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Like coastlines? You’ll like this video



If you like science, and you like spending a day along a coastline – and if you live in the Pacific Northwest or Alaska – this citizen science project might be for you. It’s called COASST, and it’s a group of scientists and volunteers who monitor beach-cast seabird carcasses to learn more about bird populations in their local ecosystems.


Julia K. Parrish, the Executive Director of COASST, explains it all in this video.


It looks really worthwhile, plus like a lot of fun!


Visit COASST’s website.






from EarthSky http://ift.tt/1Muc0Vh


If you like science, and you like spending a day along a coastline – and if you live in the Pacific Northwest or Alaska – this citizen science project might be for you. It’s called COASST, and it’s a group of scientists and volunteers who monitor beach-cast seabird carcasses to learn more about bird populations in their local ecosystems.


Julia K. Parrish, the Executive Director of COASST, explains it all in this video.


It looks really worthwhile, plus like a lot of fun!


Visit COASST’s website.






from EarthSky http://ift.tt/1Muc0Vh

How Sea Floor Ecosystems Are Damaged By, And Recover From, Abrupt Climate Change [Greg Laden's Blog]

A new study by Sarah Moffitt, Tessa Hill, Peter Roopnarine, and James Kennett (Response of seafloor ecosystems to abrubt global climate change) gets a handle on the effects of relatively rapid warming and associated Oxygen loss in the sea on invertebrate communities. The study looked at a recent warming event (the end of the last glacial) in order to understand the present warming event, which is the result of human-caused greenhouse gas pollution.


Here is what is unique about the study. A 30 foot deep core representing the time period from 3,400 to 16,100 year ago, was raised from a site in the pacific, and the researchers tried to identify and characterize all of the complex invertebrate remains in the core. That is not usually how it is done. Typically a limited number of species, and usually microscopic surface invertebrates (Foraminifera) only, are identified and counted. There are good reasons it is done that way. But the new study looks instead at non-single-celled invertebrates (i.e., clams and such) typically found at the bottom, not top, of the water column. This study identified over 5,400 fossils and trace fossils from Mollusca, Echinodermata, Arthropoda, and Annelida (clams, worms, etc.).


Complex invertebrates are important because of their high degree of connectivity in an ecosystem. In the sea, a clam, crab, or sea cucumber may be the canary in the proverbial coal mine. Study co-author Peter Roopnarine says, “The complexity and diversity of a community depends on how much energy is available. To truly understand the health of an ecosystem and the food webs within, we have to look at the simple and small as well as the complex. In this case, marine invertebrates give us a better understanding of the health of ecosystems as a whole.”


The most important finding of the study is this: the marine ecosystem sampled by this core underwent dramatic changes, including local extinctions, and took up to something like 1,000 years to recover from that. The amount of change in bottom ecosystems under these conditions was previously not well known, and the recovery rate was previously assumed to be much shorter, on the order of a century.


From the abstract of the paper:



Anthropogenic climate change is predicted to decrease oceanic oxygen (O2) concentrations, with potentially significant effects on marine ecosystems. Geologically recent episodes of abrupt climatic warming provide opportunities to assess the effects of changing oxygenation on marine communities. Thus far, this knowledge has been largely restricted to investigations using Foraminifera, with little being known about ecosystem-scale responses to abrupt, climate-forced deoxygenation. We here present high-resolution records based on the first comprehensive quantitative analysis, to our knowledge, of changes in marine metazoans … in response to the global warming associated with the last glacial to interglacial episode. The molluscan archive is dominated by extremophile taxa, including those containing endosymbiotic sulfur-oxidizing bacteria (Lucinoma aequizonatum) and those that graze on filamentous sulfur-oxidizing benthic bacterial mats (Alia permodesta). This record … demonstrates that seafloor invertebrate communities are subject to major turnover in response to relatively minor inferred changes in oxygenation (>1.5 to <0.5 mL·L−1 [O2]) associated with abrupt (<100 y) warming of the eastern Pacific. The biotic turnover and recovery events within the record expand known rates of marine biological recovery by an order of magnitude, from <100 to >1,000 y, and illustrate the crucial role of climate and oceanographic change in driving long-term successional changes in ocean ecosystems.



