EPA “Aim High” Success Stories on Climate and Air Quality

By Administrator Gina McCarthy

The public health case for climate action is compelling beyond words. The interagency Climate and Health Assessment released last month confirms that climate change endangers our health by affecting our food and water sources, the weather we experience, and the air we breathe. And we know that it will exacerbate certain health threats that already exist – while also creating new ones.

As we celebrate the recent signing of the historic Paris Agreement by countries around the world, there’s no better time to reflect on EPA’s many ongoing efforts to fight climate change and protect the air we breathe.

As part of our “Aim High” effort to highlight success stories from across the agency, I asked EPA staff to share examples of their work to protect public health by taking action on climate and air quality. Here are some highlights:

Child with pinwheel and blue sky in the background.Asthma Awareness Month: Asthma affects nearly 23 million Americans and disproportionally impacts low-income and minority communities. In the U.S., the direct medical costs of asthma and indirect costs, such as missed school and work days, amount to over $50 billion a year. Every May, EPA leads a National Asthma Awareness Campaign to increase public awareness about asthma risks, strengthen partnerships with community-based asthma organizations, and recognize exceptional asthma programs that are making a difference. Every year, this effort reaches 9,000 groups and individuals and provides them with the information and motivation to take action.

Group photo of employees from EPA and the Ghana Environmental Protection Agency .U.S EPA Africa Megacity Partnership: EPA’s environmental program in sub-Saharan Africa is focused on addressing the region’s growing urban and industrial pollution issues, including air quality and indoor air from cookstoves. The World Health Organization estimates that exposure to smoke from cooking causes 4.3 million premature deaths per year. EPA and the Ghana Environmental Protection Agency are working together under the Africa Megacities Partnership to develop an integrated air quality action plan for Accra. As a result of this partnership, Ghana EPA has already made significant progress using air quality monitoring and analysis and is serving as a model for other African cities with limited data, that want to take action.

Group of people by reservoir impacted by drought.Climate Change and Water Utilities: Between 1980 and 2015, the United States was impacted by more than 20 major droughts, each costing over one billion dollars. EPA staff in the Office of Water developed an easy-to-use guide to assist small- to medium-sized water utilities with responding to drought. The Drought Response and Recovery Guide for Water Utilities, release last month, includes best practices, implementation examples and customizable worksheets that help states and communities set short-term/emergency action plans, while also building long-term resilience to drought. EPA staff also developed an interactive drought case study map that tells the story of how seven diverse small- to medium-sized utilities in California, Texas, Georgia, New Mexico, Kansas, and Oklahoma were challenged by drought impacts and were able to successfully respond to and recover from drought.

Screenshot of EPA Region 1 Valley Indication Tool.Outreach on Risks from Wood Smoke: Exposure to particle pollution from wood smoke has been linked to a number of adverse health effects. Valleys in New England, where terrain and meteorology contribute to poor dispersion of pollutants, are especially vulnerable during winter air inversions. EPA Region 1 used publically available study results, databases and in-house Geographic Information System resources to develop “The Valley Identification Tool” that identifies populated valleys throughout New England that are at risk for wood-smoke pollution. Using this tool, EPA and state air quality managers and staff can better plan air-quality monitoring, outreach, and mitigation.

Biogas facilityBiogas to Energy: Water Resource Recovery Facilities (WRRFs) help recover water, nutrients, and energy from wastewater. EPA Region 9 is working with WRRFs to boost energy production through the addition of non-traditional organic wastes ranging from municipally collected food scraps to the byproducts of food processing facilities and agricultural production. As a result of these efforts, some of these facilities are becoming “energy positive,” producing enough energy to power the facility and transferring excess energy into the electricity grid for use by others. EPA, in collaboration with universities and industry, is also working to collect and share information on co-digestion practices and biogas management technologies. This work helps improve understanding of the air quality impacts of biogas-to-energy technologies and helps state and local governments, regulators, and developers identify cleaner, geographically-appropriate and cost-effective biogas management options.



from The EPA Blog http://ift.tt/1QNczW5

By Administrator Gina McCarthy

The public health case for climate action is compelling beyond words. The interagency Climate and Health Assessment released last month confirms that climate change endangers our health by affecting our food and water sources, the weather we experience, and the air we breathe. And we know that it will exacerbate certain health threats that already exist – while also creating new ones.

As we celebrate the recent signing of the historic Paris Agreement by countries around the world, there’s no better time to reflect on EPA’s many ongoing efforts to fight climate change and protect the air we breathe.

As part of our “Aim High” effort to highlight success stories from across the agency, I asked EPA staff to share examples of their work to protect public health by taking action on climate and air quality. Here are some highlights:

Child with pinwheel and blue sky in the background.Asthma Awareness Month: Asthma affects nearly 23 million Americans and disproportionally impacts low-income and minority communities. In the U.S., the direct medical costs of asthma and indirect costs, such as missed school and work days, amount to over $50 billion a year. Every May, EPA leads a National Asthma Awareness Campaign to increase public awareness about asthma risks, strengthen partnerships with community-based asthma organizations, and recognize exceptional asthma programs that are making a difference. Every year, this effort reaches 9,000 groups and individuals and provides them with the information and motivation to take action.

Group photo of employees from EPA and the Ghana Environmental Protection Agency .U.S EPA Africa Megacity Partnership: EPA’s environmental program in sub-Saharan Africa is focused on addressing the region’s growing urban and industrial pollution issues, including air quality and indoor air from cookstoves. The World Health Organization estimates that exposure to smoke from cooking causes 4.3 million premature deaths per year. EPA and the Ghana Environmental Protection Agency are working together under the Africa Megacities Partnership to develop an integrated air quality action plan for Accra. As a result of this partnership, Ghana EPA has already made significant progress using air quality monitoring and analysis and is serving as a model for other African cities with limited data, that want to take action.

Group of people by reservoir impacted by drought.Climate Change and Water Utilities: Between 1980 and 2015, the United States was impacted by more than 20 major droughts, each costing over one billion dollars. EPA staff in the Office of Water developed an easy-to-use guide to assist small- to medium-sized water utilities with responding to drought. The Drought Response and Recovery Guide for Water Utilities, release last month, includes best practices, implementation examples and customizable worksheets that help states and communities set short-term/emergency action plans, while also building long-term resilience to drought. EPA staff also developed an interactive drought case study map that tells the story of how seven diverse small- to medium-sized utilities in California, Texas, Georgia, New Mexico, Kansas, and Oklahoma were challenged by drought impacts and were able to successfully respond to and recover from drought.

Screenshot of EPA Region 1 Valley Indication Tool.Outreach on Risks from Wood Smoke: Exposure to particle pollution from wood smoke has been linked to a number of adverse health effects. Valleys in New England, where terrain and meteorology contribute to poor dispersion of pollutants, are especially vulnerable during winter air inversions. EPA Region 1 used publically available study results, databases and in-house Geographic Information System resources to develop “The Valley Identification Tool” that identifies populated valleys throughout New England that are at risk for wood-smoke pollution. Using this tool, EPA and state air quality managers and staff can better plan air-quality monitoring, outreach, and mitigation.

Biogas facilityBiogas to Energy: Water Resource Recovery Facilities (WRRFs) help recover water, nutrients, and energy from wastewater. EPA Region 9 is working with WRRFs to boost energy production through the addition of non-traditional organic wastes ranging from municipally collected food scraps to the byproducts of food processing facilities and agricultural production. As a result of these efforts, some of these facilities are becoming “energy positive,” producing enough energy to power the facility and transferring excess energy into the electricity grid for use by others. EPA, in collaboration with universities and industry, is also working to collect and share information on co-digestion practices and biogas management technologies. This work helps improve understanding of the air quality impacts of biogas-to-energy technologies and helps state and local governments, regulators, and developers identify cleaner, geographically-appropriate and cost-effective biogas management options.



from The EPA Blog http://ift.tt/1QNczW5

Video: Mars and Saturn in 2016

Opposition of Mars and Saturn for 2016 in the Constellations of Libra and Scorpius from Larry Koehn on Vimeo.

Larry Koehn at the beautiful website shadowandsubstance.com created this video, which shows the 2016 oppositions of Mars and Saturn and tracks their motions on our sky’s dome from January to September. He’s showing the planets not as they would appear to the eye, but as a telescope would show them. He wrote:

Opposition occurs when a planet is in line with the Earth and the sun. This year, Mars will be at opposition on May 22 followed by Saturn on June 3. Opposition of a planet also means the planet can be seen all night long from sunset to sunrise. Mars this year will come close as 47 million miles to Earth in May.

Yes, it will be an excellent opposition of Mars this year!

Click here to learn more about Mars’ 2016 opposition.

And here are some things to notice about this video:

1. Notice that – when they are at opposition around late May and early June – Mars and Saturn appear close together on our sky’s dome. In fact, they’re already close together on the sky’s dome, as you’ll notice if you look at the chart below. It makes sense, because their oppositions in 2016 take place so near each other in time.

2. Notice that, as Larry shows in the video, Mars grows apparently larger around its late May opposition. That’s because, as he said, opposition takes place when a planet is in line with the Earth and sun. It happens when Earth goes between that planet and the sun. Mars is the next planet outward in orbit around the sun. It’s nearer to us in space than Saturn, and, at opposition, it’s especially near. That’s why Mars will appear so large in our sky – as seen through a telescope – around its May 22, 2016, opposition.

3. Notice that – by tracking these worlds on our sky’s dome from January to September of this year – he’s also portraying the retrograde loops of the planets, which begin and end with each planet’s stationary point (marked in the video) in our sky.

Read more: What is retrograde motion?

How can you identify Mars and Saturn? They are up late at night now and easily seen before dawn. They’re rising earlier each evening and – in late May and early June – will be visible in the east just after sunset, and all night long.

A good time to start watching them would be in late March, when the moon will sweep past them. See the chart below.

Watch the moon move past the planets Mars and Saturn, plus the star Antares over the next several mornings. The moon swings to the north of the December solstice point on March 30. The green line depicts the ecliptic - Earth's orbital plane projected onto the constellations of the Zodiac.

Watch the moon move past the planets Mars and Saturn, plus the star Antares, in late March. The green line depicts the ecliptic – the sun’s path across our sky.

Bottom line: Mars will reach opposition on May 22, and Saturn on June 3. As a result, they now appear near each other in our sky. This video from Larry Koehn at shadowandsubstance.com tracks their motion on our sky’s from January to September, 2016.

Mars oppositions 2010 – 2022



from EarthSky http://ift.tt/21Jgj1a

Opposition of Mars and Saturn for 2016 in the Constellations of Libra and Scorpius from Larry Koehn on Vimeo.

Larry Koehn at the beautiful website shadowandsubstance.com created this video, which shows the 2016 oppositions of Mars and Saturn and tracks their motions on our sky’s dome from January to September. He’s showing the planets not as they would appear to the eye, but as a telescope would show them. He wrote:

Opposition occurs when a planet is in line with the Earth and the sun. This year, Mars will be at opposition on May 22 followed by Saturn on June 3. Opposition of a planet also means the planet can be seen all night long from sunset to sunrise. Mars this year will come close as 47 million miles to Earth in May.

Yes, it will be an excellent opposition of Mars this year!

Click here to learn more about Mars’ 2016 opposition.

