aads

The Double Cluster in Perseus

The Double Cluster in Perseus, via Tom Wildoner at The Dark Side Observatory in Weatherly, Pennsylvania.

Tom Wildoner wrote:

Here is a view of the famous double cluster in the constellation Perseus (between Perseus and Cassiopeia). They are also designate NGC 869 and NGC 884. Check out the red supergiants in this view!

Tech Specs: Sky-Watcher Esprit 120mm ED Triplet APO Refractor, Celestron CGEM-DX mount, Canon 6D stock camera, ISO 3200, 20 x 60 second exposures with dark/bias frames, guided using a ZWO ASI290MC and Orion 60mm guide scope. Image date: October 1, 2018. Location: The Dark Side Observatory, Weatherly, PA, USA.

Double Cluster in Perseus

Here’s the relationship between the prominent M or W shape of Cassiopeia and the Double Cluster in Perseus. Read more: Meet the Double Cluster

Bottom line: The Double Cluster in Perseus.



from EarthSky https://ift.tt/2QDVr0w

The Double Cluster in Perseus, via Tom Wildoner at The Dark Side Observatory in Weatherly, Pennsylvania.

Tom Wildoner wrote:

Here is a view of the famous double cluster in the constellation Perseus (between Perseus and Cassiopeia). They are also designate NGC 869 and NGC 884. Check out the red supergiants in this view!

Tech Specs: Sky-Watcher Esprit 120mm ED Triplet APO Refractor, Celestron CGEM-DX mount, Canon 6D stock camera, ISO 3200, 20 x 60 second exposures with dark/bias frames, guided using a ZWO ASI290MC and Orion 60mm guide scope. Image date: October 1, 2018. Location: The Dark Side Observatory, Weatherly, PA, USA.

Double Cluster in Perseus

Here’s the relationship between the prominent M or W shape of Cassiopeia and the Double Cluster in Perseus. Read more: Meet the Double Cluster

Bottom line: The Double Cluster in Perseus.



from EarthSky https://ift.tt/2QDVr0w

Cassiopeia, Queen of the north

On these December evenings, turn toward the northern sky and see its famous constellation Cassiopeia the Queen. In early Decemer, Cassiopeia swings directly over Polaris, the North Star, at roughly 8 p.m. local clock time. Cassiopeia – sometimes called The Lady of the Chair – is famous for having the shape of a telltale W or M. You will find this configuration of stars as a starlit M whenever she reigns highest in the sky, hovering over Polaris.

At this time of year, Cassiopeia can also be seen from tropical and subtropical latitudes in the Southern Hemisphere, too. From there, the constellation appears low in the north around 7 to 8 p.m. on early December evenings. As for Polaris … from the Southern Hemisphere, it’s below the horizon.

Because Cassiopeia returns to the same spot in the sky about four minutes earlier with each passing day, or one-half earlier with each passing week, look for Cassiopeia to be at her high point over Polaris, the North Star, around 6 p.m. in early January.

Zefri Besar in Brunei Darussalam caught Cassiopeia and Andromeda galaxy in November 2016, using a DSLR camera and 50mm lens. Notice that – no matter how they are oriented in the sky – the deeper “V” of Cassiopeia points toward the galaxy.

From a dark country sky, you’ll see that Cassiopeia sits atop the luminous band of stars known as the Milky Way. Arching from horizon to horizon, this soft-glowing boulevard of stars represents an edgewise view into the flat disk of our own Milky Way galaxy. When Cassiopeia climbs above Polaris, the North Star, on these dark winter evenings, note that this hazy belt of stars that we call the Milky Way extends through the Northern Cross in the western sky and past Orion the Hunter in your eastern sky.

This Milky Way is fainter than the glorious broad band of the Milky Way we see in a Northern Hemisphere summer or Southern Hemisphere winter. That’s because we are looking toward the star-rich center of the galaxy at the opposite side of the year. On these December nights, we are looking toward the galaxy’s outer edge, not the center.

The famous Double Cluster in the constellation Perseus is not far from Cassiopeia on the sky’s dome. This chart shows how to use the W or M shape of Cassiopeia to find the Double Cluster. To appreciate the clusters fully, look with your binoculars in a dark sky! More about the Double Cluster here.

As the night marches onward, Cassiopeia – like the hour hand of a clock – circles around the North Star, though in a counter-clockwise direction.

By dawn, you will find Cassiopeia has swept down in the northwest – to a point below the North Star. At that time, if you’re at a southerly latitude, such as the far south U.S., you might not be able to see Cassiopeia. The constellation might be below your horizon. But if you’re located at a latitude like those in the northern U.S., you will still see Cassiopeia sitting on or near your northern horizon.

Look northward on these cold December evenings to see the Queen Cassiopeia sitting proudly on her throne, atop the northern terminus of the Milky Way!

The Queen Cassiopeia, aka The Lady of the Chair. Image via Hubble Source

Bottom line: Watch for Cassiopeia the Queen on these December evenings. The constellation is shaped like an M or W. You’ll find Cassiopeia in the northeast at nightfall, sweeping higher in the north as evening progresses.

A planisphere is virtually indispensable for beginning stargazers. Order your EarthSky Planisphere today!



from EarthSky https://ift.tt/2zIlQk8

On these December evenings, turn toward the northern sky and see its famous constellation Cassiopeia the Queen. In early Decemer, Cassiopeia swings directly over Polaris, the North Star, at roughly 8 p.m. local clock time. Cassiopeia – sometimes called The Lady of the Chair – is famous for having the shape of a telltale W or M. You will find this configuration of stars as a starlit M whenever she reigns highest in the sky, hovering over Polaris.

At this time of year, Cassiopeia can also be seen from tropical and subtropical latitudes in the Southern Hemisphere, too. From there, the constellation appears low in the north around 7 to 8 p.m. on early December evenings. As for Polaris … from the Southern Hemisphere, it’s below the horizon.

Because Cassiopeia returns to the same spot in the sky about four minutes earlier with each passing day, or one-half earlier with each passing week, look for Cassiopeia to be at her high point over Polaris, the North Star, around 6 p.m. in early January.

Zefri Besar in Brunei Darussalam caught Cassiopeia and Andromeda galaxy in November 2016, using a DSLR camera and 50mm lens. Notice that – no matter how they are oriented in the sky – the deeper “V” of Cassiopeia points toward the galaxy.

