aads

Young moon and Spica, west after sunset

It’s fun to hunt for a young moon, a thin crescent moon visible in the west shortly after sunset. The new moon was August 19, 2020 – early in the day – at 2:42 UTC. Thus we expect many people around the world to catch the whisker-thin waxing crescent after sunset August 20. If you miss the slender young moon at dusk on August 20, try again on August 21, 22 and 23.

To see a young moon, you’ll want an unobstructed horizon in the direction of sunset. Find a hill or balcony to stand on, enabling you to peek just a little farther over your horizon. Binoculars come in handy, too, especially around August 20, when the bright evening twilight will be competing with the tiny, ghostly lunar crescent.

Although the star Spica, brightest light in the constellation Virgo the Maiden, serves as a prime example of a first-magnitude star, it might be hard to see this star in the glow of evening dusk (especially from northerly latitudes). If you can’t see it, binoculars will help.

Very thin crescent moon in western twilight after sunset with feathery pink clouds.

View larger. | Jenney Disimon caught the young moon after sunset in August 2019, from Sabah, North Borneo. Thank you, Jenney!

As a general rule, it’s difficult to spot a crescent that’s less than 24 hours old (24 hours after new moon). Everywhere around the world, at sunset August 20, the moon will be over one day old. Even so, from much of the world, the slim crescent will follow the sun beneath the horizon before nightfall.

Want to know when the moon sets in your sky? Click on this Sunset Sunset Calendar, remembering to check the moonrise/moonset box. The time for sunset and moonset presumes a level horizon.

Day by day, watch the illumined portion of the lunar crescent grow, and for the moon to stay out longer after sundown. For a special treat, check out the earthshine softly illuminating the dark side of the moon with either the unaided eye or binoculars.

Bottom line: Will you catch the young moon in the west after sunset on August 20, 2020? Maybe. It’ll be easier to see on August 21, 22 and 23.



from EarthSky https://ift.tt/34jJxiW

It’s fun to hunt for a young moon, a thin crescent moon visible in the west shortly after sunset. The new moon was August 19, 2020 – early in the day – at 2:42 UTC. Thus we expect many people around the world to catch the whisker-thin waxing crescent after sunset August 20. If you miss the slender young moon at dusk on August 20, try again on August 21, 22 and 23.

To see a young moon, you’ll want an unobstructed horizon in the direction of sunset. Find a hill or balcony to stand on, enabling you to peek just a little farther over your horizon. Binoculars come in handy, too, especially around August 20, when the bright evening twilight will be competing with the tiny, ghostly lunar crescent.

Although the star Spica, brightest light in the constellation Virgo the Maiden, serves as a prime example of a first-magnitude star, it might be hard to see this star in the glow of evening dusk (especially from northerly latitudes). If you can’t see it, binoculars will help.

Very thin crescent moon in western twilight after sunset with feathery pink clouds.

View larger. | Jenney Disimon caught the young moon after sunset in August 2019, from Sabah, North Borneo. Thank you, Jenney!

As a general rule, it’s difficult to spot a crescent that’s less than 24 hours old (24 hours after new moon). Everywhere around the world, at sunset August 20, the moon will be over one day old. Even so, from much of the world, the slim crescent will follow the sun beneath the horizon before nightfall.

Want to know when the moon sets in your sky? Click on this Sunset Sunset Calendar, remembering to check the moonrise/moonset box. The time for sunset and moonset presumes a level horizon.

Day by day, watch the illumined portion of the lunar crescent grow, and for the moon to stay out longer after sundown. For a special treat, check out the earthshine softly illuminating the dark side of the moon with either the unaided eye or binoculars.

Bottom line: Will you catch the young moon in the west after sunset on August 20, 2020? Maybe. It’ll be easier to see on August 21, 22 and 23.



from EarthSky https://ift.tt/34jJxiW

Truck-sized asteroid swept within 2,000 miles on Sunday

Small Earth, with green line going past it bent around where it comes nearest Earth, and also the moon's orbit shown.

View larger. | The blue ball in the lower left of this image represents Earth. The curved green arrow represents asteroid 2020 QG, whose orbit was changed by its near-Earth encounter on Sunday. The tick marks on the green line represent 30-minute intervals. You can see that this asteroid was really zooming past! Image via Minor Planet Center.

Newly discovered asteroid ZTF0DxQ – now officially labeled 2020 QG – swept about 1,830 miles (2,900 km) from Earth’s surface on Sunday, August 16, 2020, then zoomed on. It was moving at a speed of about 7.7 miles per second (12.4 km per second) or about 27,600 mph. Because it approached Earth from a sunward direction, it flew past us unseen at 04:08 UTC. Astronomers didn’t detect it until six hours later. This object now holds the record among known asteroids for having swept closest to us without striking us.

Should we be glad it didn’t hit us, or mad it wasn’t detected earlier? Neither one.

And here’s why: relatively speaking, this object is very, very small.

Animated image of tiny object passing Earth.

View larger. | This illustration shows asteroid 2020 QG’s trajectory bending during its close approach to Earth. The asteroid is the closest known nonimpacting asteroid ever detected. Image via NASA/ JPL-Caltech.

It was never going to harm us. Size estimates for objects of this kind are based upon the object’s observed brightness as seen from Earth. 2020 QG is thought to be about 10 to 20 feet (3 to 6 meters) across. That’s in contrast to the biggest asteroids, which are hundreds of miles across. And it’s in contrast to the small asteroid that created 2013’s famous Chelyabinsk meteor, which came even closer to us, entering Earth’s atmosphere over Russia. The Chelyabinsk meteor started out some 66 feet (20 meters) across. It created a gigantic shockwave that broke windows in six Russian cities, causing hundreds of injuries, mostly from flying glass. On the other hand, if an asteroid the size of 2020 QG does enter our atmosphere (and indeed they do, several times each year, according to NASA), the airburst it creates would be too high in Earth’s atmosphere to cause damage on the ground. What’s more, a 10- to 20-foot asteroid would either completely vaporize on its fall through the atmosphere, or drop as a small remnant of its former self – a rock from space, prized by meteorite hunters – onto Earth’s surface or into the ocean. So there was never any real danger of harm. In fact, astronomers appear to get a kick out of seeing tiny asteroids like 2020 QG come this close. Paul Chodas, director of NASA’s Center for Near Earth Object Studies, said in a NASA statement:

It’s really cool to see a small asteroid come by this close, because we can see the Earth’s gravity dramatically bend its trajectory. Our calculations show that this asteroid got turned by 45 degrees or so as it swung by our planet.

But what about that six-hour delay in astronomers’ detection of this asteroid? Cause for outrage? On the contrary …

A red circle around a short white line on a gray background spotted with white dots.

View larger. | The circled streak in the center of this image is asteroid 2020 QG. This image shows how the Zwicky Transient Facility noticed the asteroid – as a fast-moving streak in front of the stars – 6 hours after its closest approach. Image via ZTF/ Caltech Optical Observatories.