And here are some things to notice about this video:

1. Notice that – when they are at opposition around late May and early June – Mars and Saturn appear close together on our sky’s dome. In fact, they’re already close together on the sky’s dome, as you’ll notice if you look at the chart below. It makes sense, because their oppositions in 2016 take place so near each other in time.

2. Notice that, as Larry shows in the video, Mars grows apparently larger around its late May opposition. That’s because, as he said, opposition takes place when a planet is in line with the Earth and sun. It happens when Earth goes between that planet and the sun. Mars is the next planet outward in orbit around the sun. It’s nearer to us in space than Saturn, and, at opposition, it’s especially near. That’s why Mars will appear so large in our sky – as seen through a telescope – around its May 22, 2016, opposition.

3. Notice that – by tracking these worlds on our sky’s dome from January to September of this year – he’s also portraying the retrograde loops of the planets, which begin and end with each planet’s stationary point (marked in the video) in our sky.

Read more: What is retrograde motion?

How can you identify Mars and Saturn? They are up late at night now and easily seen before dawn. They’re rising earlier each evening and – in late May and early June – will be visible in the east just after sunset, and all night long.

A good time to start watching them would be in late March, when the moon will sweep past them. See the chart below.

Watch the moon move past the planets Mars and Saturn, plus the star Antares over the next several mornings. The moon swings to the north of the December solstice point on March 30. The green line depicts the ecliptic - Earth's orbital plane projected onto the constellations of the Zodiac.

Watch the moon move past the planets Mars and Saturn, plus the star Antares, in late March. The green line depicts the ecliptic – the sun’s path across our sky.

Bottom line: Mars will reach opposition on May 22, and Saturn on June 3. As a result, they now appear near each other in our sky. This video from Larry Koehn at shadowandsubstance.com tracks their motion on our sky’s from January to September, 2016.

Mars oppositions 2010 – 2022



from EarthSky http://ift.tt/21Jgj1a

Follow the arc to star Arcturus in May

Now is the perfect time to look outside in the evening and learn a phrase useful to sky watchers. The phrase is: follow the arc to Arcturus.

First locate the Big Dipper asterism in the northeastern sky. Then draw an imaginary line following the curve in the Dipper’s handle until you come to a bright orange star. This star is Arcturus in the constellation Bootes, known in skylore as the bear guard.

Arcturus is a much larger star than our sun. Read more about Arcturus here.

Enjoying EarthSky so far? Sign up for our free daily newsletter today!

Arcturus is a giant star with an estimated distance of 37 light-years. It’s special because it’s not moving with the general stream of stars, in the flat disk of the Milky Way galaxy. Instead, Arcturus is cutting perpendicularly through the galaxy’s disk at a tremendous rate of speed … some 150 kilometers per second. Millions of years from now this star will be lost from the view of any future inhabitants of Earth, or at least those who are earthbound and looking with the eye alone.

So that’s how to “follow the arc” to the star Arcturus in the constellation Bootes. Learn how you can drive a spike to the star Spica – and the planet Mars – in the constellation Virgo with the help of tomorrow’s sky chart.


Big and Little Dippers: Noticeable in northern sky

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

Donate: Your support means the world to us



from EarthSky http://ift.tt/1lLgQgD

Now is the perfect time to look outside in the evening and learn a phrase useful to sky watchers. The phrase is: follow the arc to Arcturus.

First locate the Big Dipper asterism in the northeastern sky. Then draw an imaginary line following the curve in the Dipper’s handle until you come to a bright orange star. This star is Arcturus in the constellation Bootes, known in skylore as the bear guard.

Arcturus is a much larger star than our sun. Read more about Arcturus here.

Enjoying EarthSky so far? Sign up for our free daily newsletter today!

Arcturus is a giant star with an estimated distance of 37 light-years. It’s special because it’s not moving with the general stream of stars, in the flat disk of the Milky Way galaxy. Instead, Arcturus is cutting perpendicularly through the galaxy’s disk at a tremendous rate of speed … some 150 kilometers per second. Millions of years from now this star will be lost from the view of any future inhabitants of Earth, or at least those who are earthbound and looking with the eye alone.

So that’s how to “follow the arc” to the star Arcturus in the constellation Bootes. Learn how you can drive a spike to the star Spica – and the planet Mars – in the constellation Virgo with the help of tomorrow’s sky chart.


Big and Little Dippers: Noticeable in northern sky

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

Donate: Your support means the world to us



from EarthSky http://ift.tt/1lLgQgD

Sayer Ji: Willfully misunderstanding overdiagnosis and misdiagnosis since…forever [Respectful Insolence]

If there’s one lesson that I like to emphasize while laying down my near-daily dose of Insolence, both Respectful and not-so-Respectful, it’s that practicing medicine and surgery is complicated. Part of the reason that it’s complicated is that for many diseases our understanding is incomplete, meaning that physicians have to apply existing science to their treatment as well as they can in the context of incomplete information and understanding. The biology of cancer, in particular, can be vexing. Some cancers appear to progress relentlessly, meaning that it’s obvious that all of them must be treated. Others, particularly when detected in their very early stages through screening tests, have a variable and therefore difficult-to-predict clinical course if left untreated. Unfortunately, some people, such as a man whom I consider to be a promoter of dangerous quackery, Sayer Ji, either can’t or won’t understand that. They like their medicine black and white, and if physicians ever change guidelines in order to align them more closely with newer scientific understanding, they write blisteringly ignorant articles like “‘Oops… It Wasn’t Cancer After All,’ Admits The National Cancer Institute/JAMA.”

Not exactly. What really happened is that an expert panel recommended reclassifying a specific thyroid lesion as not cancerous based on recent science. It’s called medicine correcting itself. Admittedly, this reclassification was probably long overdue, but what would Mr. Ji rather have? Medicine not correcting itself in this situation? In any case, when last I met Mr. Ji, he was gleefully abusing the science of genetics to argue that Angelina Jolie and other carriers of deleterious cancer-causing mutations don’t need prophylactic surgery because lifestyle interventions will save them through epigenetics, which to “natural health” enthusiasts like Mr. Ji seems to mean the magical ability to prevent any disease. Most recently, he has appeared on the deeply dishonest “documentary” about alternative medicine cancer cures, The Truth About Cancer, to expound on how chemotherapy is evil. His rant about the reclassification of a non-encapsulated follicular variant of papillary thyroid cancer as not cancer is more of the same, as you will see.

Overdiagnosis and the question of what is and isn’t “cancer”?

The sort of issue mangled by Mr. Ji in his article is one that those of us who treat breast cancer have been dealing with for a long time now. For example, as a breast cancer surgeon, I deal all the time with a disease entity known as ductal carcinoma in situ (DCIS). Basically, it’s a condition in which cancerous-appearing cells are found in the milk ducts of the breast but have not crossed the basement membrane, which surrounds the milk ducts. Generally, we consider DCIS to be stage 0 breast cancer, specifically cancer that hasn’t invaded through the basement membrane into the breast yet. Of course, as I’ve written before many times, it’s not as simple as that. Many—probably most—DCIS lesions never progress to cancer in the patient’s lifetime, particularly the so-called low grade lesions, which are called low grade because their cells resemble normal milk duct cells. On the other hand, higher grade lesions, which look more like frank cancer, likely progress to cancer at a much higher rate. However, because we have no reliable means of predicting which DCIS lesions will progress to invasive cancer and which will not, we end up treating them all in basically the same way: surgical excision plus or minus (usually plus) radiation plus or minus an estrogen-blocking drug.

Confusing the question of treatment of very early stage breast cancer is the apparent massive increase in incidence of DCIS over the last 40 years. Basically, as I’ve described multiple times before, the incidence of DCIS has increased 16-fold since 1975. Given that it’s highly implausible and unlikely that the “true” incidence of DCIS has increased so markedly in such a short time (and three or four decades is a short time for a change this massive), the likely explanation is the institution of widespread mammographic screening programs beginning in the early 1980s, leading to overdiagnosis.

Overdiagnosis is a phenomenon that’s been discussed here many times. Basically, it is the detection of disease that would never go on to harm or kill the person harboring it. If there’s one thing that the mass screening of large asymptomatic populations for diseases has taught us, it’s that there’s a lot more preclinical disease out there in healthy people than we had previously suspected, or, as I put it, if you look very hard for a condition you will find more of it. Always. Indeed, thanks to a mass thyroid screening program after the Fukushima nuclear disaster, we recently learned that even children have way more preclinical thyroid cancer than we had previously thought. As I’ve discussed before, in autopsy studies half of men over 65 and three-quarters of men over 80 have tiny foci of cancer in their prostates; thyroid cancer can be found in 36% of adults, and the study’s investigators estimated that if the slices had been made thinly enough for microscopic examination they could have “found” thyroid cancer in close to 100% of adults between 50-70, even though clinically apparent thyroid cancer requiring treatment only has a prevalence in the population studied of around 0.1%. In breast cancer, it has been estimated that as many as one in three mammographically detected cancers in otherwise asymptomatic women might be overdiagnosed, although other estimates are around 10%. The reason the estimates vary so much is that we can’t do a study in which mammographically detected small invasive breast cancers are not treated is because, even if these estimates are correct, most of them do appear to progress. We’re thus forced to rely on inferences from epidemiological studies. Whatever the true number is, given that there are 240,000 new cases of breast cancer diagnosed every year, overdiagnosis is a huge problem, no matter how much some physicians would try to claim otherwise.

Once we acknowledge the existence of overdiagnosis, the questions then become:

  • Does the disease found at such an early, asymptomatic stage need to be treated?
  • Will treating the disease earlier, before it becomes symptomatic, lead to improved outcomes in terms of survival and/or morbidity?
  • Are these early lesions actually cancer?

The answers to these questions are not straightforward in the least, particularly given how difficult it is to show a survival benefit due to early intervention, thanks to lead time bias and length bias. It is this accumulation of evidence of overdiagnosis that has led to a rethinking of cancer screening and changes in recommended screening guidelines. They’re also leading scientists and physicians to reexamine the classification of cancerous-appearing lesions formerly classified as cancer:

In fact, said Dr. Otis Brawley, chief medical officer at the American Cancer Society, the name changes that occurred went in the opposite direction, scientific evidence to the contrary. Premalignant tiny lumps in the breast became known as stage zero cancer. Small and early-stage prostate lesions were called cancerous tumors. Meanwhile, imaging with ultrasound, M.R.I.’s and C.T. scans find more and more of these tiny “cancers,” especially thyroid nodules.

“If it’s not a cancer, let’s not call it a cancer,” said Dr. John C. Morris, president-elect of the American Thyroid Association and a professor of medicine at the Mayo Clinic. Dr. Morris was not a member of the renaming panel.

Dr. Barnett S. Kramer, director of the division of cancer prevention at the National Cancer Institute, said, “There’s a growing concern that many of the terms we use don’t match our understanding of the biology of cancer.” Calling lesions cancer when they are not leads to unnecessary and harmful treatment, he said.

Exactly. It is entirely rational and scientific to adjust medical nomenclature to reflect more recent science and understanding of disease. Again, doing so is anything but simple, as there will always be disagreements, and, yes, turf wars and fears among some physicians who treat these early lesions of losing business, but just because the renaming process is messy and contentious doesn’t mean there is nefarious intent to it or that there was nefarious intent in the nomenclature being replaced.