From a dark country sky, you’ll see that Cassiopeia sits atop the luminous band of stars known as the Milky Way. Arching from horizon to horizon, this soft-glowing boulevard of stars represents an edgewise view into the flat disk of our own Milky Way galaxy. When Cassiopeia climbs above Polaris, the North Star, on these dark winter evenings, note that this hazy belt of stars that we call the Milky Way extends through the Northern Cross in the western sky and past Orion the Hunter in your eastern sky.

This Milky Way is fainter than the glorious broad band of the Milky Way we see in a Northern Hemisphere summer or Southern Hemisphere winter. That’s because we are looking toward the star-rich center of the galaxy at the opposite side of the year. On these December nights, we are looking toward the galaxy’s outer edge, not the center.

The famous Double Cluster in the constellation Perseus is not far from Cassiopeia on the sky’s dome. This chart shows how to use the W or M shape of Cassiopeia to find the Double Cluster. To appreciate the clusters fully, look with your binoculars in a dark sky! More about the Double Cluster here.

As the night marches onward, Cassiopeia – like the hour hand of a clock – circles around the North Star, though in a counter-clockwise direction.

By dawn, you will find Cassiopeia has swept down in the northwest – to a point below the North Star. At that time, if you’re at a southerly latitude, such as the far south U.S., you might not be able to see Cassiopeia. The constellation might be below your horizon. But if you’re located at a latitude like those in the northern U.S., you will still see Cassiopeia sitting on or near your northern horizon.

Look northward on these cold December evenings to see the Queen Cassiopeia sitting proudly on her throne, atop the northern terminus of the Milky Way!

The Queen Cassiopeia, aka The Lady of the Chair. Image via Hubble Source

Bottom line: Watch for Cassiopeia the Queen on these December evenings. The constellation is shaped like an M or W. You’ll find Cassiopeia in the northeast at nightfall, sweeping higher in the north as evening progresses.

A planisphere is virtually indispensable for beginning stargazers. Order your EarthSky Planisphere today!



from EarthSky https://ift.tt/2zIlQk8

Your past is calling: Can you ID stone toolmaking 'ring' tones?

Emory anthrpologist Dietrich Stout invites you to participate in an online experiment, Sounds of the Past, investigating the human ability to discriminate and interpret the sounds produced by stone toolmaking. (Photo by Ann Watson, Emory Photo/Video)

By Carol Clark

Long before everyone started carrying a smart phone everywhere they went — attuned to the sounds of a text, call or email — our ancestors carried a hand axe.

“Stone tools were the key human technology for two million years,” says Dietrich Stout, director of the Paleolithic Technology Laboratory at Emory University. In fact, he adds, the process of making them may have played an important role in our ability to communicate.

If you can spare just 10 minutes for science, you can use your smart phone and a pair of headphones to log onto a web site to help Stout test whether ancient tool-making promoted special acoustic abilities — perhaps even honing the development of spoken language.

Stout is an experimental archeologist who recreates prehistoric stone toolmaking, known as knapping, to study the evolution of the human brain and mind. In many of his experiments, subjects actually bang out the tools as activity in their brains is recorded via functional magnetic resonance imaging (fMRI). He’s already found evidence that the visual-spatial skills used in knapping activate areas of the brain that are involved in language processing.

But what about the sounds of knapping?

“An experienced knapper once told me that he would rather be blindfolded than wear ear plugs while making a stone tool, because he got so much valuable information out of the sound when he struck the stone,” Stout says. “That got me wondering: Do knappers just think that the sounds are giving them meaningful information? Could we give them a test to find out if that’s true?”

Stout teamed up with Robert Rein, from the German Sport University Cologne, to develop just such a test. The result is the online experiment Sounds of the Past, open to everyone — from expert knappers to those who have never knapped at all.


During stone tool production a stone flake is produced by hitting a stone core with another stone, used like a hammer. Factors like the geometry of the core stone and the location and the strength of the strike determine the size of the flake that falls off.

The researchers recorded the sounds of flakes breaking off during stone tool production. Participants in the online experiment are presented with a series of these sounds, with no accompanying visuals, and asked to estimate the length of the flakes produced, within a range of parameters.

Participants are also asked whether they have prior experience knapping. The aim is to get as many experienced knappers as possible to participate, and at least an equal number of those without experience, then compare the results.

“No one is going to guess all the flake sizes, to the millimeter,” Stout says. “But if we plot out the results, we should see if there is a correlation between the level of accuracy and whether someone is an experienced or novice knapper.”

The study is self-funded and does not provide compensation for participants. Individual test results are also not available. “It’s really something that we hope participants will just have fun doing, along with the satisfaction that they are providing data to help us understand the evolution of the human brain,” Stout says.

The length of time the experiment will be available is open ended, he adds, although the researchers hope to have enough results in hand for analysis sometime next year.

Click here to participate in the experiment.

Related:
Complex cognition shaped the Stone Age hand axe
Brain trumps hand in Stone Age tool study

from eScienceCommons https://ift.tt/2E4231w
Emory anthrpologist Dietrich Stout invites you to participate in an online experiment, Sounds of the Past, investigating the human ability to discriminate and interpret the sounds produced by stone toolmaking. (Photo by Ann Watson, Emory Photo/Video)

By Carol Clark

Long before everyone started carrying a smart phone everywhere they went — attuned to the sounds of a text, call or email — our ancestors carried a hand axe.

“Stone tools were the key human technology for two million years,” says Dietrich Stout, director of the Paleolithic Technology Laboratory at Emory University. In fact, he adds, the process of making them may have played an important role in our ability to communicate.

If you can spare just 10 minutes for science, you can use your smart phone and a pair of headphones to log onto a web site to help Stout test whether ancient tool-making promoted special acoustic abilities — perhaps even honing the development of spoken language.

Stout is an experimental archeologist who recreates prehistoric stone toolmaking, known as knapping, to study the evolution of the human brain and mind. In many of his experiments, subjects actually bang out the tools as activity in their brains is recorded via functional magnetic resonance imaging (fMRI). He’s already found evidence that the visual-spatial skills used in knapping activate areas of the brain that are involved in language processing.

But what about the sounds of knapping?