Astronomers’ ability to detect asteroids far exceeds what it was. Diminutive asteroids the size of 2020 QG have been sweeping past Earth for billions of years. An asteroid this size couldn’t have been detected at all a few decades ago. In our lifetimes, asteroid-detection technology has greatly advanced. 2020 QG was found via a survey telescope – the Zwicky Transient Facility (ZTF) – on Palomar Mountain in California. It was found by a robotic system developed by some of the smartest people on the planet, who, for decades, have been working to protect Earth from possible destructive asteroid impacts. Go astronomers!

However, 2020 QG’s sweep past Earth on Sunday does point to a weakness in astronomers’ highly developed asteroid-observing abilities. That is, it’s hard for them to see asteroids that come at us from the direction of the sun. Paul Chodas commented to Dave Mosher and Morgan McFall-Johnsen of Business Insider:

There’s not much we can do about detecting inbound asteroids coming from the sunward direction, as asteroids are detected using optical telescopes only (like ZTF), and we can only search for them in the night sky. The idea is that we discover them on one of their prior passages by our planet, and then make predictions years and decades in advance to see whether they have any possibility of impacting.

Mosher and McFall-Johnsen also reported:

NASA has a plan to address these gaps in its asteroid-hunting program. The agency is in the early stages of developing a space telescope that could detect asteroids and comets coming from the sun’s direction.

NASA’s 2020 budget allotted nearly $36 million for that telescope, called the Near-Earth Object Surveillance Mission.

If funding continues, it could launch as early as 2025.

NASA said that, by some estimates, there are hundreds of millions of tiny asteroids the size of 2020 QG. They are extremely hard to discover until they get very close to Earth. The vast majority pass by safely at greater distances, usually, but not always, farther away than our moon.

Meanwhile, in 2005, Congress assigned NASA the goal of finding 90% of the near-Earth asteroids that are about 460 feet (140 meters) or larger in size. Clearly, the larger asteroids pose a larger threat. The good news is that they they can be detected much farther away from Earth. Once found, their orbits can be calculated years into the future, to determine any potential for a future collision. If an asteroid were found to be on a collision course with Earth, assuming it were found years before the collision was due to take place, the world could and surely would take steps to try to divert it.

Bottom line: Asteroid ZTF0DxQ – now officially labeled 2020 QG – swept just 2,000 miles (3,000 km) from Earth’s surface, making it the closest-known asteroid flyby that didn’t involve a strike.

Via Business Insider

Via NASA



from EarthSky https://ift.tt/2EeUOWQ
Small Earth, with green line going past it bent around where it comes nearest Earth, and also the moon's orbit shown.

View larger. | The blue ball in the lower left of this image represents Earth. The curved green arrow represents asteroid 2020 QG, whose orbit was changed by its near-Earth encounter on Sunday. The tick marks on the green line represent 30-minute intervals. You can see that this asteroid was really zooming past! Image via Minor Planet Center.

Newly discovered asteroid ZTF0DxQ – now officially labeled 2020 QG – swept about 1,830 miles (2,900 km) from Earth’s surface on Sunday, August 16, 2020, then zoomed on. It was moving at a speed of about 7.7 miles per second (12.4 km per second) or about 27,600 mph. Because it approached Earth from a sunward direction, it flew past us unseen at 04:08 UTC. Astronomers didn’t detect it until six hours later. This object now holds the record among known asteroids for having swept closest to us without striking us.

Should we be glad it didn’t hit us, or mad it wasn’t detected earlier? Neither one.

And here’s why: relatively speaking, this object is very, very small.

Animated image of tiny object passing Earth.

View larger. | This illustration shows asteroid 2020 QG’s trajectory bending during its close approach to Earth. The asteroid is the closest known nonimpacting asteroid ever detected. Image via NASA/ JPL-Caltech.

It was never going to harm us. Size estimates for objects of this kind are based upon the object’s observed brightness as seen from Earth. 2020 QG is thought to be about 10 to 20 feet (3 to 6 meters) across. That’s in contrast to the biggest asteroids, which are hundreds of miles across. And it’s in contrast to the small asteroid that created 2013’s famous Chelyabinsk meteor, which came even closer to us, entering Earth’s atmosphere over Russia. The Chelyabinsk meteor started out some 66 feet (20 meters) across. It created a gigantic shockwave that broke windows in six Russian cities, causing hundreds of injuries, mostly from flying glass. On the other hand, if an asteroid the size of 2020 QG does enter our atmosphere (and indeed they do, several times each year, according to NASA), the airburst it creates would be too high in Earth’s atmosphere to cause damage on the ground. What’s more, a 10- to 20-foot asteroid would either completely vaporize on its fall through the atmosphere, or drop as a small remnant of its former self – a rock from space, prized by meteorite hunters – onto Earth’s surface or into the ocean. So there was never any real danger of harm. In fact, astronomers appear to get a kick out of seeing tiny asteroids like 2020 QG come this close. Paul Chodas, director of NASA’s Center for Near Earth Object Studies, said in a NASA statement:

It’s really cool to see a small asteroid come by this close, because we can see the Earth’s gravity dramatically bend its trajectory. Our calculations show that this asteroid got turned by 45 degrees or so as it swung by our planet.

But what about that six-hour delay in astronomers’ detection of this asteroid? Cause for outrage? On the contrary …

A red circle around a short white line on a gray background spotted with white dots.

View larger. | The circled streak in the center of this image is asteroid 2020 QG. This image shows how the Zwicky Transient Facility noticed the asteroid – as a fast-moving streak in front of the stars – 6 hours after its closest approach. Image via ZTF/ Caltech Optical Observatories.

Astronomers’ ability to detect asteroids far exceeds what it was. Diminutive asteroids the size of 2020 QG have been sweeping past Earth for billions of years. An asteroid this size couldn’t have been detected at all a few decades ago. In our lifetimes, asteroid-detection technology has greatly advanced. 2020 QG was found via a survey telescope – the Zwicky Transient Facility (ZTF) – on Palomar Mountain in California. It was found by a robotic system developed by some of the smartest people on the planet, who, for decades, have been working to protect Earth from possible destructive asteroid impacts. Go astronomers!

However, 2020 QG’s sweep past Earth on Sunday does point to a weakness in astronomers’ highly developed asteroid-observing abilities. That is, it’s hard for them to see asteroids that come at us from the direction of the sun. Paul Chodas commented to Dave Mosher and Morgan McFall-Johnsen of Business Insider:

There’s not much we can do about detecting inbound asteroids coming from the sunward direction, as asteroids are detected using optical telescopes only (like ZTF), and we can only search for them in the night sky. The idea is that we discover them on one of their prior passages by our planet, and then make predictions years and decades in advance to see whether they have any possibility of impacting.

Mosher and McFall-Johnsen also reported:

NASA has a plan to address these gaps in its asteroid-hunting program. The agency is in the early stages of developing a space telescope that could detect asteroids and comets coming from the sun’s direction.