Reclassifying thyroid cancer

Mr. Ji, of course, is not interested in any of the complexities briefly touched on above. Rather, he is interested in vilifying “conventional” medicine:

Back in 2012, The National Cancer Institute convened an expert panel to evaluate the problem of cancer’s misclassification and subsequent overdiagnosis and overtreatment, determining that millions may have been wrongly diagnosed with “cancer” of the breast, prostate, thyroid, and lung, when in fact their conditions were likely harmless, and should have been termed “indolent or benign growths of epithelial origin.” No apology was issued. No major media coverage occurred. And more importantly, no radical change occurred in the conventional practice of cancer diagnosis, prevention, or treatment.

No major media coverage? Seriously? Besides Medscape, The Wall Street Journal covered it. So did The New York Times. I remember several stories about it in the national media, including television, at the time. Since then, there’s been a lot of coverage of the scientific controversy about overdiagnosis, particularly due to mammographic screening, in the national and international press. Perhaps Mr. Ji’s memory is faulty, which is why I am glad I was able to help jog it.

In any case, the summary to which Mr. Ji refers in his introductory rant is this article published in JAMA in 2013 by Laura Esserman (a breast surgeon whose work I admire) and colleagues. It summarized the NCI panel’s recommendations thusly:

  1. Physicians, patients, and the general public must recognize that overdiagnosis is common and occurs more frequently with cancer screening.
  2. Change cancer terminology based on companion diagnostics.
  3. Create observational registries for low malignant potential lesions.
  4. Mitigate overdiagnosis.
  5. Expand the concept of how to approach cancer progression.

Esserman et al concluded:

The original intent of screening was to detect cancer at the earliest stages to improve outcomes; however, detection of cancers with better biology contributes to better outcomes. Screening always results in identifying more indolent disease. Although no physician has the intention to overtreat or overdiagnose cancer, screening and patient awareness have increased the chance of identifying a spectrum of cancers, some of which are not life threatening. Policies that prevent or reduce the chance of overdiagnosis and avoid overtreatment are needed, while maintaining those gains by which early detection is a major contributor to decreasing mortality and locally advanced disease. The recommendations of the task force are intended as initial approaches. Physicians and patients should engage in open discussion about these complex issues. The media should better understand and communicate the message so that as a community the approach to screening can be improved.

In this light, it is easy to see how utterly silly Mr. Ji’s rant is. The task forces’ recommendations were meant as a starting point for discussion, not a pronouncement. Moreover, one could very much view the reclassification of a variant of thyroid cancer as not being malignant as addressing recommendations #2, 4, and 5. Indeed, this is the first time a lesion that had been classified as a cancer has been reclassified as not cancer.

Let’s take a look at the actual study.

When is thyroid cancer not cancer?

The relevant study, whose first author is Yuri E. Nikiforov, vice chairman of the pathology department at the University of Pittsburgh, basically tells you what you need to know: “Nomenclature Revision for Encapsulated Follicular Variant of Papillary Thyroid Carcinoma: A Paradigm Shift to Reduce Overtreatment of Indolent Tumors.” There it is right there in the title: This study is addressing recommendations #2 and 4 (at minimum) from the NCI workshop. In fact, it says right in the introduction that that was the purpose of this study! In essence, this paper lays out the case for changing the nomenclature of “encapsulated follicular variant of papillary thyroid carcinoma” (EFVPTC), which is generally treated like thyroid cancer now, to call these lesions “noninvasive follicular thyroid neoplasm with papillary-like nuclear features” (NIFTP). As I’ve discussed before, with the widespread use of thyroid ultrasound, overdiagnosis of indolent thyroid cancers has become a major problem, with large increases in the incidence of these lesions being reported, including noninvasive EFVPTC.

What the authors did was an international, multidisciplinary, retrospective study of patients with thyroid nodules diagnosed as EFVPTC, including 109 patients with noninvasive EFVPTC observed for 10 to 26 years and 101 patients with invasive EFVPTC observed for 1 to 18 years. Noninvasive EFVPTC included EFVPTC that had not invaded through its capsule. Twenty-four pathologists making up the Endocrine Pathology Society working group developed consensus criteria for the diagnosis of EFVPTC, and these were applied to the pathology slides. Molecular analysis of the tumors was also carried out using using ThyroSeq v2, which looks at a panel of 14 oncogenes for mutations.

The authors observed that none of the patients with noninvasive EFVPTC died of their disease in the follow-up period, while five of the patients with EFVPTC developed metastatic disease and two died. Genetic analysis of the lesions showed that noninvasive EFVPTC was predominately driven by mutations in the RAS oncogene, which are associated with follicular thyroid cancer, as opposed to the mutations in invasive EFVPTC, which were driven by BRAF and RET rearrangements, which have classically been associated with papillary thyroid cancer. On the basis of these observations and a review of the literature the authors recommended their proposed name change and listed rigorous, reproducible diagnostic criteria they propose for differentiating EFVPTC from NIFTP. Because approximately 20% of thyroid cancer is EFVPTC, this name change could affect up to 45,000 patients worldwide per year.

The authors conclude:

The results of this study, together with previously reported observations, suggest that when the diagnosis of NIFTP is made on the basis of careful histopathological examination, the tumor will have a low recurrence rate, likely less than 1% within the first 15 years. Of note, most differentiated thyroid carcinomas relapse within the first decade after initial therapy, although late recurrences and distant spread are documented. Importantly, a large proportion of patients with tumors diagnosed as NIFTP in the present study underwent lobectomy only and none received RAI [radioiodine] ablation. This suggests that clinical management of patients with NIFTP can be deescalated because they are unlikely to benefit from immediate completion thyroidectomy and RAI therapy. Staging would be unnecessary. In addition to eliminating the psychological impact of the diagnosis of cancer, this would reduce complications of total thyroidectomy, risk of secondary tumors following RAI therapy, and the overall cost of health care. Avoidance of RAI treatment alone would save between $5000 and $8500 per patient (based on US cost). Decreased long-term surveillance would account for another substantial proportion of cost reduction.

In other words, for this lesion, taking the involved thyroid lobe (or even perhaps just excising the lesion) is probably enough treatment. No completion total thyroidectomy would be necessary, nor would radioactive iodine or follow-up tests to screen for recurrence. The need for lifelong thyroid hormone supplementation would be eliminated in most patients because they would not require a total thyroidectomy.

Where do we go from here?

As hard as it is to come to a science-based agreement on a set of diagnostic guidelines and a reclassification of a disease entity, where the rubber hits the road will be how these recommendations will be viewed by practicing physicians. It’s reassuring to learn that eight leading professional societies have signed on to the new classification and the new name. That will definitely help with the adoption of the new classification and nomenclature, but it won’t be enough. As I’ve pointed out before, change in medicine is slower than we would like in some areas. We’ve learned that lesson from the Choosing Wisely program, and as the co-director of a statewide quality consortium I’ve learned that implementing change is complex and difficult, and that the wrong kind of change is often too easy to implement.

Practice is also changing to reflect these new realities. For example, men with low grade prostate cancers now often undergo “watchful waiting,” with no intervention unless the tumors progress. (Indeed, I know someone whose treatment involved just that. Unfortunately, he ultimately required radiation therapy, but that was because his tumor progressed.) In breast cancer treatment, recommendations are now less aggressive. For instance, in women over 70 with well-differentiated hormone receptor-positive cancers, radiation is now no longer routinely recommended. Our treatments have become more targeted, as well. For another example, there is the OncoType assay that measures the expression of 21 genes to predict whether women with hormone receptor-positive breast cancers with negative lymph nodes require chemotherapy, resulting in less chemotherapy being given; and this is only one of several such assays.

Indeed, it’s funny how Mr. Ji fails to note that, in this case, Dr. Nikiforov is basically going back to do what Mr. Ji thinks he should do: Let the patients previously treated as though they had cancer know that they didn’t. From a New York Times story on the change:

Dr. Nikiforov says he owes it to patients with reclassified tumors to tell them they never had cancer after all. At the University of Pittsburgh Medical Center, he and others are going to start reviewing medical records and pathology reports to identify previous patients and contact them. He estimates there have been about 50 to 100 each year at the medical center. They no longer have to go back for checkups. They lose the shadow of cancer that the diagnosis hung over their lives.

Informing these patients, Dr. Nikiforov said, “is a moral obligation of doctors.”

Indeed it is. In fact, this reclassification of EFVPTC as NIFTP is arguably the first fruit of the NCI recommendations that Mr. Ji keeps pointing to that actually involved renaming a disease entity. It’s not the first fruit of those recommendations, however. The ACS recommendations for mammographic screening are another. However, renaming disease entities is more difficult in other cancers because the delineation is not so clear-cut. There is no doubt that DCIS can progress to cancer at a substantial rate; the same is true for a lot of other early lesions classified as cancer that might be candidates for a name change, such as prostate cancer. Indeed, when doctors proposed doing just what the NCI proposed for early prostate cancers, there was a great deal of push-back—and not just from physicians. Great care and weighing a huge body of evidence, some of it contradictory, will be required, and it is taking years, as anyone who knew anything about the issues involved in 2012, when the NCI conference occurred, knew it would.

Of course, Mr. Ji isn’t about the careful weighing of evidence. He is about attacking “conventional” medicine and using the “science was wrong before” trope to try to claim that he was right all along and, by implication, he must be right about the “natural” treatments for cancer that he promotes on his website. Even then, he doesn’t understand:

Another topic I have been trying to spread awareness about is thyroid cancer overdiagnosis and overtreatment. When I first reported on this two years ago in my article, Thyroid Cancer Epidemic Caused by Misinformation, Not Cancer, a series of compelling studies from around the world revealed that the rapid increase in diagnoses in thyroid cancer reflected their misclassification and misdiagnosis. As was the case with screening detected breast and prostate “cancers,” and even many ovarian “cancers,” the standard of care often required the removal of the organ, as well as irradiation and chemotherapy — two known cancer promoting interventions.

Actually, overdiagnosis does not involve misdiagnosis. The two are not the same thing. A breast cancer picked up on screening mammography is a breast cancer. Its cells look just as malignant as cells from cancers picked up when a lump forms. The same is true for prostate cancer and, yes, most thyroid cancers. Remember, it’s not just the cancers being reclassified here that are being overdiagnosed by the widespread use of thyroid ultrasound. The real issue is that over the last decade we are learning that many of these cancers are indolent and would never harm the patient if left alone; the problem, of course, is figuring out which are dangerous and which can be either be safely watched or be adequately treated by excision alone. Dr. Nikiforov’s team’s work addresses exactly that question: Which cancers don’t need aggressive treatment? A side benefit of his work is that he identified a variant of thyroid cancer that is so indolent that it basically never metastasizes and therefore shouldn’t be called cancer.

It is useful in these situations to compare alternative medicine to science-based medicine. Those of us advocating for SBM realize its shortcomings better than most, and at least as well as Mr. Ji. We also actively work to change areas where conventional medical care is not adequately science-based. Indeed, this proposed reclassification of a type of thyroid cancer came about because a physician looked at medical practice and saw something not science-based:

The reclassification drive began two years ago when Dr. Yuri E. Nikiforov, vice chairman of the pathology department at the University of Pittsburgh, was asked his opinion about a small thyroid tumor in a 19-year-old woman. It was completely encased in a capsule and the lobe of her thyroid containing it had been removed to establish a diagnosis.