“An experienced knapper once told me that he would rather be blindfolded than wear ear plugs while making a stone tool, because he got so much valuable information out of the sound when he struck the stone,” Stout says. “That got me wondering: Do knappers just think that the sounds are giving them meaningful information? Could we give them a test to find out if that’s true?”

Stout teamed up with Robert Rein, from the German Sport University Cologne, to develop just such a test. The result is the online experiment Sounds of the Past, open to everyone — from expert knappers to those who have never knapped at all.


During stone tool production a stone flake is produced by hitting a stone core with another stone, used like a hammer. Factors like the geometry of the core stone and the location and the strength of the strike determine the size of the flake that falls off.

The researchers recorded the sounds of flakes breaking off during stone tool production. Participants in the online experiment are presented with a series of these sounds, with no accompanying visuals, and asked to estimate the length of the flakes produced, within a range of parameters.

Participants are also asked whether they have prior experience knapping. The aim is to get as many experienced knappers as possible to participate, and at least an equal number of those without experience, then compare the results.

“No one is going to guess all the flake sizes, to the millimeter,” Stout says. “But if we plot out the results, we should see if there is a correlation between the level of accuracy and whether someone is an experienced or novice knapper.”

The study is self-funded and does not provide compensation for participants. Individual test results are also not available. “It’s really something that we hope participants will just have fun doing, along with the satisfaction that they are providing data to help us understand the evolution of the human brain,” Stout says.

The length of time the experiment will be available is open ended, he adds, although the researchers hope to have enough results in hand for analysis sometime next year.

Click here to participate in the experiment.

Related:
Complex cognition shaped the Stone Age hand axe
Brain trumps hand in Stone Age tool study

from eScienceCommons https://ift.tt/2E4231w

Learn ethnobotany while making holiday gifts


Click here if video does not appear on screen.

What does an ethnobotanist give for presents during the holidays? If you’re Cassandra Quave, you enlist your kids to help you make herbal-infused, bees-wax chapstick from scratch. Marigold, cinnamon, nutmeg and black pepper are just a few of the ingredients.

Quave is an assistant professor in Emory’s Center for the Study of Human Health and in the School of Medicine’s Department of Dermatology. Her specialty of ethnobotany takes her around the world, studying how traditional healers use plants. She’s particularly interested in plants for treating skin infections and wounds. She collects the plants, extracts their chemical compounds, and tests them for efficacy in combating antibiotic-resistant infections.

Watch Quave’s latest video on her TeachEthnobotany YouTube channel to learn how to make your own botanical chapstick. And check out some of her other videos. She’ll take you to a traditional market in Kuwait to learn about dates, and to the Atlanta Botanical Garden for the backstory of “the vine of the soul.”

Related:
The Plant Hunters
Invasive weed packs power to knock out antibiotic-resistant bacteria
Her patient approach to health



from eScienceCommons https://ift.tt/2E1DqTq

Click here if video does not appear on screen.

What does an ethnobotanist give for presents during the holidays? If you’re Cassandra Quave, you enlist your kids to help you make herbal-infused, bees-wax chapstick from scratch. Marigold, cinnamon, nutmeg and black pepper are just a few of the ingredients.

Quave is an assistant professor in Emory’s Center for the Study of Human Health and in the School of Medicine’s Department of Dermatology. Her specialty of ethnobotany takes her around the world, studying how traditional healers use plants. She’s particularly interested in plants for treating skin infections and wounds. She collects the plants, extracts their chemical compounds, and tests them for efficacy in combating antibiotic-resistant infections.

Watch Quave’s latest video on her TeachEthnobotany YouTube channel to learn how to make your own botanical chapstick. And check out some of her other videos. She’ll take you to a traditional market in Kuwait to learn about dates, and to the Atlanta Botanical Garden for the backstory of “the vine of the soul.”

Related:
The Plant Hunters
Invasive weed packs power to knock out antibiotic-resistant bacteria
Her patient approach to health



from eScienceCommons https://ift.tt/2E1DqTq

Lung cancer screening part 1: the benefits and harms according to clinical trials

Lung cancer CT scan

Beating lung cancer remains one of our biggest challenges. With more than 35,000 lives lost to the disease every year, it’s the most common cause of cancer death in the UK.

Survival from lung cancer remains stubbornly low. And one reason for this is that people are often diagnosed at a late stage, when there are few curative treatment options available.

That’s why researchers are finding out if it’s possible to detect lung cancer at an early stage through screening, and whether the benefits of diagnosing more lung cancers early through screening outweigh the harms.

In part one of this two-part series, we’ll fill you in on the story of lung cancer screening and some of the big unanswered questions.

A history of lung cancer screening

Screening people without symptoms for early signs of lung cancer isn’t a new idea.

Doctors first started researching the use of chest x-rays to find early lung tumours in groups of men in the 1950s. But trials carried out both in the UK and the US produced disappointing results – giving men regular chest x-rays didn’t reduce the number of lung cancer deaths.

Lung cancer screening was put on the backburner.

In 1977 the first study of computed tomography (CT) scans to look for lung cancer was published. The computing power combined with x-rays meant doctors could see the lungs in more detail than before. But this came with a big downside – the amount of radiation people are exposed to in a CT scan is much higher than traditional chest x-rays.

Again, technology improved to help overcome this problem. In 1996, researchers showed that newer CT scanners, which give off a lower radiation dose, were just as good at detecting small abnormalities, which could be lung cancer, as older machines.

Several clinical trials were carried out to see if offering regular scans to certain people with no symptoms of lung cancer could find more cases at an early stage, when they are more likely to be treated successfully.

But the number of people who get lung cancer is relatively small compared to the number who don’t. This is even true for those at higher risk, such as smokers. So many thousands of people need to be screened to get robust evidence that screening decreases the number of people dying from the disease. And the early attempts at clinical trials were too small to provide a definite answer.

The need to go big: a large trial opens

In 2002 an ambitious trial, called the National Lung Screening Trial (NLST), opened in the US to build a clearer picture.

The trial involved more than 53,000 people at high risk from lung cancer – that’s people over 50 who had smoked heavily over a long period. They were screened annually for 3 years, using either a chest x-ray or the low radiation dose CT scan.

The results showed around a 20% reduction in the number of lung cancer deaths in the group monitored with the low dose CT scans compared to x-rays – we blogged about it when the results were released back in 2011. More cancers were diagnosed at the earliest stage using low dose CT, and one death from lung cancer was averted for every 330 people screened with low dose CT compared to an x-ray. But the trial left several points unaddressed.