NASA’s 2020 budget allotted nearly $36 million for that telescope, called the Near-Earth Object Surveillance Mission.

If funding continues, it could launch as early as 2025.

NASA said that, by some estimates, there are hundreds of millions of tiny asteroids the size of 2020 QG. They are extremely hard to discover until they get very close to Earth. The vast majority pass by safely at greater distances, usually, but not always, farther away than our moon.

Meanwhile, in 2005, Congress assigned NASA the goal of finding 90% of the near-Earth asteroids that are about 460 feet (140 meters) or larger in size. Clearly, the larger asteroids pose a larger threat. The good news is that they they can be detected much farther away from Earth. Once found, their orbits can be calculated years into the future, to determine any potential for a future collision. If an asteroid were found to be on a collision course with Earth, assuming it were found years before the collision was due to take place, the world could and surely would take steps to try to divert it.

Bottom line: Asteroid ZTF0DxQ – now officially labeled 2020 QG – swept just 2,000 miles (3,000 km) from Earth’s surface, making it the closest-known asteroid flyby that didn’t involve a strike.

Via Business Insider

Via NASA



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

Researchers track slowly splitting ‘dent’ in Earth’s magnetic field

Earth’s magnetic field acts like a protective shield around the planet, repelling and trapping charged particles from the sun. But there’s an unusually weak spot in the field, a slowly expanding “dent” over South America and the southern Atlantic Ocean – called the South Atlantic Anomaly, or SAA – that allows these particles to dip closer to the surface than normal. The SAA developed as a result in changes to the motion of Earth’s core, according to an August 12, 2020, NASA statement.

Although the SAA arises from processes inside Earth, it has effects that reach far beyond Earth’s surface. Particle radiation in this region can knock out onboard computers and interfere with the data collection of satellites that pass through it. If a satellite is hit by a high-energy proton, it can short-circuit and cause an event called single event upset, or SEU. This can cause the satellite’s function to glitch temporarily or can cause permanent damage if a key component is hit. In order to avoid losing instruments or an entire satellite, operators commonly shut down non-essential components as they pass through the SAA.

And although the SAA currently creates no visible impacts on daily life on our planet’s surface, recent observations show that the region is expanding westward and continuing to weaken in intensity. It’s also splitting, say scientists. Recent data shows the anomaly’s valley, or region of minimum field strength, has split into two lobes, creating additional challenges for satellite missions.

Earth, with lines that arc from north to south poles.

This visualization shows a simple model of the Earth’s magnetic field. The magnetic field partially shields the Earth from harmful charged particles emanating from the sun. Image via NASA’s Goddard Space Flight Center.

The International Space Station (ISS), which is in low Earth orbit, also passes through the SAA. It is well protected, and astronauts are safe from harm while inside. However, the ISS has other passengers affected by the higher radiation levels: Instruments like the Global Ecosystem Dynamics Investigation mission, or GEDI, which collect data from various positions on the outside of the ISS. The SAA causes “blips” on GEDI’s detectors and resets the instrument’s power boards about once a month, said Bryan Blair, the mission’s deputy principal investigator and instrument scientist. Blair said:

These events cause no harm to GEDI. The detector blips are rare compared to the number of laser shots – about one blip in a million shots – and the reset line event causes a couple of hours of lost data, but it only happens every month or so.

Earth with fuzzy false-color donuts around it cut away to show their depth.

When solar material streams into Earth’s magnetosphere, it can become trapped and held in two donut-shaped belts around the planet called the Van Allen Belts. The belts restrain the particles to travel along Earth’s magnetic field lines, continually bouncing back and forth from pole to pole. Image via NASA Goddard/ Tom Bridgman.

A host of scientists in geomagnetic, geophysics, and heliophysics research groups observe and monitor the SAA to predict future changes, and help prepare for future challenges to satellites and humans in space. The South Atlantic Anomaly is also of interest to Earth scientists who monitor the changes in magnetic field strength there, both for how such changes affect Earth’s atmosphere and as an indicator of what’s happening to Earth’s magnetic fields deep inside the globe. Hear more from NASA scientists studying the SAA.

NASA geophysicist Terry Sabaka said in a statement:

Even though the SAA is slow-moving, it is going through some change in morphology [shape and structure], so it’s also important that we keep observing it by having continued missions. Because that’s what helps us make models and predictions.

Large sun on left, Earth in the middle surrounded by arc-shaped lines from pole to pole.

The sun expels a constant outflow of particles and magnetic fields, known as the solar wind, and vast clouds of hot plasma and radiation, called coronal mass ejections. This solar material streams across space and strikes Earth’s magnetosphere, the space occupied by Earth’s magnetic field, which acts like a protective shield around the planet. Image via NASA Goddard/ Bailee DesRocher.

Bottom line: Researchers are tracking a slowly splitting “dent” in Earth’s magnetic field, called the South Atlantic Anomaly or SAA.

Read more from NASA



from EarthSky https://ift.tt/3iT6e1n

Earth’s magnetic field acts like a protective shield around the planet, repelling and trapping charged particles from the sun. But there’s an unusually weak spot in the field, a slowly expanding “dent” over South America and the southern Atlantic Ocean – called the South Atlantic Anomaly, or SAA – that allows these particles to dip closer to the surface than normal. The SAA developed as a result in changes to the motion of Earth’s core, according to an August 12, 2020, NASA statement.

Although the SAA arises from processes inside Earth, it has effects that reach far beyond Earth’s surface. Particle radiation in this region can knock out onboard computers and interfere with the data collection of satellites that pass through it. If a satellite is hit by a high-energy proton, it can short-circuit and cause an event called single event upset, or SEU. This can cause the satellite’s function to glitch temporarily or can cause permanent damage if a key component is hit. In order to avoid losing instruments or an entire satellite, operators commonly shut down non-essential components as they pass through the SAA.

And although the SAA currently creates no visible impacts on daily life on our planet’s surface, recent observations show that the region is expanding westward and continuing to weaken in intensity. It’s also splitting, say scientists. Recent data shows the anomaly’s valley, or region of minimum field strength, has split into two lobes, creating additional challenges for satellite missions.

Earth, with lines that arc from north to south poles.

This visualization shows a simple model of the Earth’s magnetic field. The magnetic field partially shields the Earth from harmful charged particles emanating from the sun. Image via NASA’s Goddard Space Flight Center.

The International Space Station (ISS), which is in low Earth orbit, also passes through the SAA. It is well protected, and astronauts are safe from harm while inside. However, the ISS has other passengers affected by the higher radiation levels: Instruments like the Global Ecosystem Dynamics Investigation mission, or GEDI, which collect data from various positions on the outside of the ISS. The SAA causes “blips” on GEDI’s detectors and resets the instrument’s power boards about once a month, said Bryan Blair, the mission’s deputy principal investigator and instrument scientist. Blair said:

These events cause no harm to GEDI. The detector blips are rare compared to the number of laser shots – about one blip in a million shots – and the reset line event causes a couple of hours of lost data, but it only happens every month or so.