Over the last decade, Dr. Nikiforov had watched as pathologists began classifying noninvasive tumors as cancers and attributed the change to rare cases in which patients had a tumor that had broken out of its capsule, did not receive aggressive treatment and died of thyroid cancer. Worried doctors began treating all tumors composed of cells with nuclei that looked like cancer nuclei as if they were cancers. But this young woman’s story drove Dr. Nikiforov over the edge.

“I told the surgeon, who was a good friend, ‘This is a very low grade tumor. You do not have to do anything else.’ ” But the surgeon replied that according to practice guidelines, she had to remove the woman’s entire thyroid gland and treat her with radioactive iodine. And the woman had to have regular checkups for the rest of her life.

“I said, ‘That’s enough. Someone has to take responsibility and stop this madness,’ ” Dr. Nikiforov said.

It’s doctors like Dr. Nikiforov who see a medical practice that is not adequately science-based and fix it, not quacks like Mr. Ji, whose main interests in cancer seem to be to convince you that chemotherapy kills and causes far more harm than untreated cancer (wrong), that patients with cancer-causing gene mutations don’t need surgery (wrong), and that natural lifestyle changes and whatever supplements he likes can prevent cancer through the magic of epigenetics (wrong again). He latches on to examples like the reclassification of thyroid cancer of SBM correcting itself as evidence that conventional medicine is hopelessly flawed not because he wants to improve medical practice, but because he wants to substitute pseudoscience for science and non-evidence-based “alternative” treatments for validated science-based treatments. Doctors, like Dr. Nikiforov, who promote evidence-based practice are not a validation of Mr. Ji’s profoundly misguided beliefs.



from ScienceBlogs http://ift.tt/1SHNJsJ

If there’s one lesson that I like to emphasize while laying down my near-daily dose of Insolence, both Respectful and not-so-Respectful, it’s that practicing medicine and surgery is complicated. Part of the reason that it’s complicated is that for many diseases our understanding is incomplete, meaning that physicians have to apply existing science to their treatment as well as they can in the context of incomplete information and understanding. The biology of cancer, in particular, can be vexing. Some cancers appear to progress relentlessly, meaning that it’s obvious that all of them must be treated. Others, particularly when detected in their very early stages through screening tests, have a variable and therefore difficult-to-predict clinical course if left untreated. Unfortunately, some people, such as a man whom I consider to be a promoter of dangerous quackery, Sayer Ji, either can’t or won’t understand that. They like their medicine black and white, and if physicians ever change guidelines in order to align them more closely with newer scientific understanding, they write blisteringly ignorant articles like “‘Oops… It Wasn’t Cancer After All,’ Admits The National Cancer Institute/JAMA.”

Not exactly. What really happened is that an expert panel recommended reclassifying a specific thyroid lesion as not cancerous based on recent science. It’s called medicine correcting itself. Admittedly, this reclassification was probably long overdue, but what would Mr. Ji rather have? Medicine not correcting itself in this situation? In any case, when last I met Mr. Ji, he was gleefully abusing the science of genetics to argue that Angelina Jolie and other carriers of deleterious cancer-causing mutations don’t need prophylactic surgery because lifestyle interventions will save them through epigenetics, which to “natural health” enthusiasts like Mr. Ji seems to mean the magical ability to prevent any disease. Most recently, he has appeared on the deeply dishonest “documentary” about alternative medicine cancer cures, The Truth About Cancer, to expound on how chemotherapy is evil. His rant about the reclassification of a non-encapsulated follicular variant of papillary thyroid cancer as not cancer is more of the same, as you will see.

Overdiagnosis and the question of what is and isn’t “cancer”?

The sort of issue mangled by Mr. Ji in his article is one that those of us who treat breast cancer have been dealing with for a long time now. For example, as a breast cancer surgeon, I deal all the time with a disease entity known as ductal carcinoma in situ (DCIS). Basically, it’s a condition in which cancerous-appearing cells are found in the milk ducts of the breast but have not crossed the basement membrane, which surrounds the milk ducts. Generally, we consider DCIS to be stage 0 breast cancer, specifically cancer that hasn’t invaded through the basement membrane into the breast yet. Of course, as I’ve written before many times, it’s not as simple as that. Many—probably most—DCIS lesions never progress to cancer in the patient’s lifetime, particularly the so-called low grade lesions, which are called low grade because their cells resemble normal milk duct cells. On the other hand, higher grade lesions, which look more like frank cancer, likely progress to cancer at a much higher rate. However, because we have no reliable means of predicting which DCIS lesions will progress to invasive cancer and which will not, we end up treating them all in basically the same way: surgical excision plus or minus (usually plus) radiation plus or minus an estrogen-blocking drug.

Confusing the question of treatment of very early stage breast cancer is the apparent massive increase in incidence of DCIS over the last 40 years. Basically, as I’ve described multiple times before, the incidence of DCIS has increased 16-fold since 1975. Given that it’s highly implausible and unlikely that the “true” incidence of DCIS has increased so markedly in such a short time (and three or four decades is a short time for a change this massive), the likely explanation is the institution of widespread mammographic screening programs beginning in the early 1980s, leading to overdiagnosis.

Overdiagnosis is a phenomenon that’s been discussed here many times. Basically, it is the detection of disease that would never go on to harm or kill the person harboring it. If there’s one thing that the mass screening of large asymptomatic populations for diseases has taught us, it’s that there’s a lot more preclinical disease out there in healthy people than we had previously suspected, or, as I put it, if you look very hard for a condition you will find more of it. Always. Indeed, thanks to a mass thyroid screening program after the Fukushima nuclear disaster, we recently learned that even children have way more preclinical thyroid cancer than we had previously thought. As I’ve discussed before, in autopsy studies half of men over 65 and three-quarters of men over 80 have tiny foci of cancer in their prostates; thyroid cancer can be found in 36% of adults, and the study’s investigators estimated that if the slices had been made thinly enough for microscopic examination they could have “found” thyroid cancer in close to 100% of adults between 50-70, even though clinically apparent thyroid cancer requiring treatment only has a prevalence in the population studied of around 0.1%. In breast cancer, it has been estimated that as many as one in three mammographically detected cancers in otherwise asymptomatic women might be overdiagnosed, although other estimates are around 10%. The reason the estimates vary so much is that we can’t do a study in which mammographically detected small invasive breast cancers are not treated is because, even if these estimates are correct, most of them do appear to progress. We’re thus forced to rely on inferences from epidemiological studies. Whatever the true number is, given that there are 240,000 new cases of breast cancer diagnosed every year, overdiagnosis is a huge problem, no matter how much some physicians would try to claim otherwise.

Once we acknowledge the existence of overdiagnosis, the questions then become:

  • Does the disease found at such an early, asymptomatic stage need to be treated?
  • Will treating the disease earlier, before it becomes symptomatic, lead to improved outcomes in terms of survival and/or morbidity?
  • Are these early lesions actually cancer?

The answers to these questions are not straightforward in the least, particularly given how difficult it is to show a survival benefit due to early intervention, thanks to lead time bias and length bias. It is this accumulation of evidence of overdiagnosis that has led to a rethinking of cancer screening and changes in recommended screening guidelines. They’re also leading scientists and physicians to reexamine the classification of cancerous-appearing lesions formerly classified as cancer:

In fact, said Dr. Otis Brawley, chief medical officer at the American Cancer Society, the name changes that occurred went in the opposite direction, scientific evidence to the contrary. Premalignant tiny lumps in the breast became known as stage zero cancer. Small and early-stage prostate lesions were called cancerous tumors. Meanwhile, imaging with ultrasound, M.R.I.’s and C.T. scans find more and more of these tiny “cancers,” especially thyroid nodules.

“If it’s not a cancer, let’s not call it a cancer,” said Dr. John C. Morris, president-elect of the American Thyroid Association and a professor of medicine at the Mayo Clinic. Dr. Morris was not a member of the renaming panel.

Dr. Barnett S. Kramer, director of the division of cancer prevention at the National Cancer Institute, said, “There’s a growing concern that many of the terms we use don’t match our understanding of the biology of cancer.” Calling lesions cancer when they are not leads to unnecessary and harmful treatment, he said.

Exactly. It is entirely rational and scientific to adjust medical nomenclature to reflect more recent science and understanding of disease. Again, doing so is anything but simple, as there will always be disagreements, and, yes, turf wars and fears among some physicians who treat these early lesions of losing business, but just because the renaming process is messy and contentious doesn’t mean there is nefarious intent to it or that there was nefarious intent in the nomenclature being replaced.

Reclassifying thyroid cancer

Mr. Ji, of course, is not interested in any of the complexities briefly touched on above. Rather, he is interested in vilifying “conventional” medicine:

Back in 2012, The National Cancer Institute convened an expert panel to evaluate the problem of cancer’s misclassification and subsequent overdiagnosis and overtreatment, determining that millions may have been wrongly diagnosed with “cancer” of the breast, prostate, thyroid, and lung, when in fact their conditions were likely harmless, and should have been termed “indolent or benign growths of epithelial origin.” No apology was issued. No major media coverage occurred. And more importantly, no radical change occurred in the conventional practice of cancer diagnosis, prevention, or treatment.

No major media coverage? Seriously? Besides Medscape, The Wall Street Journal covered it. So did The New York Times. I remember several stories about it in the national media, including television, at the time. Since then, there’s been a lot of coverage of the scientific controversy about overdiagnosis, particularly due to mammographic screening, in the national and international press. Perhaps Mr. Ji’s memory is faulty, which is why I am glad I was able to help jog it.

In any case, the summary to which Mr. Ji refers in his introductory rant is this article published in JAMA in 2013 by Laura Esserman (a breast surgeon whose work I admire) and colleagues. It summarized the NCI panel’s recommendations thusly:

  1. Physicians, patients, and the general public must recognize that overdiagnosis is common and occurs more frequently with cancer screening.
  2. Change cancer terminology based on companion diagnostics.
  3. Create observational registries for low malignant potential lesions.
  4. Mitigate overdiagnosis.
  5. Expand the concept of how to approach cancer progression.

Esserman et al concluded:

The original intent of screening was to detect cancer at the earliest stages to improve outcomes; however, detection of cancers with better biology contributes to better outcomes. Screening always results in identifying more indolent disease. Although no physician has the intention to overtreat or overdiagnose cancer, screening and patient awareness have increased the chance of identifying a spectrum of cancers, some of which are not life threatening. Policies that prevent or reduce the chance of overdiagnosis and avoid overtreatment are needed, while maintaining those gains by which early detection is a major contributor to decreasing mortality and locally advanced disease. The recommendations of the task force are intended as initial approaches. Physicians and patients should engage in open discussion about these complex issues. The media should better understand and communicate the message so that as a community the approach to screening can be improved.

In this light, it is easy to see how utterly silly Mr. Ji’s rant is. The task forces’ recommendations were meant as a starting point for discussion, not a pronouncement. Moreover, one could very much view the reclassification of a variant of thyroid cancer as not being malignant as addressing recommendations #2, 4, and 5. Indeed, this is the first time a lesion that had been classified as a cancer has been reclassified as not cancer.

Let’s take a look at the actual study.

When is thyroid cancer not cancer?