Lead author Sarah Moffitt, of the UC Davis Bodega Marine Laboratory and Coastal and Marine Sciences Institute notes, “In this study, we used the past to forecast the future. Tracing changes in marine biodiversity during historical episodes of warming and cooling tells us what might happen in years to come. We don’t want to hear that ecosystems need thousands of years to recover from disruption, but it’s critical that we understand the global need to combat modern climate impacts.”


There is a video:





Caption from the figure at the top of the post: Fig. 1. Core MV0811–15JC’s (SBB; 418 m water depth; 9.2 m core length; 34.37°N, 120.13°W) oxygen isotopic, foraminiferal, and metazoan deglacial record of the latest Quaternary. Timescale (ka) is in thousands of years before present, and major climatic events include the Last Glacial Maximum (LGM), the Bølling and Allerød (B/A), the Younger Dryas (YD), and the Holocene. (A) GISP2 ice core δ18O values (46). (B) Planktonic Foraminifera Globigerina bulloides δ18O values for core MV0811–15JC, which reflects both deglacial temperature changes in Eastern Pacific surface waters and changes in global ice volume. (C) Benthic foraminiferal density (individuals/cm3). (D) Relative frequency (%) of benthic Foraminifera with faunal oxygen-tolerance categories including oxic–mildly hypoxic (>1.5 mL·L−1 O2; N. labradorica, Quinqueloculina spp., Pyrgo spp.), intermediate hypoxia (1.5–0.5 mL·L−1 O2; Epistominella spp., Bolivina spp., Uvigerina spp.), and severe hypoxia (<0.5 mL·L−1 O2; N. stella, B. tumida) (19). (E) Log mollusc density (individuals/cm3). (F) Ophiuroids (brittle star) presence (presence = 1, absence = 0, 5-cm moving average). (G) Ostracod valve density (circles, valves/cm3) and 5-cm moving average.






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

A new study by Sarah Moffitt, Tessa Hill, Peter Roopnarine, and James Kennett (Response of seafloor ecosystems to abrubt global climate change) gets a handle on the effects of relatively rapid warming and associated Oxygen loss in the sea on invertebrate communities. The study looked at a recent warming event (the end of the last glacial) in order to understand the present warming event, which is the result of human-caused greenhouse gas pollution.


Here is what is unique about the study. A 30 foot deep core representing the time period from 3,400 to 16,100 year ago, was raised from a site in the pacific, and the researchers tried to identify and characterize all of the complex invertebrate remains in the core. That is not usually how it is done. Typically a limited number of species, and usually microscopic surface invertebrates (Foraminifera) only, are identified and counted. There are good reasons it is done that way. But the new study looks instead at non-single-celled invertebrates (i.e., clams and such) typically found at the bottom, not top, of the water column. This study identified over 5,400 fossils and trace fossils from Mollusca, Echinodermata, Arthropoda, and Annelida (clams, worms, etc.).


Complex invertebrates are important because of their high degree of connectivity in an ecosystem. In the sea, a clam, crab, or sea cucumber may be the canary in the proverbial coal mine. Study co-author Peter Roopnarine says, “The complexity and diversity of a community depends on how much energy is available. To truly understand the health of an ecosystem and the food webs within, we have to look at the simple and small as well as the complex. In this case, marine invertebrates give us a better understanding of the health of ecosystems as a whole.”


The most important finding of the study is this: the marine ecosystem sampled by this core underwent dramatic changes, including local extinctions, and took up to something like 1,000 years to recover from that. The amount of change in bottom ecosystems under these conditions was previously not well known, and the recovery rate was previously assumed to be much shorter, on the order of a century.


From the abstract of the paper:



Anthropogenic climate change is predicted to decrease oceanic oxygen (O2) concentrations, with potentially significant effects on marine ecosystems. Geologically recent episodes of abrupt climatic warming provide opportunities to assess the effects of changing oxygenation on marine communities. Thus far, this knowledge has been largely restricted to investigations using Foraminifera, with little being known about ecosystem-scale responses to abrupt, climate-forced deoxygenation. We here present high-resolution records based on the first comprehensive quantitative analysis, to our knowledge, of changes in marine metazoans … in response to the global warming associated with the last glacial to interglacial episode. The molluscan archive is dominated by extremophile taxa, including those containing endosymbiotic sulfur-oxidizing bacteria (Lucinoma aequizonatum) and those that graze on filamentous sulfur-oxidizing benthic bacterial mats (Alia permodesta). This record … demonstrates that seafloor invertebrate communities are subject to major turnover in response to relatively minor inferred changes in oxygenation (>1.5 to <0.5 mL·L−1 [O2]) associated with abrupt (<100 y) warming of the eastern Pacific. The biotic turnover and recovery events within the record expand known rates of marine biological recovery by an order of magnitude, from <100 to >1,000 y, and illustrate the crucial role of climate and oceanographic change in driving long-term successional changes in ocean ecosystems.