  • There wasn’t an ‘unscreened’ group – all the participants had a scan of some kind (either x-ray or low dose CT), meaning the true benefits and harms of screening compared to people not having any type of screening were left unknown.
  • There was a high rate of ‘false alarms’ – around 4 in 10 people had CT scans that warranted further investigation, but more than 9 in 10 of these cases (96%) turned out not to be cancer.
  • Further diagnostic tests carry risks – a small number of people died because of having further invasive tests, such as a biopsy under anaesthetic, after an abnormal scan result. Some of these people didn’t have lung cancer.
  • Overdiagnosis – it’s been estimated that in this trial around 1 in 5 lung cancers detected by low dose CT were overdiagnosed. An overdiagnosed cancer is one that that would never become dangerous. As it’s not possible to tell on an individual basis if a cancer is overdiagnosed, and adjust treatment plans accordingly, these people were treated for a lung cancer unnecessarily – this is called overtreatment.

Many other smaller European lung screening studies have been carried out since the publication of the US trial. This includes the UK Lung Screening Trial (UKLST) and the second largest lung screening trial to date, the NELSON trial (based in Belgium and Holland).

Like the US trial, both European studies included people aged 50-74 who were long-term, heavy current or former smokers. But the European trials also included a group who had no screening as a comparison. Those who did get screening were tested just once (UKLST) or at different intervals between 1 and 2.5 years (NELSON).

The two trials ask a few other important questions about screening.

  • Is it possible to cut the number of people needing invasive diagnostic tests by better predicting which abnormal results might be lung cancer?
  • Can studying the size and growth of lung abnormalities found on scans (called nodules) help reduce the number of cancers being treated unnecessarily?
  • What is the psychological impact on people who have a ‘false alarm’, and does screening impact on smokers’ motivation to quit?

Results from the UK Lung Screening Trial showed that around 85% of the lung cancers picked up through screening were early stage. But as a pilot – with 2027 people receiving a CT scan and 2028 people receiving no screening – the study wasn’t large enough to tell if lung screening reduces the number of people dying from lung cancer.

The UKLST researchers have speculated that adopting a ‘watch and wait’ approach for low risk nodules might reduce false positives and overdiganosis of lung cancer. More research will uncover if this is the case.

Researchers leading the bigger NELSON trial have been analysing the data, and an early glimpse of some of the highly-anticipated results were presented at a recent European conference. While the full results are yet to be published in a scientific journal, those revealed at the conference suggest CT lung screening can reduce deaths from lung cancer in those at high risk.

If it saves lives, what are the downsides?

Research has shown that not all lung cancers need treating. Some grow quickly and need to be treated urgently, while others grow very slowly without causing any harm. They may even disappear completely thanks to our immune system.

We don’t yet fully understand the biology of lung cancer and how it develops, so doctors can’t reliably tell the slow growing harmless tumours from the aggressive, life-threatening ones.

Screening will likely result in doctors treating people who didn’t need treatment, which means some people having unnecessary surgery, radiotherapy and chemotherapy. And they will also face the physical and psychological side effects that come with this diagnosis and treatment.

Other harms of screening include spotting something that turns out not to be cancer (false alarms), which can result in further scans, potentially invasive biopsies, surgery, as well as unnecessary distress. Screening also exposes people to radiation. And even though modern CT scanners give out lower levels of radiation, it still increases the risk of developing cancer in the future, particularly in people with lungs already damaged by long-term smoking.

Weighing up the benefits and harms is hugely complicated, and the only way to fully understand the pros and cons is through years of research and pooling together the results of large clinical trials.

The next steps

The combined weight of data from the NELSON trial and its UK counterpart could be enough to settle the discussions on lung screening.

But the decision on whether certain groups of people in the UK should be offered lung screening in the form of CT scans falls to the National Screening Committee.

It has the difficult task of weighing up all the pros and cons to come up with a recommendation. Together with experts from the field, it needs to work out if lung screening would overall do more good than harm, while also being cost-effective for the NHS. If so, it would then work out details, like the age at which screening might be offered, who it should be offered to and how often scans should be done.

Researchers are looking for improvements

In the meantime, researchers are continuing to test screening in studies. In some cases, this involves an assessment of someone’s risk of developing lung cancer in the future, based on lifestyle information and then further investigations for those judged at certain levels of risk. In parts of England, some people are being offered a lung health assessment, followed by a low dose CT scan in some cases, as part of NHS projects trying to address poor lung cancer survival. And the UK’s latest, and largest, lung cancer screening trial has just been announced by University College London Hospitals NHS Foundation Trust (UCLH) and UCL.

If you’ve been offered the opportunity to have a low dose CT scan as part of these projects, it’s important to remember that having tests when you don’t have symptoms of a disease comes with both harms and benefits. You can speak to your doctor or other health professionals for advice, as well as making sure you read all the information that comes with the invitation.

Together this paints a complicated picture. There isn’t a national lung screening programme available in the UK, but there’s appetite from doctors and the NHS to run studies and introduce initiatives that look a lot like screening.

To help reach a consensus on how this type of activity should proceed, we ran an expert workshop in March with representatives from the National Screening Committee, NHS England and senior doctors and researchers. It was agreed that robust, evidence-led guidelines should be developed for the NHS projects, so that the way the projects are carried out, and they data they collect, are consistent.

While researchers and the National Screening Committee are still looking at the results from lung screening studies and gathering more evidence, science never stops. Researchers across the world are finding ways to improve CT scans as a screening test and looking for new ways to try and save lives from lung cancer.

Could other tests that don’t use radiation be as good, or better, than CT scans at detecting lung cancers earlier? Are there more reliable ways to tell which cancers need treating versus cancers or small growths that won’t cause any harm?

We’ll discuss that and more in part two of this series, looking at the latest research into detection technology that could make a big impact on lung cancer.

Emma



from Cancer Research UK – Science blog https://ift.tt/2SuwNN9
Lung cancer CT scan

Beating lung cancer remains one of our biggest challenges. With more than 35,000 lives lost to the disease every year, it’s the most common cause of cancer death in the UK.

Survival from lung cancer remains stubbornly low. And one reason for this is that people are often diagnosed at a late stage, when there are few curative treatment options available.