The relevant study, whose first author is Yuri E. Nikiforov, vice chairman of the pathology department at the University of Pittsburgh, basically tells you what you need to know: “Nomenclature Revision for Encapsulated Follicular Variant of Papillary Thyroid Carcinoma: A Paradigm Shift to Reduce Overtreatment of Indolent Tumors.” There it is right there in the title: This study is addressing recommendations #2 and 4 (at minimum) from the NCI workshop. In fact, it says right in the introduction that that was the purpose of this study! In essence, this paper lays out the case for changing the nomenclature of “encapsulated follicular variant of papillary thyroid carcinoma” (EFVPTC), which is generally treated like thyroid cancer now, to call these lesions “noninvasive follicular thyroid neoplasm with papillary-like nuclear features” (NIFTP). As I’ve discussed before, with the widespread use of thyroid ultrasound, overdiagnosis of indolent thyroid cancers has become a major problem, with large increases in the incidence of these lesions being reported, including noninvasive EFVPTC.

What the authors did was an international, multidisciplinary, retrospective study of patients with thyroid nodules diagnosed as EFVPTC, including 109 patients with noninvasive EFVPTC observed for 10 to 26 years and 101 patients with invasive EFVPTC observed for 1 to 18 years. Noninvasive EFVPTC included EFVPTC that had not invaded through its capsule. Twenty-four pathologists making up the Endocrine Pathology Society working group developed consensus criteria for the diagnosis of EFVPTC, and these were applied to the pathology slides. Molecular analysis of the tumors was also carried out using using ThyroSeq v2, which looks at a panel of 14 oncogenes for mutations.

The authors observed that none of the patients with noninvasive EFVPTC died of their disease in the follow-up period, while five of the patients with EFVPTC developed metastatic disease and two died. Genetic analysis of the lesions showed that noninvasive EFVPTC was predominately driven by mutations in the RAS oncogene, which are associated with follicular thyroid cancer, as opposed to the mutations in invasive EFVPTC, which were driven by BRAF and RET rearrangements, which have classically been associated with papillary thyroid cancer. On the basis of these observations and a review of the literature the authors recommended their proposed name change and listed rigorous, reproducible diagnostic criteria they propose for differentiating EFVPTC from NIFTP. Because approximately 20% of thyroid cancer is EFVPTC, this name change could affect up to 45,000 patients worldwide per year.

The authors conclude:

The results of this study, together with previously reported observations, suggest that when the diagnosis of NIFTP is made on the basis of careful histopathological examination, the tumor will have a low recurrence rate, likely less than 1% within the first 15 years. Of note, most differentiated thyroid carcinomas relapse within the first decade after initial therapy, although late recurrences and distant spread are documented. Importantly, a large proportion of patients with tumors diagnosed as NIFTP in the present study underwent lobectomy only and none received RAI [radioiodine] ablation. This suggests that clinical management of patients with NIFTP can be deescalated because they are unlikely to benefit from immediate completion thyroidectomy and RAI therapy. Staging would be unnecessary. In addition to eliminating the psychological impact of the diagnosis of cancer, this would reduce complications of total thyroidectomy, risk of secondary tumors following RAI therapy, and the overall cost of health care. Avoidance of RAI treatment alone would save between $5000 and $8500 per patient (based on US cost). Decreased long-term surveillance would account for another substantial proportion of cost reduction.

In other words, for this lesion, taking the involved thyroid lobe (or even perhaps just excising the lesion) is probably enough treatment. No completion total thyroidectomy would be necessary, nor would radioactive iodine or follow-up tests to screen for recurrence. The need for lifelong thyroid hormone supplementation would be eliminated in most patients because they would not require a total thyroidectomy.

Where do we go from here?

As hard as it is to come to a science-based agreement on a set of diagnostic guidelines and a reclassification of a disease entity, where the rubber hits the road will be how these recommendations will be viewed by practicing physicians. It’s reassuring to learn that eight leading professional societies have signed on to the new classification and the new name. That will definitely help with the adoption of the new classification and nomenclature, but it won’t be enough. As I’ve pointed out before, change in medicine is slower than we would like in some areas. We’ve learned that lesson from the Choosing Wisely program, and as the co-director of a statewide quality consortium I’ve learned that implementing change is complex and difficult, and that the wrong kind of change is often too easy to implement.

Practice is also changing to reflect these new realities. For example, men with low grade prostate cancers now often undergo “watchful waiting,” with no intervention unless the tumors progress. (Indeed, I know someone whose treatment involved just that. Unfortunately, he ultimately required radiation therapy, but that was because his tumor progressed.) In breast cancer treatment, recommendations are now less aggressive. For instance, in women over 70 with well-differentiated hormone receptor-positive cancers, radiation is now no longer routinely recommended. Our treatments have become more targeted, as well. For another example, there is the OncoType assay that measures the expression of 21 genes to predict whether women with hormone receptor-positive breast cancers with negative lymph nodes require chemotherapy, resulting in less chemotherapy being given; and this is only one of several such assays.

Indeed, it’s funny how Mr. Ji fails to note that, in this case, Dr. Nikiforov is basically going back to do what Mr. Ji thinks he should do: Let the patients previously treated as though they had cancer know that they didn’t. From a New York Times story on the change:

Dr. Nikiforov says he owes it to patients with reclassified tumors to tell them they never had cancer after all. At the University of Pittsburgh Medical Center, he and others are going to start reviewing medical records and pathology reports to identify previous patients and contact them. He estimates there have been about 50 to 100 each year at the medical center. They no longer have to go back for checkups. They lose the shadow of cancer that the diagnosis hung over their lives.

Informing these patients, Dr. Nikiforov said, “is a moral obligation of doctors.”

Indeed it is. In fact, this reclassification of EFVPTC as NIFTP is arguably the first fruit of the NCI recommendations that Mr. Ji keeps pointing to that actually involved renaming a disease entity. It’s not the first fruit of those recommendations, however. The ACS recommendations for mammographic screening are another. However, renaming disease entities is more difficult in other cancers because the delineation is not so clear-cut. There is no doubt that DCIS can progress to cancer at a substantial rate; the same is true for a lot of other early lesions classified as cancer that might be candidates for a name change, such as prostate cancer. Indeed, when doctors proposed doing just what the NCI proposed for early prostate cancers, there was a great deal of push-back—and not just from physicians. Great care and weighing a huge body of evidence, some of it contradictory, will be required, and it is taking years, as anyone who knew anything about the issues involved in 2012, when the NCI conference occurred, knew it would.

Of course, Mr. Ji isn’t about the careful weighing of evidence. He is about attacking “conventional” medicine and using the “science was wrong before” trope to try to claim that he was right all along and, by implication, he must be right about the “natural” treatments for cancer that he promotes on his website. Even then, he doesn’t understand:

Another topic I have been trying to spread awareness about is thyroid cancer overdiagnosis and overtreatment. When I first reported on this two years ago in my article, Thyroid Cancer Epidemic Caused by Misinformation, Not Cancer, a series of compelling studies from around the world revealed that the rapid increase in diagnoses in thyroid cancer reflected their misclassification and misdiagnosis. As was the case with screening detected breast and prostate “cancers,” and even many ovarian “cancers,” the standard of care often required the removal of the organ, as well as irradiation and chemotherapy — two known cancer promoting interventions.

Actually, overdiagnosis does not involve misdiagnosis. The two are not the same thing. A breast cancer picked up on screening mammography is a breast cancer. Its cells look just as malignant as cells from cancers picked up when a lump forms. The same is true for prostate cancer and, yes, most thyroid cancers. Remember, it’s not just the cancers being reclassified here that are being overdiagnosed by the widespread use of thyroid ultrasound. The real issue is that over the last decade we are learning that many of these cancers are indolent and would never harm the patient if left alone; the problem, of course, is figuring out which are dangerous and which can be either be safely watched or be adequately treated by excision alone. Dr. Nikiforov’s team’s work addresses exactly that question: Which cancers don’t need aggressive treatment? A side benefit of his work is that he identified a variant of thyroid cancer that is so indolent that it basically never metastasizes and therefore shouldn’t be called cancer.

It is useful in these situations to compare alternative medicine to science-based medicine. Those of us advocating for SBM realize its shortcomings better than most, and at least as well as Mr. Ji. We also actively work to change areas where conventional medical care is not adequately science-based. Indeed, this proposed reclassification of a type of thyroid cancer came about because a physician looked at medical practice and saw something not science-based:

The reclassification drive began two years ago when Dr. Yuri E. Nikiforov, vice chairman of the pathology department at the University of Pittsburgh, was asked his opinion about a small thyroid tumor in a 19-year-old woman. It was completely encased in a capsule and the lobe of her thyroid containing it had been removed to establish a diagnosis.

Over the last decade, Dr. Nikiforov had watched as pathologists began classifying noninvasive tumors as cancers and attributed the change to rare cases in which patients had a tumor that had broken out of its capsule, did not receive aggressive treatment and died of thyroid cancer. Worried doctors began treating all tumors composed of cells with nuclei that looked like cancer nuclei as if they were cancers. But this young woman’s story drove Dr. Nikiforov over the edge.

“I told the surgeon, who was a good friend, ‘This is a very low grade tumor. You do not have to do anything else.’ ” But the surgeon replied that according to practice guidelines, she had to remove the woman’s entire thyroid gland and treat her with radioactive iodine. And the woman had to have regular checkups for the rest of her life.

“I said, ‘That’s enough. Someone has to take responsibility and stop this madness,’ ” Dr. Nikiforov said.

It’s doctors like Dr. Nikiforov who see a medical practice that is not adequately science-based and fix it, not quacks like Mr. Ji, whose main interests in cancer seem to be to convince you that chemotherapy kills and causes far more harm than untreated cancer (wrong), that patients with cancer-causing gene mutations don’t need surgery (wrong), and that natural lifestyle changes and whatever supplements he likes can prevent cancer through the magic of epigenetics (wrong again). He latches on to examples like the reclassification of thyroid cancer of SBM correcting itself as evidence that conventional medicine is hopelessly flawed not because he wants to improve medical practice, but because he wants to substitute pseudoscience for science and non-evidence-based “alternative” treatments for validated science-based treatments. Doctors, like Dr. Nikiforov, who promote evidence-based practice are not a validation of Mr. Ji’s profoundly misguided beliefs.



from ScienceBlogs http://ift.tt/1SHNJsJ

Sunday Chess Problem [EvolutionBlog]

It’s been a busy few weeks. I hosted a Passover seder. (What? Atheists can’t have seders?) Actually, I run a pretty laid back seder, all the more so this year considering there were goyim in attendance. It’s mostly just a big dinner with some Hebrew and matzoh and charoset thrown in for fun. But if I go a year without doing the four questions then I go through withdrawal, so a seder it is. My parents drove down from New Jersey for the big event, and since I can’t let them see the squalor I actually live in this meant a fair amount of cleaning. It’s good that they visit from time to time, since I need the incentive.

On top of that, the semester entered its dramatic final week. We still have finals to get through, but regular classes are now done. Yay!

But I’ve plainly been neglecting the blog again, so how about a new Sunday Chess Problem? I’ve chosen an easy to digest morsel for you, once again from Milan Vukcevich. The diagram below calls for Helpmate in Two:



We have not featured a helpmate in a while, so let me remind you how this works. In a helpmate, black and white cooperate to produce a position in which black is mated. Black always moves first! So, in a helpmate in two, we seek a sequence that goes 1. Black moves, white moves; 2. Black moves, white gives mate.