Earth with fuzzy false-color donuts around it cut away to show their depth.

When solar material streams into Earth’s magnetosphere, it can become trapped and held in two donut-shaped belts around the planet called the Van Allen Belts. The belts restrain the particles to travel along Earth’s magnetic field lines, continually bouncing back and forth from pole to pole. Image via NASA Goddard/ Tom Bridgman.

A host of scientists in geomagnetic, geophysics, and heliophysics research groups observe and monitor the SAA to predict future changes, and help prepare for future challenges to satellites and humans in space. The South Atlantic Anomaly is also of interest to Earth scientists who monitor the changes in magnetic field strength there, both for how such changes affect Earth’s atmosphere and as an indicator of what’s happening to Earth’s magnetic fields deep inside the globe. Hear more from NASA scientists studying the SAA.

NASA geophysicist Terry Sabaka said in a statement:

Even though the SAA is slow-moving, it is going through some change in morphology [shape and structure], so it’s also important that we keep observing it by having continued missions. Because that’s what helps us make models and predictions.

Large sun on left, Earth in the middle surrounded by arc-shaped lines from pole to pole.

The sun expels a constant outflow of particles and magnetic fields, known as the solar wind, and vast clouds of hot plasma and radiation, called coronal mass ejections. This solar material streams across space and strikes Earth’s magnetosphere, the space occupied by Earth’s magnetic field, which acts like a protective shield around the planet. Image via NASA Goddard/ Bailee DesRocher.

Bottom line: Researchers are tracking a slowly splitting “dent” in Earth’s magnetic field, called the South Atlantic Anomaly or SAA.

Read more from NASA



from EarthSky https://ift.tt/3iT6e1n

The team tackling the serious side effects of cancer treatment in an ageing population

By 2066, it’s predicted that around a quarter of the total UK population will be over 65 years old. A number approximately equivalent to the population of London.

This is in part due to increasing life expectancy, a result of progress made through medical research. But as life expectancy increases, an ageing population brings up a whole host of new challenges for healthcare, as we’ve blogged about before.

One of these problems is considering the side effects of cancer treatments, which can often be experienced more intensely by older patients.

We can see this with radiosensitisation, where additional treatment, such as small doses of chemotherapy, can be added to enhance the sensitivity of a tumour to radiotherapy.

But this comes at the cost of harmful side effects.

We caught up with Professor Anne Kiltie and PhD student, Chee Then, who are part of a team looking into the relationship between the gut microbiome and radiosensitisation in bladder cancer.

What is radiosensitisation?

A radiosensitiser can be thought of as an enhancer, an additional agent that increases the sensitivity of tumour cells to radiotherapy.

“So classically, radiotherapy was given on its own for any sort of tumour. And then people discovered that if you add a little bit of chemo at the same time as giving radiotherapy, , it acts locally to enhance the effects of the radiotherapy,” explains Kiltie.  

This is often the case for patients who are being treated for pelvic tumours including cervical, rectal and bladder cancers. The problem, Kiltie explains, is that the radiosensitising chemotherapy frequently results in increased toxicity in local organs and tissues, causing negative side effects.  

And these negative side effects may be too much for older people to cope with. Kiltie has witnessed this first-hand in her clinics. “The median age of my radiotherapy patients is about 81 to 82,” Kiltie explains, “and patients older than this end up having radiotherapy alone”.

So Kiltie and Then set out on the hunt for a radiosensitiser with reduced side effects, which led them to the gut.

Fibre consumption and the microbiome

The gut is one of the most widely researched parts of the body, but scientists are finding out eye-opening information about the gut and its unusual inhabitants every day.

More specifically, the trillions of bacteria, fungi and viruses that call the human body home, often called the microbiome.

The vibrant community of bugs can help protect us from harm, programming our immune system as well as providing nutrients for our cells. And it’s a real area of interest for cancer research.

Scientists, including our OPTIMISTICC Cancer Grand Challenges team, are interested in a whole host of possible links between the gut and cancer, from looking for cancer clues in poo, to discovering unique strains of bacteria that could act as a genetic marker for bowel cancer.

So far, changes to the gut microbiome enhancing anti-cancer treatment have only been explored in the context of chemotherapy and immunotherapy, “but there is not any study about radiotherapy and the gut microbiome,” says Then.

Because of its effect on the microbiome, scientists are also interested in the role that diet – particularly high fibre foods – can play in cancer. Previous studies have looked at how a high fibre diet has the capacity to reduce tumour growth, but haven’t looked explicitly at the mechanism behind how a high fibre diet could change the bacterial composition in the gut. 

Kiltie and her team wanted to explore this gap in the research by further examining the connection between the microbiome and radiotherapy.

Back to bacteria  

The lab focussed their work on mice with a compromised immune system and bladder cancer, who were fed a variety of fibre diets. “We treated the mice with either a low fibre diet, or a high soluble fibre or insoluble fibre diet or a mix of the two,” Then explains.

The team went on to analyse the composition of the gut microbiome of the different groups of mice, and how they responded to radiotherapy.

The team found that the mice fed with the high soluble fibre diet on average had the slowest tumour growth rate following small doses of radiotherapy.

Changes to fibre consumption can be seen almost immediately in the mice’s poo. With an indication of an increased amount of a short chain fatty acid known to confer anti-cancer effects, called butyrate.

Interestingly, and more unexpectedly, of the mice administered the high soluble fibre diet, those who responded to radiotherapy were enriched with a strain of bacterium known as Bacteroides acidifaciens. “A relatively newly-discovered bacterium, I suppose isolated in 2000,” Then comments.

The team believe the increase in the Bacteroides acidifaciens could be the missing link between the change in fibre consumption, short chain fatty acids and radiosensitisation. And that this bacterial strain plays a crucial role in the production of short chain fatty acids.

“So, the gut microbiota needs the fibre to produce short chain fatty acids and we think that this might be a potential radiosensitiser,” Then explains. 

Like Kiltie and Chee, Our Cancer Grand Challenges OPTIMISTICC team are also investigating correlations between the microbiome and treatment response. Some of their latest work has identified a bacterial strain which is associated with a higher chance of relapse of patients with rectal cancer who have been treated with chemotherapy.

From the lab to the clinic 

Kiltie and her team believe the proof is in the fibre. And it won’t take any expensive medicine to get this into practice, but repurposing of an existing treatment.

The team are looking into different types of fibre, including ispaghula husk. This is currently administered as a standard treatment for radiotherapy patients, but as a way to reduce diarrhoea.

Currently, patients “only start taking it halfway through their radiotherapy to help the side effects,” explains Kiltie. “But the argument is that the fibre can actually increase the short chain fatty acid production.”

The idea would be to get patients to take the fibre supplement before and during their radiotherapy to act as a radiosensitiser, whilst also reducing side effects. And most importantly, this would be something easily administered to older patients.

“The beauty of ispaghula husk, or whatever fibre supplement we end up giving, is it’s a medicine and old people take lots medicines and they’re generally pretty compliant,” says Kiltie. “To try and modify somebody’s diet is unlikely to work in a 78-year old, they’re probably going to say ‘no way’.” 