That’s why researchers are finding out if it’s possible to detect lung cancer at an early stage through screening, and whether the benefits of diagnosing more lung cancers early through screening outweigh the harms.

In part one of this two-part series, we’ll fill you in on the story of lung cancer screening and some of the big unanswered questions.

A history of lung cancer screening

Screening people without symptoms for early signs of lung cancer isn’t a new idea.

Doctors first started researching the use of chest x-rays to find early lung tumours in groups of men in the 1950s. But trials carried out both in the UK and the US produced disappointing results – giving men regular chest x-rays didn’t reduce the number of lung cancer deaths.

Lung cancer screening was put on the backburner.

In 1977 the first study of computed tomography (CT) scans to look for lung cancer was published. The computing power combined with x-rays meant doctors could see the lungs in more detail than before. But this came with a big downside – the amount of radiation people are exposed to in a CT scan is much higher than traditional chest x-rays.

Again, technology improved to help overcome this problem. In 1996, researchers showed that newer CT scanners, which give off a lower radiation dose, were just as good at detecting small abnormalities, which could be lung cancer, as older machines.

Several clinical trials were carried out to see if offering regular scans to certain people with no symptoms of lung cancer could find more cases at an early stage, when they are more likely to be treated successfully.

But the number of people who get lung cancer is relatively small compared to the number who don’t. This is even true for those at higher risk, such as smokers. So many thousands of people need to be screened to get robust evidence that screening decreases the number of people dying from the disease. And the early attempts at clinical trials were too small to provide a definite answer.

The need to go big: a large trial opens

In 2002 an ambitious trial, called the National Lung Screening Trial (NLST), opened in the US to build a clearer picture.

The trial involved more than 53,000 people at high risk from lung cancer – that’s people over 50 who had smoked heavily over a long period. They were screened annually for 3 years, using either a chest x-ray or the low radiation dose CT scan.

The results showed around a 20% reduction in the number of lung cancer deaths in the group monitored with the low dose CT scans compared to x-rays – we blogged about it when the results were released back in 2011. More cancers were diagnosed at the earliest stage using low dose CT, and one death from lung cancer was averted for every 330 people screened with low dose CT compared to an x-ray. But the trial left several points unaddressed.

  • There wasn’t an ‘unscreened’ group – all the participants had a scan of some kind (either x-ray or low dose CT), meaning the true benefits and harms of screening compared to people not having any type of screening were left unknown.
  • There was a high rate of ‘false alarms’ – around 4 in 10 people had CT scans that warranted further investigation, but more than 9 in 10 of these cases (96%) turned out not to be cancer.
  • Further diagnostic tests carry risks – a small number of people died because of having further invasive tests, such as a biopsy under anaesthetic, after an abnormal scan result. Some of these people didn’t have lung cancer.
  • Overdiagnosis – it’s been estimated that in this trial around 1 in 5 lung cancers detected by low dose CT were overdiagnosed. An overdiagnosed cancer is one that that would never become dangerous. As it’s not possible to tell on an individual basis if a cancer is overdiagnosed, and adjust treatment plans accordingly, these people were treated for a lung cancer unnecessarily – this is called overtreatment.

Many other smaller European lung screening studies have been carried out since the publication of the US trial. This includes the UK Lung Screening Trial (UKLST) and the second largest lung screening trial to date, the NELSON trial (based in Belgium and Holland).

Like the US trial, both European studies included people aged 50-74 who were long-term, heavy current or former smokers. But the European trials also included a group who had no screening as a comparison. Those who did get screening were tested just once (UKLST) or at different intervals between 1 and 2.5 years (NELSON).

The two trials ask a few other important questions about screening.

  • Is it possible to cut the number of people needing invasive diagnostic tests by better predicting which abnormal results might be lung cancer?
  • Can studying the size and growth of lung abnormalities found on scans (called nodules) help reduce the number of cancers being treated unnecessarily?
  • What is the psychological impact on people who have a ‘false alarm’, and does screening impact on smokers’ motivation to quit?

Results from the UK Lung Screening Trial showed that around 85% of the lung cancers picked up through screening were early stage. But as a pilot – with 2027 people receiving a CT scan and 2028 people receiving no screening – the study wasn’t large enough to tell if lung screening reduces the number of people dying from lung cancer.

The UKLST researchers have speculated that adopting a ‘watch and wait’ approach for low risk nodules might reduce false positives and overdiganosis of lung cancer. More research will uncover if this is the case.

Researchers leading the bigger NELSON trial have been analysing the data, and an early glimpse of some of the highly-anticipated results were presented at a recent European conference. While the full results are yet to be published in a scientific journal, those revealed at the conference suggest CT lung screening can reduce deaths from lung cancer in those at high risk.

If it saves lives, what are the downsides?

Research has shown that not all lung cancers need treating. Some grow quickly and need to be treated urgently, while others grow very slowly without causing any harm. They may even disappear completely thanks to our immune system.

We don’t yet fully understand the biology of lung cancer and how it develops, so doctors can’t reliably tell the slow growing harmless tumours from the aggressive, life-threatening ones.

Screening will likely result in doctors treating people who didn’t need treatment, which means some people having unnecessary surgery, radiotherapy and chemotherapy. And they will also face the physical and psychological side effects that come with this diagnosis and treatment.

Other harms of screening include spotting something that turns out not to be cancer (false alarms), which can result in further scans, potentially invasive biopsies, surgery, as well as unnecessary distress. Screening also exposes people to radiation. And even though modern CT scanners give out lower levels of radiation, it still increases the risk of developing cancer in the future, particularly in people with lungs already damaged by long-term smoking.

Weighing up the benefits and harms is hugely complicated, and the only way to fully understand the pros and cons is through years of research and pooling together the results of large clinical trials.

The next steps

The combined weight of data from the NELSON trial and its UK counterpart could be enough to settle the discussions on lung screening.

But the decision on whether certain groups of people in the UK should be offered lung screening in the form of CT scans falls to the National Screening Committee.

It has the difficult task of weighing up all the pros and cons to come up with a recommendation. Together with experts from the field, it needs to work out if lung screening would overall do more good than harm, while also being cost-effective for the NHS. If so, it would then work out details, like the age at which screening might be offered, who it should be offered to and how often scans should be done.