Now, in a short helpmate like this one, it is generally impossible to pack enough strategy into a single solution to make things interesting. With white and black working together, it is just too easy to contrive a mate. For that reason, short helpmates will generally have multiple solutions. This one, as it happens, has four solutions. For the problem to be interesting the solutions should be thematically related in some way.

Let’s have a look at the diagram. Since white essentially has only the two rooks with which to work, we might suspect the classic two rooks mate. You know the one I mean. The black king is trapped on the edge of the board, with the rooks occupying adjacent files to give mate. In the diagram we could try to contrive this mate either on the first and second ranks, or on the g and h files. As it happens, two of the solutions execute the first approach, while two of the solutions execute the second.

There are certainly some obstacles to overcome in giving these mates. Regardless of which of the two mating patterns we pursue, the white rook on b6 is obstructed by one of his pawns. The black rook, bishop and queen are all poised to interpose. And the white rook on g2 must move to somewhere safe, since currently he can be taken by the black king.

Can white and black, working together, overcome all these problems in a mere two moves? Yes he can!

Beyond that, the solutions pretty much speak for themselves. Just pay attention to all the line-openings, shut-offs, and interferences. Here we go. The first solution is this: 1. Rxb4 Rd2 2. Re4 Rb1 mate.



Next up is: 1. Nxb4 Rc2 2. Nd5 Rb1 mate.



Now we try to contrive mate on the g and h files. Here’s the first way: 1. Nxg6 Rg4 2. Ne7 Rh6 mate.



And finally we have this: 1. Bxg6 Rg5 2. Be4 Rh6 mate.



That was a lot of fun! Helpmates can sometimes seem like the candy of the chess problem world, though. Very enjoyable, and they certainly give you a brief thrill, but perhaps they are not as nourishing as those intricate, strategical, direct mates.

See you next week!



from ScienceBlogs http://ift.tt/1SHNH4a

It’s been a busy few weeks. I hosted a Passover seder. (What? Atheists can’t have seders?) Actually, I run a pretty laid back seder, all the more so this year considering there were goyim in attendance. It’s mostly just a big dinner with some Hebrew and matzoh and charoset thrown in for fun. But if I go a year without doing the four questions then I go through withdrawal, so a seder it is. My parents drove down from New Jersey for the big event, and since I can’t let them see the squalor I actually live in this meant a fair amount of cleaning. It’s good that they visit from time to time, since I need the incentive.

On top of that, the semester entered its dramatic final week. We still have finals to get through, but regular classes are now done. Yay!

But I’ve plainly been neglecting the blog again, so how about a new Sunday Chess Problem? I’ve chosen an easy to digest morsel for you, once again from Milan Vukcevich. The diagram below calls for Helpmate in Two:



We have not featured a helpmate in a while, so let me remind you how this works. In a helpmate, black and white cooperate to produce a position in which black is mated. Black always moves first! So, in a helpmate in two, we seek a sequence that goes 1. Black moves, white moves; 2. Black moves, white gives mate.

Now, in a short helpmate like this one, it is generally impossible to pack enough strategy into a single solution to make things interesting. With white and black working together, it is just too easy to contrive a mate. For that reason, short helpmates will generally have multiple solutions. This one, as it happens, has four solutions. For the problem to be interesting the solutions should be thematically related in some way.

Let’s have a look at the diagram. Since white essentially has only the two rooks with which to work, we might suspect the classic two rooks mate. You know the one I mean. The black king is trapped on the edge of the board, with the rooks occupying adjacent files to give mate. In the diagram we could try to contrive this mate either on the first and second ranks, or on the g and h files. As it happens, two of the solutions execute the first approach, while two of the solutions execute the second.

There are certainly some obstacles to overcome in giving these mates. Regardless of which of the two mating patterns we pursue, the white rook on b6 is obstructed by one of his pawns. The black rook, bishop and queen are all poised to interpose. And the white rook on g2 must move to somewhere safe, since currently he can be taken by the black king.

Can white and black, working together, overcome all these problems in a mere two moves? Yes he can!

Beyond that, the solutions pretty much speak for themselves. Just pay attention to all the line-openings, shut-offs, and interferences. Here we go. The first solution is this: 1. Rxb4 Rd2 2. Re4 Rb1 mate.



Next up is: 1. Nxb4 Rc2 2. Nd5 Rb1 mate.



Now we try to contrive mate on the g and h files. Here’s the first way: 1. Nxg6 Rg4 2. Ne7 Rh6 mate.



And finally we have this: 1. Bxg6 Rg5 2. Be4 Rh6 mate.



That was a lot of fun! Helpmates can sometimes seem like the candy of the chess problem world, though. Very enjoyable, and they certainly give you a brief thrill, but perhaps they are not as nourishing as those intricate, strategical, direct mates.

See you next week!



from ScienceBlogs http://ift.tt/1SHNH4a

Guide to Mars’ opposition on May 22

On May 22, 2016, Earth will fly between Mars and the sun, bringing the red planet closer to Earth than it’s been for over a decade. Astronomers call this event an opposition of Mars, and, although Mars’ oppositions typically come every other year, some bring Mars especially close. At this 2016 opposition, Mars isn’t as close as it can be. We’ll have to wait until 2018 for that. But, at a distance of 46.78 million miles (75.28 million km), this opposition brings Mars closer than it has been since the Martian opposition of November 7, 2005. As a result, for some weeks around late May, Mars will appear very bright! Follow the links below to learn more about Mars at its amazing 2016 opposition:

What is an opposition?

Why are Mars’ oppositions so variable?

How to see Mars near its 2016 opposition

Close Mars oppositions recur in cycles

Distant Mars oppositions recur in cycles, too

View larger | Mikhail Chubarets in the Ukraine made this chart. It shows the view of Mars through a telescope in 2016. We pass between Mars and the sun on May 22. We won't see Mars as a disk like this with the eye alone. But, between the start of 2016 and May, the dot of light that is Mars will grow dramatically brighter and redder in our night sky. Watch for it!

View larger | Mikhail Chubarets in the Ukraine made this chart. It shows the view of Mars through a telescope in 2016. We pass between Mars and the sun on May 22. We won’t see Mars as a disk like this with the eye alone. But, between the start of 2016 and May, the dot of light that is Mars will grow dramatically brighter and redder in our night sky. Watch for it!

What is an opposition? All superior planets – that is, planets orbiting the sun outside Earth’s orbit – are said to be at opposition whenever the Earth passes in between that planet and the sun, in our smaller and faster orbit.

The superior planets that are easily visible to the unaided eye include Mars, Jupiter and Saturn. Uranus and Neptune are also superior planets.

Mars is the next planet outward from Earth, at a mean distance from the sun of just over 1.5 astronomical units (AU). One AU equals one Earth-sun distance.

For comparison, the superior planets Jupiter and Saturn reside at a distance of about 5.2 AU and 9.6 AU.

Earth passes between the sun and Mars in a mean period of two years and 49 days, though the time period between successive oppositions is actually quite variable. An opposition can come anywhere from two years and one month – up to two years and two and one-half months – after the prior one.

At all oppositions of Mars (or any superior planet), the planet shines at its brightest in our sky and rises when the sun sets. It’s opposite the sun, as we swing between it and the sun. Mars at opposition stays out all night long, from sundown to sunup. It climbs highest up for the night at midnight.

Diagram by Roy L. Bishop. Copyright Royal Astronomical Society of Canada. Used with permission. Visit the RASC estore to purchase the Observers Handbook, a necessary tool for all skywatchers.

Diagram by Roy L. Bishop. Copyright Royal Astronomical Society of Canada. Used with permission. Visit the RASC estore to purchase the Observers Handbook, a necessary tool for all skywatchers. Read more about this image.

Why are Mars’ oppositions so variable? Earth’s orbit around the sun is very nearly circular. But Mars has a much more eccentric (oblong) orbit, which brings the red planet some 43 million kilometers (26 million miles) farther from the sun at its farthest point (aphelion) than at its closest point (perihelion).

That’s why the distance of Mars at opposition varies so widely. Earth flies between Mars and the sun every two years; sometimes that happens when Mars is far from the sun in its orbit, and sometimes it happens when Mars is close. The cycle of close and far Mars oppositions is about 15 years long. More about that below, or examine the chart above.

You might see that a Mars opposition coinciding with perihelion (the planet’s closest point to the sun) will be much more magnificent than a Mars’ opposition at aphelion (farthest point from the sun).

Astronomers call a Mars opposition coinciding with Mars’ closest point to the sun a perihelic opposition.

For example, the angular size of Mars’ disk during a perihelic opposition is nearly twice as large, and the brightness of Mars is nearly five times as great, than at an aphelic opposition.

Planets and moon on March 29, 2016 from Tom Wildoner in Weatherly, Pennsylvania.

Mars, Saturn, star Antares and moon on March 29, 2016 from Tom Wildoner in Weatherly, Pennsylvania. The two planets and bright star make a recognizable triangle on our sky’s dome throughout the opposition months.

Look for the Blue Moon to pair up with Mars on the sky's dome on May 21. The green line depicts the ecliptic - Earth's orbital plane projected onto the dome of sky.

Or let the moon guide you to Mars. Look for the Blue Moon to pair up with Mars on the sky’s dome on May 21. The green line depicts the ecliptic – sun’s path across our sky.

How to see Mars near its 2016 opposition. This year, we’re doubly lucky, when it comes to Mars. The planet is having a close opposition. And it’s visible on our sky’s dome within a noticeable pattern – a triangle – with Mars, Saturn and the bright star Antares marking the corners.

Mars shines near the planet Saturn and Antares, the brightest star in the constellation Scorpius the Scorpion, not just at opposition, but for many months in 2016.

You’ll enjoy picking this triangle out on the sky’s dome now, and comparing the brightness of Mars to that of Saturn and Antares in the coming months. On its opposition date on May 22, Mars shines some 7 times more brilliantly than Saturn, and some 17 times more brilliantly than the red star Antares.

Incidentally, the name Antares means like Mars. The ancients probably gave it that name because of the similarity of color between this star and the red planet. Notice the two objects’ colors. And notice how much the star twinkles while the planet Mars shines steadily. If you’ve never been able notice the steady light of planets, Mars and Antares can help!

Be sure to let the moon guide you to Mars, Saturn and Antares for several nights, centered on May 21. See the chart above.

After opposition, Mars will start to decrease in brightness, fading to Saturn’s magnitude by November, 2016, and then to Antares’ magnitude in January, 2017. But you can see that Northern Hemisphere summer (Southern Hemisphere winter) in 2016 will be an awesome time to amaze your family and friends by pointing Mars out in the night sky.

In 2016, Mars will briefly match the brightness of Jupiter, currently the brightest starlike object in the evening sky (since Venus is now behind the sun).

By the way, Mars has a much greater swing in brightness than do the planets Jupiter and Saturn. On rare occasions, Mars can (briefly) outshine Jupiter in the night sky during a favorable opposition. Meanwhile, in a non-opposition year, the red planet remains rather inconspicuous, blending in with nighttime’s numerous modestly-bright stars.

For instance, one year after the May 22, 2016 opposition, Mars will be some 5 times farther from Earth and some 30 times fainter.

In the year 2017, Mars will fade into a faint ember of its once-fiery self at opposition.

When Mars is far from the sun, as on March 3, 2012, it's a particularly distant opposition. But when Mars is near the sun, as on August 28, 2003, it's an extra-close opposition. Diagram via Sydney Observatory.

