Spacedotcom, Facebook and Google+. Original article on

Image of the Day

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Image of the Day

Twilight Haze on Titan

Credit: NASA/JPL-Caltech/Space Science Institute

Why Wednesday’s Super Blue Blood Moon Eclipse Is So Special

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Why Wednesday’s Super Blue Blood Moon Eclipse Is So Special

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Why Wednesday's Super Blue Blood Moon Eclipse Is So Special

People who peer up at the night sky this Wednesday (Jan. 31) may see something like this illustration, which shows a blood moon during a total lunar eclipse.

Credit: NASA

Imagine going to a drive-thru and ordering the following: a blue moon, a supermoon, a blood moon and a total lunar eclipse. Although such a request is impossible (if only!), all four events are actually happening tomorrow (Jan. 31).

But what, exactly, are these four celestial treats? And how rare is it that skywatchers can view all of them on the same night?

For starters, it’s extremely rare. A super-blue-blood-moon-and-total-lunar-eclipse combo hasn’t happened in more than 150 years, Live Science previously reported. [Super Blue Blood Moon 2018: When, Where and How to See It]

Even separately, these events are rare. For instance, a blue moon happens when two full moons occur within the same calendar month. Normally, Earth has 12 full moons per year, which equates to one per month. But because the lunar month — the time between two new moons — averages 29.530589 days, which is shorter than most months (with the exception of February), some years have 13 full moons, Live Science previously reported.

Blue moons happen once every 2.7 years, which explains why the last one happened on July 31, 2015. But despite their name, blue moons don’t actually appear blue. A bluish tint is only possible when smoke or ash from a large fire or volcanic eruption gets into the atmosphere. These fine particles can scatter blue light and make the moon appear blue.

Supermoons, however, are more common than blue moons. A supermoon happens when a full moon is at or near perigee, the point in the moon’s monthly orbit when it’s closest to Earth. Because they’re marginally closer to Earth, supermoons can appear up to 14 percent larger and up to 30 percent brighter than regular full moons, Live Science previously reported.

The most recent supermoon happened this past New Year’s Day, on Jan. 1, 2018. Because the upcoming full moon will be January’s second full moon, it has earned the title of “blue moon.”

Finally, the last two events — the total lunar eclipse and the blood moon — are linked. A total lunar eclipse can happen only when the sun, Earth and full moon are perfectly lined up, in that order. With this alignment, the full moon is completely covered in Earth’s shadow.

A composite image showing the total lunar eclipse that happened during a supermoon on Sept. 27, 2015, as seen from Denver. Before 2015, the last supermoon-and-total-lunar-eclipse combo happened in 1982.

A composite image showing the total lunar eclipse that happened during a supermoon on Sept. 27, 2015, as seen from Denver. Before 2015, the last supermoon-and-total-lunar-eclipse combo happened in 1982.

Credit: NASA/Bill Ingalls

During a total lunar eclipse, the moon may appear “blood red,” or at least ruddy brown. This unusual hue happens because when the moon is covered by Earth’s shadow, some of the light from Earth’s sunrises and sunsets falls on the moon and makes it appear red, at least from Earth,according to, a Live Science sister site.

The last total lunar eclipse happened during Sept. 27 and 28, 2015. To watch the upcoming total lunar eclipse, tune into

Skywatchers in North America will be able to see the total lunar eclipse before sunrise on Jan. 31. People in the Middle East, Asia, eastern Russia, Australia and New Zealand will be able to view it during moonrise on the evening of Jan. 31, according to NASA.

However, the supermoon will be visible worldwide, as will the blue moon, so long as there isn’t too much cloud cover.

Original article on Live Science.