Researchers are looking for improvements

In the meantime, researchers are continuing to test screening in studies. In some cases, this involves an assessment of someone’s risk of developing lung cancer in the future, based on lifestyle information and then further investigations for those judged at certain levels of risk. In parts of England, some people are being offered a lung health assessment, followed by a low dose CT scan in some cases, as part of NHS projects trying to address poor lung cancer survival. And the UK’s latest, and largest, lung cancer screening trial has just been announced by University College London Hospitals NHS Foundation Trust (UCLH) and UCL.

If you’ve been offered the opportunity to have a low dose CT scan as part of these projects, it’s important to remember that having tests when you don’t have symptoms of a disease comes with both harms and benefits. You can speak to your doctor or other health professionals for advice, as well as making sure you read all the information that comes with the invitation.

Together this paints a complicated picture. There isn’t a national lung screening programme available in the UK, but there’s appetite from doctors and the NHS to run studies and introduce initiatives that look a lot like screening.

To help reach a consensus on how this type of activity should proceed, we ran an expert workshop in March with representatives from the National Screening Committee, NHS England and senior doctors and researchers. It was agreed that robust, evidence-led guidelines should be developed for the NHS projects, so that the way the projects are carried out, and they data they collect, are consistent.

While researchers and the National Screening Committee are still looking at the results from lung screening studies and gathering more evidence, science never stops. Researchers across the world are finding ways to improve CT scans as a screening test and looking for new ways to try and save lives from lung cancer.

Could other tests that don’t use radiation be as good, or better, than CT scans at detecting lung cancers earlier? Are there more reliable ways to tell which cancers need treating versus cancers or small growths that won’t cause any harm?

We’ll discuss that and more in part two of this series, looking at the latest research into detection technology that could make a big impact on lung cancer.

Emma



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A giant relic of a disrupted tadpole galaxy

Here are 2 galaxies in a galaxy group with an unusual name: Hickson’s Compact Group 98. See the 2 “smudges” at the center of the image? Each smudge is a galaxy not unlike our Milky Way. Notice the “tadpole” structure of the pair, which astronomers believe was formed when the pair demolished a much smaller galaxy. Image via N. Brosch/Tel Aviv University/RAS.

When larger galaxies collide with smaller ones, the smaller galaxies’ stars are either incorporated into the larger galaxies, or they’re ejected into intergalactic space. In this ongoing process, the galaxies around us in space may form patterns discernible to our human eyes and brains, in the great Rorschach test of the night sky. And so a team of astronomers from Israel, the U.S. and Russia has identified a disrupted galaxy that they say resembles a giant “tadpole,” complete with an elliptical head and a long, straight tail, located about 300 million light-years away from Earth. They describe this “tadpole” galaxy in research that will appear in the January 2019 issue of the peer-reviewed journal Monthly Notices of the Royal Astronomical Society (you’ll find it online here).

Astronomer Noah Brosch of Tel Aviv University led the research for the study. He said:

We have found a giant, exceptional relic of a disrupted galaxy.

Disrupted, in this case, means by another galaxy. In other words, astronomers believe the “tadpole” galaxy pair formed when they collided with and demolished a much smaller galaxy. According to the study, when the gravitational force of two larger galaxies pulled on stars in this smaller, vulnerable galaxy, the stars closer to the pair formed the “head” of the tadpole. Stars lingering in the victim galaxy formed the “tail.”

Astronomer R. Michael Rich of UCLA, who participated in the study, said:

What makes this object extraordinary is that the tail alone is almost 500,000 light-years long. If it were at the distance of the Andromeda galaxy, which is about 2.5 million light years from Earth, it would reach a fifth of the way to our own Milky Way.

Overall, the “tadpole” galaxy is one million light-years long from end to end, 10 times larger than our home galaxy, the Milky Way.

It’s part of a small group of galaxies called Hickson’s Compact Group 98, which, astronomers believe, will merge into a single galaxy in the next billion years.

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Bottom line: Astronomers have identified 2 galaxies in the galaxy group Hickson’s Compact Group 98 that have a “tadpole” structure. Astronomers believe this structure was formed when the pair demolished a much smaller galaxy.

Source: Hickson Compact Group 98: a complex merging group with a giant tidal tail and a humongous envelope

Via RAS



from EarthSky https://ift.tt/2RA2c0M

Here are 2 galaxies in a galaxy group with an unusual name: Hickson’s Compact Group 98. See the 2 “smudges” at the center of the image? Each smudge is a galaxy not unlike our Milky Way. Notice the “tadpole” structure of the pair, which astronomers believe was formed when the pair demolished a much smaller galaxy. Image via N. Brosch/Tel Aviv University/RAS.

When larger galaxies collide with smaller ones, the smaller galaxies’ stars are either incorporated into the larger galaxies, or they’re ejected into intergalactic space. In this ongoing process, the galaxies around us in space may form patterns discernible to our human eyes and brains, in the great Rorschach test of the night sky. And so a team of astronomers from Israel, the U.S. and Russia has identified a disrupted galaxy that they say resembles a giant “tadpole,” complete with an elliptical head and a long, straight tail, located about 300 million light-years away from Earth. They describe this “tadpole” galaxy in research that will appear in the January 2019 issue of the peer-reviewed journal Monthly Notices of the Royal Astronomical Society (you’ll find it online here).

Astronomer Noah Brosch of Tel Aviv University led the research for the study. He said:

We have found a giant, exceptional relic of a disrupted galaxy.

Disrupted, in this case, means by another galaxy. In other words, astronomers believe the “tadpole” galaxy pair formed when they collided with and demolished a much smaller galaxy. According to the study, when the gravitational force of two larger galaxies pulled on stars in this smaller, vulnerable galaxy, the stars closer to the pair formed the “head” of the tadpole. Stars lingering in the victim galaxy formed the “tail.”

Astronomer R. Michael Rich of UCLA, who participated in the study, said:

What makes this object extraordinary is that the tail alone is almost 500,000 light-years long. If it were at the distance of the Andromeda galaxy, which is about 2.5 million light years from Earth, it would reach a fifth of the way to our own Milky Way.

Overall, the “tadpole” galaxy is one million light-years long from end to end, 10 times larger than our home galaxy, the Milky Way.

It’s part of a small group of galaxies called Hickson’s Compact Group 98, which, astronomers believe, will merge into a single galaxy in the next billion years.