The inner dark circle represents Earth’s orbit around the sun; the outer dark circle represents Mars’ orbit. When Mars is near the sun, as it was in 2003, we have an extra-close opposition. On the other hand, 2012 was a particularly distant opposition of Mars because Mars was far from the sun in its orbit. At the 2014 opposition, Mars is getting closer to the sun again and therefore it’ll be closer to us than it was in 2012. But it’s not as close at this opposition as it will be in 2018. Diagram via Sydney Observatory.

Close Mars oppositions recur in cycles

The greatest/closest opposition of Mars since Stone Age times happened on August 28, 2003 (55.76 million kilometers or 34.65 miles). Close oppositions repeat in cycles of 15 to 17 years, so the oppositions of 2018 and 2020 will feature respectably close encounters – though neither will match the record-breaking opposition of August, 2003.

Similarly great Martian oppositions recur in cycles of 79 and 284 years. Seventy-nine years after the 2003 opposition, the opposition on September 1, 2082, will present Mars only a hair’s-breadth more distant than it was during the super-close opposition of August 28, 2003. Then 284 years after the 2003 opposition, a new record for closeness will accompany the August 29, 2287 opposition (55.69 million kilometers or 34.60 million miles).

Then 363 years (284 years + 79 years = 363 years) after the record-setting August 29, 2287 opposition, the opposition of September 4, 2650, will break that milestone to set another new record (55.65 million kilometers or 34.58 million miles).

Hubble Site contrasts the very distant opposition on February 12, 1995 (101.08 million kilometers) with the super-close opposition of August 28, 2003 (55.76 million kilometers). Image via Hubblesite

Hubble Site contrasts the very distant opposition on February 12, 1995 (101.08 million kilometers) with the super-close opposition of August 28, 2003 (55.76 million kilometers). Image via Hubblesite

Distant Mars oppositions recur in cycles, too. Surprised? Of course, you aren’t. Cycles abound in outer space.

A particularly small or distant opposition of Mars will happen on February 19, 2027 (101.42 million kilometers or 63.02 million miles). Distant oppositions recur in periods of 15 to 17 years, so the years 2042 and 2044 will feature small oppositions, as well.

Neither Mars opposition will be as distant as the 2027 one, however.

Similarly distant oppositions recur in periods of 79 and 284 years. But we don’t find a more distant opposition than the one occurring in the year 2027 until 442 years later (284 years + 79 years + 79 years = 442 years), on February 27, 2469. At that time, the red planet will be a whopping 101.46 million kilometers (63.04 million miles) from Earth.

Read more: Close and far Martian oppositions

So put Mars viewing on your calendar for 2016. You won’t see Mars this size again until 2018, when Mars will put on an even better show. Illustration via nasa.tumblr.com.

Telescopic image of Mars. During a close opposition, like the one in 2016, observers will make out more features on the planets surface. We won’t see Mars this size again until 2018, when Mars will put on an even better show. Illustration via nasa.tumblr.com.

Bottom line: This year, in 2016, enjoy the favorable opposition of May 22, as the red planet Mars shines in close vicinity of the planet Saturn and the red star Antares.



from EarthSky http://ift.tt/24gpFYS

On May 22, 2016, Earth will fly between Mars and the sun, bringing the red planet closer to Earth than it’s been for over a decade. Astronomers call this event an opposition of Mars, and, although Mars’ oppositions typically come every other year, some bring Mars especially close. At this 2016 opposition, Mars isn’t as close as it can be. We’ll have to wait until 2018 for that. But, at a distance of 46.78 million miles (75.28 million km), this opposition brings Mars closer than it has been since the Martian opposition of November 7, 2005. As a result, for some weeks around late May, Mars will appear very bright! Follow the links below to learn more about Mars at its amazing 2016 opposition:

What is an opposition?

Why are Mars’ oppositions so variable?

How to see Mars near its 2016 opposition

Close Mars oppositions recur in cycles

Distant Mars oppositions recur in cycles, too

View larger | Mikhail Chubarets in the Ukraine made this chart. It shows the view of Mars through a telescope in 2016. We pass between Mars and the sun on May 22. We won't see Mars as a disk like this with the eye alone. But, between the start of 2016 and May, the dot of light that is Mars will grow dramatically brighter and redder in our night sky. Watch for it!

View larger | Mikhail Chubarets in the Ukraine made this chart. It shows the view of Mars through a telescope in 2016. We pass between Mars and the sun on May 22. We won’t see Mars as a disk like this with the eye alone. But, between the start of 2016 and May, the dot of light that is Mars will grow dramatically brighter and redder in our night sky. Watch for it!

What is an opposition? All superior planets – that is, planets orbiting the sun outside Earth’s orbit – are said to be at opposition whenever the Earth passes in between that planet and the sun, in our smaller and faster orbit.

The superior planets that are easily visible to the unaided eye include Mars, Jupiter and Saturn. Uranus and Neptune are also superior planets.

Mars is the next planet outward from Earth, at a mean distance from the sun of just over 1.5 astronomical units (AU). One AU equals one Earth-sun distance.

For comparison, the superior planets Jupiter and Saturn reside at a distance of about 5.2 AU and 9.6 AU.

Earth passes between the sun and Mars in a mean period of two years and 49 days, though the time period between successive oppositions is actually quite variable. An opposition can come anywhere from two years and one month – up to two years and two and one-half months – after the prior one.

At all oppositions of Mars (or any superior planet), the planet shines at its brightest in our sky and rises when the sun sets. It’s opposite the sun, as we swing between it and the sun. Mars at opposition stays out all night long, from sundown to sunup. It climbs highest up for the night at midnight.

Diagram by Roy L. Bishop. Copyright Royal Astronomical Society of Canada. Used with permission. Visit the RASC estore to purchase the Observers Handbook, a necessary tool for all skywatchers.

Diagram by Roy L. Bishop. Copyright Royal Astronomical Society of Canada. Used with permission. Visit the RASC estore to purchase the Observers Handbook, a necessary tool for all skywatchers. Read more about this image.

Why are Mars’ oppositions so variable? Earth’s orbit around the sun is very nearly circular. But Mars has a much more eccentric (oblong) orbit, which brings the red planet some 43 million kilometers (26 million miles) farther from the sun at its farthest point (aphelion) than at its closest point (perihelion).

That’s why the distance of Mars at opposition varies so widely. Earth flies between Mars and the sun every two years; sometimes that happens when Mars is far from the sun in its orbit, and sometimes it happens when Mars is close. The cycle of close and far Mars oppositions is about 15 years long. More about that below, or examine the chart above.

You might see that a Mars opposition coinciding with perihelion (the planet’s closest point to the sun) will be much more magnificent than a Mars’ opposition at aphelion (farthest point from the sun).

Astronomers call a Mars opposition coinciding with Mars’ closest point to the sun a perihelic opposition.

For example, the angular size of Mars’ disk during a perihelic opposition is nearly twice as large, and the brightness of Mars is nearly five times as great, than at an aphelic opposition.

Planets and moon on March 29, 2016 from Tom Wildoner in Weatherly, Pennsylvania.

Mars, Saturn, star Antares and moon on March 29, 2016 from Tom Wildoner in Weatherly, Pennsylvania. The two planets and bright star make a recognizable triangle on our sky’s dome throughout the opposition months.

Look for the Blue Moon to pair up with Mars on the sky's dome on May 21. The green line depicts the ecliptic - Earth's orbital plane projected onto the dome of sky.

Or let the moon guide you to Mars. Look for the Blue Moon to pair up with Mars on the sky’s dome on May 21. The green line depicts the ecliptic – sun’s path across our sky.

How to see Mars near its 2016 opposition. This year, we’re doubly lucky, when it comes to Mars. The planet is having a close opposition. And it’s visible on our sky’s dome within a noticeable pattern – a triangle – with Mars, Saturn and the bright star Antares marking the corners.

Mars shines near the planet Saturn and Antares, the brightest star in the constellation Scorpius the Scorpion, not just at opposition, but for many months in 2016.

You’ll enjoy picking this triangle out on the sky’s dome now, and comparing the brightness of Mars to that of Saturn and Antares in the coming months. On its opposition date on May 22, Mars shines some 7 times more brilliantly than Saturn, and some 17 times more brilliantly than the red star Antares.

Incidentally, the name Antares means like Mars. The ancients probably gave it that name because of the similarity of color between this star and the red planet. Notice the two objects’ colors. And notice how much the star twinkles while the planet Mars shines steadily. If you’ve never been able notice the steady light of planets, Mars and Antares can help!

Be sure to let the moon guide you to Mars, Saturn and Antares for several nights, centered on May 21. See the chart above.

After opposition, Mars will start to decrease in brightness, fading to Saturn’s magnitude by November, 2016, and then to Antares’ magnitude in January, 2017. But you can see that Northern Hemisphere summer (Southern Hemisphere winter) in 2016 will be an awesome time to amaze your family and friends by pointing Mars out in the night sky.

In 2016, Mars will briefly match the brightness of Jupiter, currently the brightest starlike object in the evening sky (since Venus is now behind the sun).

By the way, Mars has a much greater swing in brightness than do the planets Jupiter and Saturn. On rare occasions, Mars can (briefly) outshine Jupiter in the night sky during a favorable opposition. Meanwhile, in a non-opposition year, the red planet remains rather inconspicuous, blending in with nighttime’s numerous modestly-bright stars.

For instance, one year after the May 22, 2016 opposition, Mars will be some 5 times farther from Earth and some 30 times fainter.

In the year 2017, Mars will fade into a faint ember of its once-fiery self at opposition.

When Mars is far from the sun, as on March 3, 2012, it's a particularly distant opposition. But when Mars is near the sun, as on August 28, 2003, it's an extra-close opposition. Diagram via Sydney Observatory.

The inner dark circle represents Earth’s orbit around the sun; the outer dark circle represents Mars’ orbit. When Mars is near the sun, as it was in 2003, we have an extra-close opposition. On the other hand, 2012 was a particularly distant opposition of Mars because Mars was far from the sun in its orbit. At the 2014 opposition, Mars is getting closer to the sun again and therefore it’ll be closer to us than it was in 2012. But it’s not as close at this opposition as it will be in 2018. Diagram via Sydney Observatory.

Close Mars oppositions recur in cycles

The greatest/closest opposition of Mars since Stone Age times happened on August 28, 2003 (55.76 million kilometers or 34.65 miles). Close oppositions repeat in cycles of 15 to 17 years, so the oppositions of 2018 and 2020 will feature respectably close encounters – though neither will match the record-breaking opposition of August, 2003.

Similarly great Martian oppositions recur in cycles of 79 and 284 years. Seventy-nine years after the 2003 opposition, the opposition on September 1, 2082, will present Mars only a hair’s-breadth more distant than it was during the super-close opposition of August 28, 2003. Then 284 years after the 2003 opposition, a new record for closeness will accompany the August 29, 2287 opposition (55.69 million kilometers or 34.60 million miles).

Then 363 years (284 years + 79 years = 363 years) after the record-setting August 29, 2287 opposition, the opposition of September 4, 2650, will break that milestone to set another new record (55.65 million kilometers or 34.58 million miles).