Lead author Sarah Moffitt, of the UC Davis Bodega Marine Laboratory and Coastal and Marine Sciences Institute notes, “In this study, we used the past to forecast the future. Tracing changes in marine biodiversity during historical episodes of warming and cooling tells us what might happen in years to come. We don’t want to hear that ecosystems need thousands of years to recover from disruption, but it’s critical that we understand the global need to combat modern climate impacts.”


There is a video:





Caption from the figure at the top of the post: Fig. 1. Core MV0811–15JC’s (SBB; 418 m water depth; 9.2 m core length; 34.37°N, 120.13°W) oxygen isotopic, foraminiferal, and metazoan deglacial record of the latest Quaternary. Timescale (ka) is in thousands of years before present, and major climatic events include the Last Glacial Maximum (LGM), the Bølling and Allerød (B/A), the Younger Dryas (YD), and the Holocene. (A) GISP2 ice core δ18O values (46). (B) Planktonic Foraminifera Globigerina bulloides δ18O values for core MV0811–15JC, which reflects both deglacial temperature changes in Eastern Pacific surface waters and changes in global ice volume. (C) Benthic foraminiferal density (individuals/cm3). (D) Relative frequency (%) of benthic Foraminifera with faunal oxygen-tolerance categories including oxic–mildly hypoxic (>1.5 mL·L−1 O2; N. labradorica, Quinqueloculina spp., Pyrgo spp.), intermediate hypoxia (1.5–0.5 mL·L−1 O2; Epistominella spp., Bolivina spp., Uvigerina spp.), and severe hypoxia (<0.5 mL·L−1 O2; N. stella, B. tumida) (19). (E) Log mollusc density (individuals/cm3). (F) Ophiuroids (brittle star) presence (presence = 1, absence = 0, 5-cm moving average). (G) Ostracod valve density (circles, valves/cm3) and 5-cm moving average.






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

Shrinking of Antarctic ice shelves is accelerating

Antarctica’s Brunt Ice Shelf photographed in October 2011 from NASA’s DC-8 research aircraft during an Operation IceBridge flight. Michael Studinger/NASA

Antarctica’s Brunt Ice Shelf photographed in October 2011 from NASA’s DC-8 research aircraft during an Operation IceBridge flight. Michael Studinger/NASA



By Laurence Padman, Earth and Space Research ; Fernando Paolo, University of California, San Diego , and Helen Amanda Fricker, University of California, San Diego


Ask people what they know about Antarctica and they usually mention cold, snow and ice. In fact, there’s so much ice on Antarctica that if it all melted into the ocean, average sea level around the entire world would rise about 200 feet, roughly the height of a 20-story building.


Could this happen? There’s evidence that at various times in the past there was much less ice on Antarctica than there is today. For example, during an extended warm period called the Eemian interglacial about 100,000 years ago, Antarctica probably lost enough ice to raise sea level by several meters.


Scientists think that global average temperature back then was only about two degrees Fahrenheit warmer than today. Assuming we continue to burn fossil fuels and add greenhouse gases to the atmosphere, global temperature is expected to rise by at least two degrees Fahrenheit by 2100. What will that do to Antarctica’s ice sheet? Even one meter of worldwide sea level rise – that is, melting only a fiftieth of the ice sheet – would cause massive displacements of coastal populations and require major investments to protect or relocate cities, ports and other coastal infrastructure.


Ice leaving Antarctica enters the ocean through ice shelves, which are the floating edges of the ice sheet. We expect that any changes to the ice sheet caused by changes in the ocean will be felt first by the ice shelves. Using satellite data, we analyzed how Antarctica’s ice shelves have changed over nearly two decades. Our paper published in Science shows that not only has ice shelf volume gone down, but losses have accelerated over the past decade, a result that provides insight into how our future climate will affect the ice sheet and sea level.