It’s early days, and the team have lots planned before they can trial it in humans, but the latest results are promising. “The idea has been kind of boiling, bubbling along for two or three years,” says Kiltie, “but to actually show something in the mice is really exciting.” 

Lilly

Reference

Then, C.K., Paillas, S., Wang, X. et al. (2020). ‘Association of Bacteroides acidifaciens relative abundance with high-fibre diet-associated radiosensitisation’. BMC Biol 18, 102. DOI: https://doi.org/10.1186/s12915-020-00836-x 

 



from Cancer Research UK – Science blog https://ift.tt/2FvgqPg

By 2066, it’s predicted that around a quarter of the total UK population will be over 65 years old. A number approximately equivalent to the population of London.

This is in part due to increasing life expectancy, a result of progress made through medical research. But as life expectancy increases, an ageing population brings up a whole host of new challenges for healthcare, as we’ve blogged about before.

One of these problems is considering the side effects of cancer treatments, which can often be experienced more intensely by older patients.

We can see this with radiosensitisation, where additional treatment, such as small doses of chemotherapy, can be added to enhance the sensitivity of a tumour to radiotherapy.

But this comes at the cost of harmful side effects.

We caught up with Professor Anne Kiltie and PhD student, Chee Then, who are part of a team looking into the relationship between the gut microbiome and radiosensitisation in bladder cancer.

What is radiosensitisation?

A radiosensitiser can be thought of as an enhancer, an additional agent that increases the sensitivity of tumour cells to radiotherapy.

“So classically, radiotherapy was given on its own for any sort of tumour. And then people discovered that if you add a little bit of chemo at the same time as giving radiotherapy, , it acts locally to enhance the effects of the radiotherapy,” explains Kiltie.  

This is often the case for patients who are being treated for pelvic tumours including cervical, rectal and bladder cancers. The problem, Kiltie explains, is that the radiosensitising chemotherapy frequently results in increased toxicity in local organs and tissues, causing negative side effects.  

And these negative side effects may be too much for older people to cope with. Kiltie has witnessed this first-hand in her clinics. “The median age of my radiotherapy patients is about 81 to 82,” Kiltie explains, “and patients older than this end up having radiotherapy alone”.

So Kiltie and Then set out on the hunt for a radiosensitiser with reduced side effects, which led them to the gut.

Fibre consumption and the microbiome

The gut is one of the most widely researched parts of the body, but scientists are finding out eye-opening information about the gut and its unusual inhabitants every day.

More specifically, the trillions of bacteria, fungi and viruses that call the human body home, often called the microbiome.

The vibrant community of bugs can help protect us from harm, programming our immune system as well as providing nutrients for our cells. And it’s a real area of interest for cancer research.

Scientists, including our OPTIMISTICC Cancer Grand Challenges team, are interested in a whole host of possible links between the gut and cancer, from looking for cancer clues in poo, to discovering unique strains of bacteria that could act as a genetic marker for bowel cancer.

So far, changes to the gut microbiome enhancing anti-cancer treatment have only been explored in the context of chemotherapy and immunotherapy, “but there is not any study about radiotherapy and the gut microbiome,” says Then.

Because of its effect on the microbiome, scientists are also interested in the role that diet – particularly high fibre foods – can play in cancer. Previous studies have looked at how a high fibre diet has the capacity to reduce tumour growth, but haven’t looked explicitly at the mechanism behind how a high fibre diet could change the bacterial composition in the gut. 

Kiltie and her team wanted to explore this gap in the research by further examining the connection between the microbiome and radiotherapy.

Back to bacteria  

The lab focussed their work on mice with a compromised immune system and bladder cancer, who were fed a variety of fibre diets. “We treated the mice with either a low fibre diet, or a high soluble fibre or insoluble fibre diet or a mix of the two,” Then explains.

The team went on to analyse the composition of the gut microbiome of the different groups of mice, and how they responded to radiotherapy.

The team found that the mice fed with the high soluble fibre diet on average had the slowest tumour growth rate following small doses of radiotherapy.

Changes to fibre consumption can be seen almost immediately in the mice’s poo. With an indication of an increased amount of a short chain fatty acid known to confer anti-cancer effects, called butyrate.

Interestingly, and more unexpectedly, of the mice administered the high soluble fibre diet, those who responded to radiotherapy were enriched with a strain of bacterium known as Bacteroides acidifaciens. “A relatively newly-discovered bacterium, I suppose isolated in 2000,” Then comments.

The team believe the increase in the Bacteroides acidifaciens could be the missing link between the change in fibre consumption, short chain fatty acids and radiosensitisation. And that this bacterial strain plays a crucial role in the production of short chain fatty acids.

“So, the gut microbiota needs the fibre to produce short chain fatty acids and we think that this might be a potential radiosensitiser,” Then explains. 

Like Kiltie and Chee, Our Cancer Grand Challenges OPTIMISTICC team are also investigating correlations between the microbiome and treatment response. Some of their latest work has identified a bacterial strain which is associated with a higher chance of relapse of patients with rectal cancer who have been treated with chemotherapy.

From the lab to the clinic 

Kiltie and her team believe the proof is in the fibre. And it won’t take any expensive medicine to get this into practice, but repurposing of an existing treatment.

The team are looking into different types of fibre, including ispaghula husk. This is currently administered as a standard treatment for radiotherapy patients, but as a way to reduce diarrhoea.

Currently, patients “only start taking it halfway through their radiotherapy to help the side effects,” explains Kiltie. “But the argument is that the fibre can actually increase the short chain fatty acid production.”

The idea would be to get patients to take the fibre supplement before and during their radiotherapy to act as a radiosensitiser, whilst also reducing side effects. And most importantly, this would be something easily administered to older patients.

“The beauty of ispaghula husk, or whatever fibre supplement we end up giving, is it’s a medicine and old people take lots medicines and they’re generally pretty compliant,” says Kiltie. “To try and modify somebody’s diet is unlikely to work in a 78-year old, they’re probably going to say ‘no way’.” 

It’s early days, and the team have lots planned before they can trial it in humans, but the latest results are promising. “The idea has been kind of boiling, bubbling along for two or three years,” says Kiltie, “but to actually show something in the mice is really exciting.” 

Lilly

Reference

Then, C.K., Paillas, S., Wang, X. et al. (2020). ‘Association of Bacteroides acidifaciens relative abundance with high-fibre diet-associated radiosensitisation’. BMC Biol 18, 102. DOI: https://doi.org/10.1186/s12915-020-00836-x 

 



from Cancer Research UK – Science blog https://ift.tt/2FvgqPg

A clear night over Georgia

Silhouette of a woman sitting atop a car, shining a flashlight at the sky, with the Milky Way in the background.