Hubble Site contrasts the very distant opposition on February 12, 1995 (101.08 million kilometers) with the super-close opposition of August 28, 2003 (55.76 million kilometers). Image via Hubblesite

Hubble Site contrasts the very distant opposition on February 12, 1995 (101.08 million kilometers) with the super-close opposition of August 28, 2003 (55.76 million kilometers). Image via Hubblesite

Distant Mars oppositions recur in cycles, too. Surprised? Of course, you aren’t. Cycles abound in outer space.

A particularly small or distant opposition of Mars will happen on February 19, 2027 (101.42 million kilometers or 63.02 million miles). Distant oppositions recur in periods of 15 to 17 years, so the years 2042 and 2044 will feature small oppositions, as well.

Neither Mars opposition will be as distant as the 2027 one, however.

Similarly distant oppositions recur in periods of 79 and 284 years. But we don’t find a more distant opposition than the one occurring in the year 2027 until 442 years later (284 years + 79 years + 79 years = 442 years), on February 27, 2469. At that time, the red planet will be a whopping 101.46 million kilometers (63.04 million miles) from Earth.

Read more: Close and far Martian oppositions

So put Mars viewing on your calendar for 2016. You won’t see Mars this size again until 2018, when Mars will put on an even better show. Illustration via nasa.tumblr.com.

Telescopic image of Mars. During a close opposition, like the one in 2016, observers will make out more features on the planets surface. We won’t see Mars this size again until 2018, when Mars will put on an even better show. Illustration via nasa.tumblr.com.

Bottom line: This year, in 2016, enjoy the favorable opposition of May 22, as the red planet Mars shines in close vicinity of the planet Saturn and the red star Antares.



from EarthSky http://ift.tt/24gpFYS

2016 SkS Weekly Digest #18

SkS Highlights... El Niño to La Niña... Toon of the Week... Quote of the Week... He Said What?... SkS in the News... SkS Spotlights... Coming Soon on SkS... Poster of the Week... SkS Week in Review... 97 Hours of Consensus...

SkS Highlights

Can the Republican Party solve its science denial problem? by Dana Nuccitelli garnered the highest number of comments among the articles posted on SkS during the past week. The article was originally posted on the Climate Consensus - the 97% Guardian blog maintained by Nuccitelli and John Abraham where it generated a lengthy and quite contentious comment thread. Click here to access the Guardian article and comment thread.

El Niño to La Niñposted on SkS during the past week. a

Withering drought and sizzling temperatures from El Nino have caused food and water shortages and ravaged farming across Asia, and experts warn of a double-whammy of possible flooding from its sibling, La Nina.

The current El Nino which began last year has been one of the strongest ever, leaving the Mekong River at its lowest level in decades, causing food-related unrest in the Philippines, and smothering vast regions in a months-long heat wave often topping 40 degrees Celsius (104 Fahrenheit).

Economic losses in Southeast Asia could top $10 billion, IHS Global Insight told AFP.

The regional fever is expected to break by mid-year but fears are growing that an equally forceful La Nina will follow.

That could bring heavy rain to an already flood-prone region, exacerbating agricultural damage and leaving crops vulnerable to disease and pests.

El Nino dries up Asia as its stormy sister La Nina looms by Satish Cheney, Phys.org, Apr 29, 2016

Toon of the Week

2016 Toon 18 

Hat tip to I Heart Climate Scientists

Quote of the Week 

"Loss of oxygen in the oceans is one of the serious side effects of a warming atmosphere, and a major threat to marine life," said Matthew Long*, who is the lead author of the study. "Since oxygen concentrations in the ocean naturally vary depending on variations in winds and temperature at the surface, it's been challenging to attribute any de-oxygenation to climate change. This new study tells us when we can expect the effect from climate change to overwhelm the natural variability."

*National Center for Atmospheric Research (NCAR)

It May Soon Be Too Late to Save the Seas by Jeff Nesbit, Climate/US News & World Report, Apr 27, 2016

He Said What?

“The coal industry is being destroyed,” he* says. “And it’s scary to me because electricity is a staple of life — like potatoes were to the Irish. And Obama has largely destroyed reliable, low-cost, affordable electricity in America.”

*Robert E. Murray, chairman of the Murray Energy Corporation

A Crusader in the Coal Mine, Taking On President Obama by Jad Mouawad, Energy & Environment, New York Times, Apr 30, 2016

SkS in the News

Consensus on consensus: a synthesis of consensus estimates on human-caused global warming , Cook et al, Environmental Research LettersVolume 11, Number 4, Apr 13, 2016 has generated a slew of articles in the media and blogosphere. A list of those articles will be published as SkS News Bulletin #1 later this week.

SkS Spotlights

The Carbon Pricing Leadership Coalition brings together leaders from across government, the private sector and civil society to share experience working with carbon pricing and to expand the evidence base for the most effective carbon pricing systems and policies.

The Coalition is a voluntary partnership of national and sub-national governments, businesses, and civil society organizations that agree to advance the carbon pricing agenda by working with each other towards the long-term objective of a carbon price applied throughout the global economy by:

  • strengthening carbon pricing policies to redirect investment commensurate with the scale of the climate challenge;
  • bringing forward and strengthening the implementation of existing carbon pricing policies to better manage investment risks and opportunities; and
  • enhancing cooperation to share information, expertise and lessons learned on developing and implementing carbon pricing through various "readiness" platforms

The Coalition will collect the evidence base, benefiting from experience around the world in designing and using carbon pricing, and use this input to help inform successful carbon pricing policy development and use of carbon pricing in businesses. It will also deepen understanding of the business and economic case for carbon pricing. In that role, it is developing pathways for use by companies, investors and governments that will illustrate plausible outlooks under a variety of carbon pricing policies and timelines. Finally, the coalition will work to bring together government and business in leadership dialogues that identify and address the most pressing issues, and in doing so, accelerate the use of carbon pricing around the world.

Coming Soon on SkS 

  • Peabody coal's contrarian scientist witnesses lose their court case (John Abraham)
  • Handy resources when facing a firehose of falsehoods (Baerbel)
  • Scientists are figuring out the keys to convincing people about global warming (Dana)
  • Consensus on Consensus (AndyS)
  • Deep sea microbes may be key to oceans’ climate change feedback (Howard Lee)
  • 2016 SkS Weekly News Roundup #19 (John Hartz)
  • 2016 SkS Weekly Digest #19 (John Hartz)

Poster of the Week

2016 Poster 18 

SkS Week in Review

97 Hours of Consensus: Myles Allen

97 Hours: Myles Allen 

 

Myles Allen's bio page & Quote source



from Skeptical Science http://ift.tt/1TDYGOD

SkS Highlights... El Niño to La Niña... Toon of the Week... Quote of the Week... He Said What?... SkS in the News... SkS Spotlights... Coming Soon on SkS... Poster of the Week... SkS Week in Review... 97 Hours of Consensus...

SkS Highlights

Can the Republican Party solve its science denial problem? by Dana Nuccitelli garnered the highest number of comments among the articles posted on SkS during the past week. The article was originally posted on the Climate Consensus - the 97% Guardian blog maintained by Nuccitelli and John Abraham where it generated a lengthy and quite contentious comment thread. Click here to access the Guardian article and comment thread.

El Niño to La Niñposted on SkS during the past week. a

Withering drought and sizzling temperatures from El Nino have caused food and water shortages and ravaged farming across Asia, and experts warn of a double-whammy of possible flooding from its sibling, La Nina.

The current El Nino which began last year has been one of the strongest ever, leaving the Mekong River at its lowest level in decades, causing food-related unrest in the Philippines, and smothering vast regions in a months-long heat wave often topping 40 degrees Celsius (104 Fahrenheit).

Economic losses in Southeast Asia could top $10 billion, IHS Global Insight told AFP.

The regional fever is expected to break by mid-year but fears are growing that an equally forceful La Nina will follow.

That could bring heavy rain to an already flood-prone region, exacerbating agricultural damage and leaving crops vulnerable to disease and pests.

El Nino dries up Asia as its stormy sister La Nina looms by Satish Cheney, Phys.org, Apr 29, 2016

Toon of the Week

2016 Toon 18 

Hat tip to I Heart Climate Scientists

Quote of the Week 

"Loss of oxygen in the oceans is one of the serious side effects of a warming atmosphere, and a major threat to marine life," said Matthew Long*, who is the lead author of the study. "Since oxygen concentrations in the ocean naturally vary depending on variations in winds and temperature at the surface, it's been challenging to attribute any de-oxygenation to climate change. This new study tells us when we can expect the effect from climate change to overwhelm the natural variability."

*National Center for Atmospheric Research (NCAR)

It May Soon Be Too Late to Save the Seas by Jeff Nesbit, Climate/US News & World Report, Apr 27, 2016

He Said What?

“The coal industry is being destroyed,” he* says. “And it’s scary to me because electricity is a staple of life — like potatoes were to the Irish. And Obama has largely destroyed reliable, low-cost, affordable electricity in America.”

*Robert E. Murray, chairman of the Murray Energy Corporation

A Crusader in the Coal Mine, Taking On President Obama by Jad Mouawad, Energy & Environment, New York Times, Apr 30, 2016

SkS in the News

Consensus on consensus: a synthesis of consensus estimates on human-caused global warming , Cook et al, Environmental Research LettersVolume 11, Number 4, Apr 13, 2016 has generated a slew of articles in the media and blogosphere. A list of those articles will be published as SkS News Bulletin #1 later this week.

SkS Spotlights

The Carbon Pricing Leadership Coalition brings together leaders from across government, the private sector and civil society to share experience working with carbon pricing and to expand the evidence base for the most effective carbon pricing systems and policies.

The Coalition is a voluntary partnership of national and sub-national governments, businesses, and civil society organizations that agree to advance the carbon pricing agenda by working with each other towards the long-term objective of a carbon price applied throughout the global economy by:

  • strengthening carbon pricing policies to redirect investment commensurate with the scale of the climate challenge;
  • bringing forward and strengthening the implementation of existing carbon pricing policies to better manage investment risks and opportunities; and
  • enhancing cooperation to share information, expertise and lessons learned on developing and implementing carbon pricing through various "readiness" platforms

The Coalition will collect the evidence base, benefiting from experience around the world in designing and using carbon pricing, and use this input to help inform successful carbon pricing policy development and use of carbon pricing in businesses. It will also deepen understanding of the business and economic case for carbon pricing. In that role, it is developing pathways for use by companies, investors and governments that will illustrate plausible outlooks under a variety of carbon pricing policies and timelines. Finally, the coalition will work to bring together government and business in leadership dialogues that identify and address the most pressing issues, and in doing so, accelerate the use of carbon pricing around the world.

Coming Soon on SkS 

  • Peabody coal's contrarian scientist witnesses lose their court case (John Abraham)
  • Handy resources when facing a firehose of falsehoods (Baerbel)
  • Scientists are figuring out the keys to convincing people about global warming (Dana)
  • Consensus on Consensus (AndyS)
  • Deep sea microbes may be key to oceans’ climate change feedback (Howard Lee)
  • 2016 SkS Weekly News Roundup #19 (John Hartz)
  • 2016 SkS Weekly Digest #19 (John Hartz)

Poster of the Week

2016 Poster 18 

SkS Week in Review

97 Hours of Consensus: Myles Allen

97 Hours: Myles Allen 

 

Myles Allen's bio page & Quote source



from Skeptical Science http://ift.tt/1TDYGOD