Cork in a champagne bottle


The link between changing global temperature and ice loss from Antarctica’s ice sheet is not straightforward. By itself, air temperature has a fairly small influence on the ice sheet, since most of it is already well below freezing.


It turns out that, to understand ice loss, we need to know about changes in winds, snowfall, ocean temperature and currents, sea ice, and the geology under the ice sheets. We don’t yet have enough information on any of these to build reliable models for predicting ice sheet response to climate changes.


We do know that one important control on ice loss from Antarctica is what happens where the ice sheet meets the ocean. The Antarctic Ice Sheet gains ice by snowfall. The ice sheet spreads under its own weight forming glaciers and ice streams that flow slowly downhill towards the ocean. Once they lift off the bedrock and begin to float, they become ice shelves. To stay in balance, ice shelves have to shed the ice they gained from glacier flow and local snowfall. Chunks break off to form icebergs and ice is also lost from the bottom by melting as warm ocean water flows under it.


View larger |

Schematic diagram of an Antarctic ice shelf showing the processes causing the volume changes measured by satellites. Ice is added to the ice shelf by glaciers flowing off the continent and by snowfall that compresses to form ice. Ice is lost when icebergs break off the ice front, and by melting in some regions as warm water flows into the ocean cavity under the ice shelf. Under some ice shelves, cold and fresh meltwater rises to a point where it refreezes onto the ice shelf. View larger | Image credit: Helen Amanda Fricker, Professor, Scripps Institution of Oceanography, UC San Diego



An ice shelf acts a bit like a cork in a champagne bottle, slowing down the glaciers flowing from the ground into it; scientists call this the buttressing effect. Recent observations show that when ice shelves thin or collapse, the glacier flow from the land into the ocean speeds up, which contributes to sea level rise. So understanding what makes ice shelves change size is an important scientific question.


Building an ice shelves map


The first step towards understanding ice shelves is to work out just how much and how quickly they have changed in the past. In our paper, we show detailed maps of changes in ice shelves all around Antarctica based on the 18 years from 1994 to 2012. The data came from continuous measurements of surface height collected by three European Space Agency radar altimeter satellites. By comparing surface heights at the same point on the ice shelf at different times, we can build a record of ice height changes. We can then convert that to thickness changes using ice density and the fact that ice shelves float.


Prior studies of changes in ice shelf thickness and volume have given averages for individual ice shelves or approximated the changes in time as straight-line fits over short periods. In contrast, our new study presents high-resolution (about 30 km by 30 km) maps of thickness changes at three-month time steps for the 18-year period. This data set allows us to see how the rate of thinning varies between different parts of the same ice shelf, and between different years.


This map shows eighteen years of change in thickness and volume of Antarctic ice shelves. Rates of thickness change (meters/decade) are color-coded from -25 (thinning) to +10 (thickening). Circles represent percentage of thickness lost (red) or gained (blue) in 18 years. The central circle demarcates the area not surveyed by the satellites (south of 81.5ºS). Original data were interpolated for mapping purposes. Image credit: Scripps Institution of Oceanography, UC San Diego

This map shows eighteen years of change in thickness and volume of Antarctic ice shelves. Rates of thickness change (meters/decade) are color-coded from -25 (thinning) to +10 (thickening). Circles represent percentage of thickness lost (red) or gained (blue) in 18 years. The central circle demarcates the area not surveyed by the satellites (south of 81.5ºS). Original data were interpolated for mapping purposes. Image credit: Scripps Institution of Oceanography, UC San Diego



We find that, if recent trends continue, some ice shelves will thin dramatically within centuries, reducing their ability to buttress the ice sheet. Other ice shelves are gaining ice, and so could slow down the loss of ice from the ground.


When we sum up losses around Antarctica, we find that the change in volume of all the ice shelves was almost zero in the first decade of our record (1994-2003) but, on average, over 300 cubic kilometers per year were lost between 2003 and 2012.


The pattern of acceleration in ice loss varies between regions. During the first half of the record, ice losses from West Antarctica were almost balanced by gains in East Antarctica. After about 2003, East Antarctic ice shelf volume stabilized, and West Antarctic losses increased slightly.


Changes in climate factors like snowfall, wind speed and ocean circulation will lead to different patterns of ice shelf thickness change in time and space. We can compare the “fingerprints” of these factors with our new, much clearer maps to identify the primary causes, which might be different in different regions around Antarctica.