View at EarthSky Community Photos. | Scott Kuhn was at Fort Mountain in Georgia when he captured this single 10-second exposure on August 16, 2020. He wrote, “Finally a clear night in north Georgia, and the Milky Way was looking great!” By the way, in case you’re wondering about the horizon lights, Scott said there’s a dam below the mountain. Also, on this night, nearby city lights were illuminating some clouds from below. The bright object to the left of the Milky Way is Jupiter, and the fainter object to Jupiter’s left is Saturn. Thank you, Scott! Click here to view more photos Scott took that night.



from EarthSky https://ift.tt/348QyDg
Silhouette of a woman sitting atop a car, shining a flashlight at the sky, with the Milky Way in the background.

View at EarthSky Community Photos. | Scott Kuhn was at Fort Mountain in Georgia when he captured this single 10-second exposure on August 16, 2020. He wrote, “Finally a clear night in north Georgia, and the Milky Way was looking great!” By the way, in case you’re wondering about the horizon lights, Scott said there’s a dam below the mountain. Also, on this night, nearby city lights were illuminating some clouds from below. The bright object to the left of the Milky Way is Jupiter, and the fainter object to Jupiter’s left is Saturn. Thank you, Scott! Click here to view more photos Scott took that night.



from EarthSky https://ift.tt/348QyDg

The Teapot, 2 planets and the galaxy’s center

Every year in August – from either the Northern or Southern Hemisphere – you can look in the evening hours toward the center of our Milky Way galaxy. It’s located in the direction of the constellation Sagittarius the Archer, which happens to contain a famous asterism – or noticeable pattern of stars – called the Teapot. In 2020, there are two bright planets in this same direction in space. Jupiter is brighter than any star. Saturn is fainter than Jupiter, but still as bright as the brightest stars.

In 2020, the Teapot is found to the west of Jupiter and Saturn.

If you’re blessed with a dark sky, finding them all will be easy. In a dark sky, you’ll see a broad boulevard of stars – the edgewise view into our own Milky Way galaxy – which broadens and brightens in the direction of Teapot and the planets. From the Northern Hemisphere, you’ll be looking south around mid-to-late evening for Jupiter, Saturn and the Teapot. From the Southern Hemisphere, look closer to overhead.

Don’t know the planets and don’t have a dark sky? The chart below via AstroBob expands the view to include the constellation Scorpius, which is to the west of the Teapot. This pattern is relatively bright and easy to spot for its curved Scorpion’s Tail.

From the Northern Hemisphere, look southward in July and August evenings to see these stars. From the Southern Hemisphere, look generally northward, higher in the sky and turn this chart upside down. Chart via AstroBob.

Sagittarius the Archer – and its Teapot asterism – is next door to Scorpius on the sky’s dome. From the Northern Hemisphere, look southward on August and September evenings. From the Southern Hemisphere, look generally overhead or northward, higher in the sky and turn this chart upside down. Chart via AstroBob.

We can’t really see into the center of our Milky Way galaxy, which lies some 26,000 light-years away. The galactic center is heavily veiled by intervening stars, star clusters and nebulae (vast clouds of gas and dust). But – when we look toward the constellation Sagittarius – we are gazing toward the galactic center in space.

If your sky is dark enough, this direction in space is a sight to behold!

The Teapot asterism makes up the western half of the constellation Sagittarius the Archer. Modern eyes have an easier time envisioning a teapot than an Archer with a drawn-out bow. See the sky chart of Sagittarius below.

View larger. | The constellation Sagittarius, with the Teapot asterism outlined in green.

From temperate latitudes in the Northern Hemisphere, it’s pretty easy to make out the Summer Triangle asterism rather high in the eastern sky at nightfall. This huge star formation consists of three brilliant stars – Vega, Deneb and Altair – and can oftentimes withstand the glare of the full moon or light-polluted city. If you are otherwise lost on some starry night but can find the Summer Triangle, let this signpost star formation escort you to the Teapot …

View larger. | Great rift of Milky Way passes through the constellation Cassiopeia and the Summer Triangle. Draw an imaginary line from Deneb through Altair, going about twice the Deneb-Altair distance, to star-hop to the Teapot of Sagittarius

Bottom line: Try finding the Teapot asterism in the constellation Sagittarius the Archer. The center of our Milky Way galaxy is located in this direction of space. In 2020, you’ll also find two planets here, Jupiter and Saturn.

Read more: Sagittarius? Here’s your constellation



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

Every year in August – from either the Northern or Southern Hemisphere – you can look in the evening hours toward the center of our Milky Way galaxy. It’s located in the direction of the constellation Sagittarius the Archer, which happens to contain a famous asterism – or noticeable pattern of stars – called the Teapot. In 2020, there are two bright planets in this same direction in space. Jupiter is brighter than any star. Saturn is fainter than Jupiter, but still as bright as the brightest stars.

In 2020, the Teapot is found to the west of Jupiter and Saturn.

If you’re blessed with a dark sky, finding them all will be easy. In a dark sky, you’ll see a broad boulevard of stars – the edgewise view into our own Milky Way galaxy – which broadens and brightens in the direction of Teapot and the planets. From the Northern Hemisphere, you’ll be looking south around mid-to-late evening for Jupiter, Saturn and the Teapot. From the Southern Hemisphere, look closer to overhead.

Don’t know the planets and don’t have a dark sky? The chart below via AstroBob expands the view to include the constellation Scorpius, which is to the west of the Teapot. This pattern is relatively bright and easy to spot for its curved Scorpion’s Tail.

From the Northern Hemisphere, look southward in July and August evenings to see these stars. From the Southern Hemisphere, look generally northward, higher in the sky and turn this chart upside down. Chart via AstroBob.

Sagittarius the Archer – and its Teapot asterism – is next door to Scorpius on the sky’s dome. From the Northern Hemisphere, look southward on August and September evenings. From the Southern Hemisphere, look generally overhead or northward, higher in the sky and turn this chart upside down. Chart via AstroBob.

We can’t really see into the center of our Milky Way galaxy, which lies some 26,000 light-years away. The galactic center is heavily veiled by intervening stars, star clusters and nebulae (vast clouds of gas and dust). But – when we look toward the constellation Sagittarius – we are gazing toward the galactic center in space.

If your sky is dark enough, this direction in space is a sight to behold!

The Teapot asterism makes up the western half of the constellation Sagittarius the Archer. Modern eyes have an easier time envisioning a teapot than an Archer with a drawn-out bow. See the sky chart of Sagittarius below.

View larger. | The constellation Sagittarius, with the Teapot asterism outlined in green.

From temperate latitudes in the Northern Hemisphere, it’s pretty easy to make out the Summer Triangle asterism rather high in the eastern sky at nightfall. This huge star formation consists of three brilliant stars – Vega, Deneb and Altair – and can oftentimes withstand the glare of the full moon or light-polluted city. If you are otherwise lost on some starry night but can find the Summer Triangle, let this signpost star formation escort you to the Teapot …

View larger. | Great rift of Milky Way passes through the constellation Cassiopeia and the Summer Triangle. Draw an imaginary line from Deneb through Altair, going about twice the Deneb-Altair distance, to star-hop to the Teapot of Sagittarius

Bottom line: Try finding the Teapot asterism in the constellation Sagittarius the Archer. The center of our Milky Way galaxy is located in this direction of space. In 2020, you’ll also find two planets here, Jupiter and Saturn.