The 2019 lunar calendars are here! Order yours before they’re gone. Makes a great gift.

Bottom line: Astronomers have identified 2 galaxies in the galaxy group Hickson’s Compact Group 98 that have a “tadpole” structure. Astronomers believe this structure was formed when the pair demolished a much smaller galaxy.

Source: Hickson Compact Group 98: a complex merging group with a giant tidal tail and a humongous envelope

Via RAS



from EarthSky https://ift.tt/2RA2c0M

The spectacular Large Magellanic Cloud

This ground-based image of the Large Magellanic Cloud was taken by German astrophotographer Eckhard Slawik. Image via ESA

This ground-based image of the Large Magellanic Cloud was taken by German astrophotographer Eckhard Slawik. Image via ESA.

EarthSky lunar calendars are cool! They make great gifts. Order now. Going fast!

The Large Magellanic Cloud (LMC), which is visible to the unaided human eye, is a familiar sight to observers in Earth’s Southern Hemisphere. Along with the Small Magellanic Cloud (SMC), not far from it on our sky’s dome, it looks like nothing so much as a small, faint bit of the Milky Way that has broken off. And yet it is not part of our Milky Way galaxy. It is a separate small galaxy, thought to be orbiting our larger Milky Way.

Large Magellanic Cloud

If you’re far enough south on Earth’s globe, you can star-hop to the Large Magellanic Cloud via the bright stars Sirius (at right) and Canopus (at left). Photo taken at nightfall on May 15, 2013, from Kalgoorlie, Western Australia, by Oliver Floyd. Thank you, Oliver!

How to find the Large Magellanic Cloud. For observers south of about 20 degrees south latitude, the LMC is circumpolar, meaning that it can be seen (at least in part) all night every night of the year, weather permitting.

In the Northern Hemisphere, only observers south of about 20 degrees north latitude can ever see it at all. This excludes North America (except southern Mexico), Europe, northern Africa and northern Asia.

View larger The Large Magellanic Cloud is found in the constellations Dorado and Mensa. The nearby star is Canopus.

View larger. | The Large Magellanic Cloud is found in the constellations Dorado and Mensa. The nearby star is Canopus.

The LMC is located about 22 degrees from the South Celestial Pole, approximately on the border between the constellations Dorado and Mensa in a region of faint stars. It covers an area of the sky about 9 by 11 degrees, and shines with a total integrated magnitude of approximately zero. If all of its light were concentrated in a starlike pinpoint, it would be one of the brightest stars in the heavens. However, since the light is spread over nearly 100 square degrees, it appears only as a faint smudge.

From tropical latitudes in the Northern Hemisphere, where it still can be observed, the LMC is best seen in the evening from December to April. When the constellation Orion reaches its highest point in the sky, so does the Large Magellanic Cloud. But even at 15 degrees north latitude (the latitude of Central America), the LMC never gets far above the southern horizon.

However, it’s fairly easy to star-hop to this southern treasure by using the two brightest stars in the nighttime sky: Sirius and Canopus. Draw a line from Sirius and past the right side of Canopus to descend to the LMC. Our sky chart is designed for about 15 degrees north. Farther south, the LMC sits higher in the southern sky.

View larger. | A Perseid meteor streaks between the two Magellanic Clouds during the peak of the 2013 Perseid meteor shower. Photo by Colin Legg.

A Perseid meteor streaks between the two Magellanic Clouds in August 2013. Photo by Colin Legg.

History and myth of the Large Magellanic Cloud. Being so far south on the sky’s dome, the Large Magellanic Cloud was not known in classical northern mythology at all. Understandably, it factors better for observers in the Southern Hemisphere. The nearby constellation, Mensa (“Table”), originally was named after South Africa’s Table Mountain, and a story from that country equates the Large Magellanic Cloud with a puff of smoke from a pipe-smoking contest held on the mountain. Australian Aboriginal storytellers relate that the LMC is the campsite of an old man, whereas the Small Magellanic Cloud (SMC) is the campsite of his wife. The couple, known jointly as Jukara, had grown too old to feed themselves, so other star beings bring them fish from the sky river we know as the Milky Way.

The European “discovery” of the LMC and SMC is attributed to explorer Ferdinand Magellan, although such obvious heavenly bodies certainly were seen before.

Large Magellanic Cloud as captured by astrophotographer Justin Ng of Singapore. Justin was at Mount Bromo, an active volcano in East Java, Indonesia when he captured this photo.

Large Magellanic Cloud as captured by astrophotographer Justin Ng of Singapore. Justin was at Mount Bromo, an active volcano in East Java, Indonesia, when he took this photo.

Science of the Large Magellanic Cloud. After two smaller galaxies not visible to the human eye, the LMC is the third closest galaxy to the Milky Way, and in fact is thought by most astronomers to be orbiting the Milky Way.

Although there is some uncertainty due to various methods of distance determination, the best current estimate puts the LMC at 150,000 to about 160,000 light-years away, or about five or six times as far from Earth as Earth is from the center of the Milky Way. Other estimates have it as far as 180,000 light-years.

Its shape suggests a transitional form between a small spiral galaxy and an irregular galaxy. About 30,000 light-years across in the longest dimension, it appears from Earth more than 20 times the width of a full moon.

Estimates vary from a few billion to perhaps 10 billion stars in this galaxy, at best no more than about one-tenth the mass of the Milky Way.

The center of the LMC is approximately RA: 5h 23m 35s, dec: -69° 45’22”

Nearly 200 000 light-years from Earth, the Large Magellanic Cloud, a satellite galaxy of the Milky Way, floats in space, in a long and slow dance around our galaxy. As the Milky Way’s gravity gently tugs on its neighbour’s gas clouds, they collapse to form new stars. In turn, these light up the gas clouds in a kaleidoscope of colors, visible in this image from the NASA/ESA Hubble Space Telescope. Image via ESA/NASA/Hubble

Nearly 200 000 light-years from Earth, the Large Magellanic Cloud, a satellite galaxy of the Milky Way, floats in space in a long and slow dance around our galaxy. As the Milky Way’s gravity gently tugs on its neighbor’s gas clouds, they collapse to form new stars. In turn, these light up the gas clouds in a kaleidoscope of colors, visible in this image from the Hubble Space Telescope. Image via ESA/NASA/Hubble.