Our 18-year data set has demonstrated the value of long and continuous observations of the ice shelves, showing that shorter records cannot capture the true variability. We expect that our results will inspire new ways of thinking about how the ocean and atmosphere can affect ice shelves and, through them, ice loss from Antarctica.


The Conversation


This article was originally published on The Conversation.


Read the original article.






from EarthSky http://ift.tt/1C1e2AH
Antarctica’s Brunt Ice Shelf photographed in October 2011 from NASA’s DC-8 research aircraft during an Operation IceBridge flight. Michael Studinger/NASA

Antarctica’s Brunt Ice Shelf photographed in October 2011 from NASA’s DC-8 research aircraft during an Operation IceBridge flight. Michael Studinger/NASA



By Laurence Padman, Earth and Space Research ; Fernando Paolo, University of California, San Diego , and Helen Amanda Fricker, University of California, San Diego


Ask people what they know about Antarctica and they usually mention cold, snow and ice. In fact, there’s so much ice on Antarctica that if it all melted into the ocean, average sea level around the entire world would rise about 200 feet, roughly the height of a 20-story building.


Could this happen? There’s evidence that at various times in the past there was much less ice on Antarctica than there is today. For example, during an extended warm period called the Eemian interglacial about 100,000 years ago, Antarctica probably lost enough ice to raise sea level by several meters.


Scientists think that global average temperature back then was only about two degrees Fahrenheit warmer than today. Assuming we continue to burn fossil fuels and add greenhouse gases to the atmosphere, global temperature is expected to rise by at least two degrees Fahrenheit by 2100. What will that do to Antarctica’s ice sheet? Even one meter of worldwide sea level rise – that is, melting only a fiftieth of the ice sheet – would cause massive displacements of coastal populations and require major investments to protect or relocate cities, ports and other coastal infrastructure.


Ice leaving Antarctica enters the ocean through ice shelves, which are the floating edges of the ice sheet. We expect that any changes to the ice sheet caused by changes in the ocean will be felt first by the ice shelves. Using satellite data, we analyzed how Antarctica’s ice shelves have changed over nearly two decades. Our paper published in Science shows that not only has ice shelf volume gone down, but losses have accelerated over the past decade, a result that provides insight into how our future climate will affect the ice sheet and sea level.


Cork in a champagne bottle


The link between changing global temperature and ice loss from Antarctica’s ice sheet is not straightforward. By itself, air temperature has a fairly small influence on the ice sheet, since most of it is already well below freezing.


It turns out that, to understand ice loss, we need to know about changes in winds, snowfall, ocean temperature and currents, sea ice, and the geology under the ice sheets. We don’t yet have enough information on any of these to build reliable models for predicting ice sheet response to climate changes.


We do know that one important control on ice loss from Antarctica is what happens where the ice sheet meets the ocean. The Antarctic Ice Sheet gains ice by snowfall. The ice sheet spreads under its own weight forming glaciers and ice streams that flow slowly downhill towards the ocean. Once they lift off the bedrock and begin to float, they become ice shelves. To stay in balance, ice shelves have to shed the ice they gained from glacier flow and local snowfall. Chunks break off to form icebergs and ice is also lost from the bottom by melting as warm ocean water flows under it.


View larger |

Schematic diagram of an Antarctic ice shelf showing the processes causing the volume changes measured by satellites. Ice is added to the ice shelf by glaciers flowing off the continent and by snowfall that compresses to form ice. Ice is lost when icebergs break off the ice front, and by melting in some regions as warm water flows into the ocean cavity under the ice shelf. Under some ice shelves, cold and fresh meltwater rises to a point where it refreezes onto the ice shelf. View larger | Image credit: Helen Amanda Fricker, Professor, Scripps Institution of Oceanography, UC San Diego



An ice shelf acts a bit like a cork in a champagne bottle, slowing down the glaciers flowing from the ground into it; scientists call this the buttressing effect. Recent observations show that when ice shelves thin or collapse, the glacier flow from the land into the ocean speeds up, which contributes to sea level rise. So understanding what makes ice shelves change size is an important scientific question.


Building an ice shelves map


The first step towards understanding ice shelves is to work out just how much and how quickly they have changed in the past. In our paper, we show detailed maps of changes in ice shelves all around Antarctica based on the 18 years from 1994 to 2012. The data came from continuous measurements of surface height collected by three European Space Agency radar altimeter satellites. By comparing surface heights at the same point on the ice shelf at different times, we can build a record of ice height changes. We can then convert that to thickness changes using ice density and the fact that ice shelves float.