Read more: Sagittarius? Here’s your constellation



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

US lung cancer data points to the power of cancer research

Lung cancer cell

Whether it’s exams, a COVID-19 test or a mid-treatment scan, waiting for results can be nerve-wracking. The anxiety. The unknowns. The implications for the future. The growing sense of anticipation as the day looms. Will it be good news, or bad? 

This week, the whole of cancer research got some long-awaited results – and they’re a tentative thumbs-up. New data from the US National Cancer Institute (NCI), published in the New England Journal of Medicine, show the clearest signs yet that one of the most promising concepts in modern cancer medicine  targeted therapy – seems to be having an impact on one of the hardest cancers to treat: lung cancer. 

Long-term trends 

Lung cancer is the biggest cancer killer, claiming an estimated 1.76m lives each year around the globe. Thankfully, in many countries, the rate of people dying from the disease in the population has been gradually falling for several years. And although there have been some big changes in how the disease is diagnosed and treated over this time, the main thing driving the drop is the decline in smoking rates across the developed world, meaning fewer people are getting lung cancer. 

This is of course, extremely good news. But the huge influence smoking has on cancer rates has made it harder to unpick any underlying impact of treatment changes. A large US analysis looked at this back in January, and appeared to show a big drop in death rates from all cancers – which was initially lauded as proof that treatment was improving. But a closer look at the data revealed that other factors were at play – including the drop in smoking.  

The question of whether specific changes in treatment lead to population-level improvements in cancer outcomes is, of course, much more than an academic one. Over the decades, billions of pounds, dollars and euros have been invested in understanding cancer and developing new treatments. In the case of lung cancer, this has led to a whole slew of new therapies being approved in the last 5-10 years, and making their way into routine use – including in the UK 

Most prominent of these are the so-called ‘targeted’ therapies, designed to treat patients whose cancers are caused by particular DNA errors. After being proven effective in clinical trials, these drugs began to enter routine use in the early 2010s 

As a result, many researchers and organisations – including Cancer Research UK – have been keeping a keen eye on national and international cancer trends, looking for signs that this collective effort is having the ‘big picture’ impact that the positive trial results suggested they should.   

A not inconsiderable number of fingers have been crossed. 

Hitting the target? 

We’ve written before about the promise and challenges of targeted therapies – also referred to as ‘personalised’ or ‘precision’ medicines. Unlike conventional chemo drugs, theyre designed to interfere with specific processes within cancer cells, with the aim of more precisely targeting the disease 

Thanks to the help of our supporters, we’ve been able to play a key role in accelerating the development of these drugs. Our researchers have been at the forefront of tracking down molecular faults in cancer cells, and finding ways to target them. We’ve worked closely with pharma companies to help test experimental therapiesto bring those that are safe and effective to patients as swiftly as possible. And we’ve worked closely with the NHS, to ensure the necessary testing is available to patients, and regulators, to make sure their approval happens smoothly 

And yet, despite the hope and promise, lingering doubts remain.  

In trial settings, these drugs can offer only modest benefits – months rather than yearsThey are extremely expensive. So too is the testing infrastructure needed to use them effectively, and only about 1 in 5 patients has a relevant marker suggesting the drugs will work. As with chemotherapy, tumours can develop resistance to them. They cause side-effects – different side-effects to chemo for sure but, for many patients, no less debilitating. Many commentators have written about the ‘hype’ around these drugs, and wondered whether they might be a false, expensive dawn in the quest to beat cancer.  

The new analysis from the NCI begins to suggest otherwise.  

Promising new data 

This week’s new analysis draws on data from lung cancer patients diagnosed in the US between 2006 and 2016, and relies on the fact that the disease exists in several distinct forms. Two thirds are what’s known as ‘non small cell’ lung cancers, while just over a tenth are termed ‘small cell’ lung cancers. Both can be caused by smoking, but – crucially – targeted drugs have only been widely introduced for the former.  

These facts allowed the NCI’s researchers to compare lung cancer incidence and mortality for both forms, using data from the organisation’s massive national Surveillance, Epidemiology, and End Results (SEER) cancer registry. Any difference in trends, the researchers reasoned, would likely to be due to factors like treatment changes, rather than other ‘bigger picture’ factors like smoking or improved diagnosis. 

As expected, the analysis revealed that from 2006 mortality rates declined for both forms. But from 2013, the researchers spotted a big increase in the downward trend for patients with non-small cell lung cancer, which wasn’t apparent for those with small cell cancers.  

2013, of course, is when targeted therapies began to be used for non small cell lung cancer.  

The drop in mortality seemed to double, from 3% a year, to 6% a year. And when the researchers looked at 2-year survival data (the proportion of patients still alive two years after their diagnosis) this appeared to rise from about a quarter to over a third.  

That’s a big improvement, for a notoriously hard-to-treat cancer. And it’s wonderful news. 

But there are a few caveats. It’s not absolute ‘smoking gun’ proof that targeted therapies are behind the improvement – the SEER database doesn’t record which treatments a patient received, making the link an indirect one. Over the same time, there have also been incremental improvements in chemotherapy, radiotherapy and surgery. But many of these applied to both diseases, and the researchers were able to rule out many other factors, such as improvements in diagnosis leading to more cancers being diagnosed earlier, making their case extremely compelling.  

No room for complacency 

Despite this welcome news – in a type of cancer where progress has historically been slow – the study also highlights how much further we have to go to keep improving things for all patientsincluding those with non small cell lung cancers 

These drugs may be good – but they’re not good enough: they’re not cures, and they’re not suitable for everyone. Cancer, and lung cancer in particular, is a complex, rapidly evolving disease – so finding suitable drugs for more types (and subtypes) of cancer is going to be a long slogAnd, as our National Lung Matrix Trial results suggested last month, non small cell lung cancer’s low-hanging fruit may already have been plucked 

It will also be important to make sure that any new drugs are made available, and affordable, to all patients who need them. And just focusing on drugs certainly won’t be enough. Lung cancer can be curable in its early stages  we urgently need better ways to diagnose the disease early, to give people the best chance of long-term survival.  

Copy this link and share our graphic. Credit: Cancer Research UK

We know how much work is still to do, despite this week’s good news. 

But there is reason to be incredibly proud of your support for us. Those key lung cancer drugs introduced in 2013 are designed to target a molecule known as the epidermal growth factor receptor, or EGFRThis crucial molecule was discovered in the 1980s, by researchers at our London Research Institute – now part of the Francis Crick Institute 

None of this week’s good news would have been possible without that breakthrough 

And today, hundreds of researchers at the Crick, and around the country, are continuing to make discoveries that, we hope, will keep improving things for all people affected by cancer.  

And with COVID-19 having had such a big impact on charities like ours, your support has never been more valuable, nor more appreciated.  