Bottom line: From tropical latitudes in the Northern Hemisphere, where it can be observed, the Large Magellanic Cloud is best seen in the evening from December to April. From the Southern Hemisphere, it’s easy to see and spectacular!



from EarthSky https://ift.tt/2BQ868K
This ground-based image of the Large Magellanic Cloud was taken by German astrophotographer Eckhard Slawik. Image via ESA

This ground-based image of the Large Magellanic Cloud was taken by German astrophotographer Eckhard Slawik. Image via ESA.

EarthSky lunar calendars are cool! They make great gifts. Order now. Going fast!

The Large Magellanic Cloud (LMC), which is visible to the unaided human eye, is a familiar sight to observers in Earth’s Southern Hemisphere. Along with the Small Magellanic Cloud (SMC), not far from it on our sky’s dome, it looks like nothing so much as a small, faint bit of the Milky Way that has broken off. And yet it is not part of our Milky Way galaxy. It is a separate small galaxy, thought to be orbiting our larger Milky Way.

Large Magellanic Cloud

If you’re far enough south on Earth’s globe, you can star-hop to the Large Magellanic Cloud via the bright stars Sirius (at right) and Canopus (at left). Photo taken at nightfall on May 15, 2013, from Kalgoorlie, Western Australia, by Oliver Floyd. Thank you, Oliver!

How to find the Large Magellanic Cloud. For observers south of about 20 degrees south latitude, the LMC is circumpolar, meaning that it can be seen (at least in part) all night every night of the year, weather permitting.

In the Northern Hemisphere, only observers south of about 20 degrees north latitude can ever see it at all. This excludes North America (except southern Mexico), Europe, northern Africa and northern Asia.

View larger The Large Magellanic Cloud is found in the constellations Dorado and Mensa. The nearby star is Canopus.

View larger. | The Large Magellanic Cloud is found in the constellations Dorado and Mensa. The nearby star is Canopus.

The LMC is located about 22 degrees from the South Celestial Pole, approximately on the border between the constellations Dorado and Mensa in a region of faint stars. It covers an area of the sky about 9 by 11 degrees, and shines with a total integrated magnitude of approximately zero. If all of its light were concentrated in a starlike pinpoint, it would be one of the brightest stars in the heavens. However, since the light is spread over nearly 100 square degrees, it appears only as a faint smudge.

From tropical latitudes in the Northern Hemisphere, where it still can be observed, the LMC is best seen in the evening from December to April. When the constellation Orion reaches its highest point in the sky, so does the Large Magellanic Cloud. But even at 15 degrees north latitude (the latitude of Central America), the LMC never gets far above the southern horizon.

However, it’s fairly easy to star-hop to this southern treasure by using the two brightest stars in the nighttime sky: Sirius and Canopus. Draw a line from Sirius and past the right side of Canopus to descend to the LMC. Our sky chart is designed for about 15 degrees north. Farther south, the LMC sits higher in the southern sky.

View larger. | A Perseid meteor streaks between the two Magellanic Clouds during the peak of the 2013 Perseid meteor shower. Photo by Colin Legg.

A Perseid meteor streaks between the two Magellanic Clouds in August 2013. Photo by Colin Legg.

History and myth of the Large Magellanic Cloud. Being so far south on the sky’s dome, the Large Magellanic Cloud was not known in classical northern mythology at all. Understandably, it factors better for observers in the Southern Hemisphere. The nearby constellation, Mensa (“Table”), originally was named after South Africa’s Table Mountain, and a story from that country equates the Large Magellanic Cloud with a puff of smoke from a pipe-smoking contest held on the mountain. Australian Aboriginal storytellers relate that the LMC is the campsite of an old man, whereas the Small Magellanic Cloud (SMC) is the campsite of his wife. The couple, known jointly as Jukara, had grown too old to feed themselves, so other star beings bring them fish from the sky river we know as the Milky Way.

The European “discovery” of the LMC and SMC is attributed to explorer Ferdinand Magellan, although such obvious heavenly bodies certainly were seen before.

Large Magellanic Cloud as captured by astrophotographer Justin Ng of Singapore. Justin was at Mount Bromo, an active volcano in East Java, Indonesia when he captured this photo.

Large Magellanic Cloud as captured by astrophotographer Justin Ng of Singapore. Justin was at Mount Bromo, an active volcano in East Java, Indonesia, when he took this photo.

Science of the Large Magellanic Cloud. After two smaller galaxies not visible to the human eye, the LMC is the third closest galaxy to the Milky Way, and in fact is thought by most astronomers to be orbiting the Milky Way.

Although there is some uncertainty due to various methods of distance determination, the best current estimate puts the LMC at 150,000 to about 160,000 light-years away, or about five or six times as far from Earth as Earth is from the center of the Milky Way. Other estimates have it as far as 180,000 light-years.

Its shape suggests a transitional form between a small spiral galaxy and an irregular galaxy. About 30,000 light-years across in the longest dimension, it appears from Earth more than 20 times the width of a full moon.

Estimates vary from a few billion to perhaps 10 billion stars in this galaxy, at best no more than about one-tenth the mass of the Milky Way.

The center of the LMC is approximately RA: 5h 23m 35s, dec: -69° 45’22”

Nearly 200 000 light-years from Earth, the Large Magellanic Cloud, a satellite galaxy of the Milky Way, floats in space, in a long and slow dance around our galaxy. As the Milky Way’s gravity gently tugs on its neighbour’s gas clouds, they collapse to form new stars. In turn, these light up the gas clouds in a kaleidoscope of colors, visible in this image from the NASA/ESA Hubble Space Telescope. Image via ESA/NASA/Hubble

Nearly 200 000 light-years from Earth, the Large Magellanic Cloud, a satellite galaxy of the Milky Way, floats in space in a long and slow dance around our galaxy. As the Milky Way’s gravity gently tugs on its neighbor’s gas clouds, they collapse to form new stars. In turn, these light up the gas clouds in a kaleidoscope of colors, visible in this image from the Hubble Space Telescope. Image via ESA/NASA/Hubble.

Bottom line: From tropical latitudes in the Northern Hemisphere, where it can be observed, the Large Magellanic Cloud is best seen in the evening from December to April. From the Southern Hemisphere, it’s easy to see and spectacular!



from EarthSky https://ift.tt/2BQ868K

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