Henry Scowcroft is Cancer Research UK’s communications strategy lead  



from Cancer Research UK – Science blog https://ift.tt/2FBaVPe
Lung cancer cell

Whether it’s exams, a COVID-19 test or a mid-treatment scan, waiting for results can be nerve-wracking. The anxiety. The unknowns. The implications for the future. The growing sense of anticipation as the day looms. Will it be good news, or bad? 

This week, the whole of cancer research got some long-awaited results – and they’re a tentative thumbs-up. New data from the US National Cancer Institute (NCI), published in the New England Journal of Medicine, show the clearest signs yet that one of the most promising concepts in modern cancer medicine  targeted therapy – seems to be having an impact on one of the hardest cancers to treat: lung cancer. 

Long-term trends 

Lung cancer is the biggest cancer killer, claiming an estimated 1.76m lives each year around the globe. Thankfully, in many countries, the rate of people dying from the disease in the population has been gradually falling for several years. And although there have been some big changes in how the disease is diagnosed and treated over this time, the main thing driving the drop is the decline in smoking rates across the developed world, meaning fewer people are getting lung cancer. 

This is of course, extremely good news. But the huge influence smoking has on cancer rates has made it harder to unpick any underlying impact of treatment changes. A large US analysis looked at this back in January, and appeared to show a big drop in death rates from all cancers – which was initially lauded as proof that treatment was improving. But a closer look at the data revealed that other factors were at play – including the drop in smoking.  

The question of whether specific changes in treatment lead to population-level improvements in cancer outcomes is, of course, much more than an academic one. Over the decades, billions of pounds, dollars and euros have been invested in understanding cancer and developing new treatments. In the case of lung cancer, this has led to a whole slew of new therapies being approved in the last 5-10 years, and making their way into routine use – including in the UK 

Most prominent of these are the so-called ‘targeted’ therapies, designed to treat patients whose cancers are caused by particular DNA errors. After being proven effective in clinical trials, these drugs began to enter routine use in the early 2010s 

As a result, many researchers and organisations – including Cancer Research UK – have been keeping a keen eye on national and international cancer trends, looking for signs that this collective effort is having the ‘big picture’ impact that the positive trial results suggested they should.   

A not inconsiderable number of fingers have been crossed. 

Hitting the target? 

We’ve written before about the promise and challenges of targeted therapies – also referred to as ‘personalised’ or ‘precision’ medicines. Unlike conventional chemo drugs, theyre designed to interfere with specific processes within cancer cells, with the aim of more precisely targeting the disease 

Thanks to the help of our supporters, we’ve been able to play a key role in accelerating the development of these drugs. Our researchers have been at the forefront of tracking down molecular faults in cancer cells, and finding ways to target them. We’ve worked closely with pharma companies to help test experimental therapiesto bring those that are safe and effective to patients as swiftly as possible. And we’ve worked closely with the NHS, to ensure the necessary testing is available to patients, and regulators, to make sure their approval happens smoothly 

And yet, despite the hope and promise, lingering doubts remain.  

In trial settings, these drugs can offer only modest benefits – months rather than yearsThey are extremely expensive. So too is the testing infrastructure needed to use them effectively, and only about 1 in 5 patients has a relevant marker suggesting the drugs will work. As with chemotherapy, tumours can develop resistance to them. They cause side-effects – different side-effects to chemo for sure but, for many patients, no less debilitating. Many commentators have written about the ‘hype’ around these drugs, and wondered whether they might be a false, expensive dawn in the quest to beat cancer.  

The new analysis from the NCI begins to suggest otherwise.  

Promising new data 

This week’s new analysis draws on data from lung cancer patients diagnosed in the US between 2006 and 2016, and relies on the fact that the disease exists in several distinct forms. Two thirds are what’s known as ‘non small cell’ lung cancers, while just over a tenth are termed ‘small cell’ lung cancers. Both can be caused by smoking, but – crucially – targeted drugs have only been widely introduced for the former.  

These facts allowed the NCI’s researchers to compare lung cancer incidence and mortality for both forms, using data from the organisation’s massive national Surveillance, Epidemiology, and End Results (SEER) cancer registry. Any difference in trends, the researchers reasoned, would likely to be due to factors like treatment changes, rather than other ‘bigger picture’ factors like smoking or improved diagnosis. 

As expected, the analysis revealed that from 2006 mortality rates declined for both forms. But from 2013, the researchers spotted a big increase in the downward trend for patients with non-small cell lung cancer, which wasn’t apparent for those with small cell cancers.  

2013, of course, is when targeted therapies began to be used for non small cell lung cancer.  

The drop in mortality seemed to double, from 3% a year, to 6% a year. And when the researchers looked at 2-year survival data (the proportion of patients still alive two years after their diagnosis) this appeared to rise from about a quarter to over a third.  

That’s a big improvement, for a notoriously hard-to-treat cancer. And it’s wonderful news. 

But there are a few caveats. It’s not absolute ‘smoking gun’ proof that targeted therapies are behind the improvement – the SEER database doesn’t record which treatments a patient received, making the link an indirect one. Over the same time, there have also been incremental improvements in chemotherapy, radiotherapy and surgery. But many of these applied to both diseases, and the researchers were able to rule out many other factors, such as improvements in diagnosis leading to more cancers being diagnosed earlier, making their case extremely compelling.  

No room for complacency 

Despite this welcome news – in a type of cancer where progress has historically been slow – the study also highlights how much further we have to go to keep improving things for all patientsincluding those with non small cell lung cancers 

These drugs may be good – but they’re not good enough: they’re not cures, and they’re not suitable for everyone. Cancer, and lung cancer in particular, is a complex, rapidly evolving disease – so finding suitable drugs for more types (and subtypes) of cancer is going to be a long slogAnd, as our National Lung Matrix Trial results suggested last month, non small cell lung cancer’s low-hanging fruit may already have been plucked 

It will also be important to make sure that any new drugs are made available, and affordable, to all patients who need them. And just focusing on drugs certainly won’t be enough. Lung cancer can be curable in its early stages  we urgently need better ways to diagnose the disease early, to give people the best chance of long-term survival.  

Copy this link and share our graphic. Credit: Cancer Research UK

We know how much work is still to do, despite this week’s good news. 

But there is reason to be incredibly proud of your support for us. Those key lung cancer drugs introduced in 2013 are designed to target a molecule known as the epidermal growth factor receptor, or EGFRThis crucial molecule was discovered in the 1980s, by researchers at our London Research Institute – now part of the Francis Crick Institute 

None of this week’s good news would have been possible without that breakthrough 

And today, hundreds of researchers at the Crick, and around the country, are continuing to make discoveries that, we hope, will keep improving things for all people affected by cancer.  

And with COVID-19 having had such a big impact on charities like ours, your support has never been more valuable, nor more appreciated.  

Henry Scowcroft is Cancer Research UK’s communications strategy lead  



from Cancer Research UK – Science blog https://ift.tt/2FBaVPe

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