Prior studies of changes in ice shelf thickness and volume have given averages for individual ice shelves or approximated the changes in time as straight-line fits over short periods. In contrast, our new study presents high-resolution (about 30 km by 30 km) maps of thickness changes at three-month time steps for the 18-year period. This data set allows us to see how the rate of thinning varies between different parts of the same ice shelf, and between different years.


This map shows eighteen years of change in thickness and volume of Antarctic ice shelves. Rates of thickness change (meters/decade) are color-coded from -25 (thinning) to +10 (thickening). Circles represent percentage of thickness lost (red) or gained (blue) in 18 years. The central circle demarcates the area not surveyed by the satellites (south of 81.5ºS). Original data were interpolated for mapping purposes. Image credit: Scripps Institution of Oceanography, UC San Diego

This map shows eighteen years of change in thickness and volume of Antarctic ice shelves. Rates of thickness change (meters/decade) are color-coded from -25 (thinning) to +10 (thickening). Circles represent percentage of thickness lost (red) or gained (blue) in 18 years. The central circle demarcates the area not surveyed by the satellites (south of 81.5ºS). Original data were interpolated for mapping purposes. Image credit: Scripps Institution of Oceanography, UC San Diego



We find that, if recent trends continue, some ice shelves will thin dramatically within centuries, reducing their ability to buttress the ice sheet. Other ice shelves are gaining ice, and so could slow down the loss of ice from the ground.


When we sum up losses around Antarctica, we find that the change in volume of all the ice shelves was almost zero in the first decade of our record (1994-2003) but, on average, over 300 cubic kilometers per year were lost between 2003 and 2012.


The pattern of acceleration in ice loss varies between regions. During the first half of the record, ice losses from West Antarctica were almost balanced by gains in East Antarctica. After about 2003, East Antarctic ice shelf volume stabilized, and West Antarctic losses increased slightly.


Changes in climate factors like snowfall, wind speed and ocean circulation will lead to different patterns of ice shelf thickness change in time and space. We can compare the “fingerprints” of these factors with our new, much clearer maps to identify the primary causes, which might be different in different regions around Antarctica.


Our 18-year data set has demonstrated the value of long and continuous observations of the ice shelves, showing that shorter records cannot capture the true variability. We expect that our results will inspire new ways of thinking about how the ocean and atmosphere can affect ice shelves and, through them, ice loss from Antarctica.


The Conversation


This article was originally published on The Conversation.


Read the original article.






from EarthSky http://ift.tt/1C1e2AH

New System Watches for Things that Go Bump in the Night

Imagine taking the world’s most powerful radio telescope, used by scientists around the globe, and piping a nearly continuous data stream into your research laboratory.


That is exactly what scientists at the Naval Research Laboratory (NRL) in Washington, D.C. have done in collaboration with the National Radio Astronomy Observatory’s Karl G. Jansky Very Large Array (NRAO VLA). The newly-completed VLA Low Band Ionospheric and Transient Experiment (VLITE for short) has been built to piggyback on the $300 million dollar infrastructure of the VLA.


Radio (VLITE) and optical (SDSS) image showing the giant radio galaxy IC 711 and companions IC 708 and IC 712. All three systems are part of the distant galaxy cluster Abell 1314 and were serendipitously located in a field pointed at an unrelated low redshift galaxy. The radio data were fully processed through the VLITE pipeline and show the power of this new instrument. The field shown is the size of a full moon. (Credit: Radio (blue) from VLA Low Band Ionospheric and Transient Experiment on the NRAO VLA. Optical (red and green) from the Sloan Digital Sky Survey. U.S. Naval Research Laboratory/Dr. Tracy Clarke/Released)

Radio (VLITE) and optical (SDSS) image showing the giant radio galaxy IC 711 and companions IC 708 and IC 712. All three systems are part of the distant galaxy cluster Abell 1314 and were serendipitously located in a field pointed at an unrelated low redshift galaxy. The radio data were fully processed through the VLITE pipeline and show the power of this new instrument. The field shown is the size of a full moon.

(Photo: Radio (blue) from VLA Low Band Ionospheric and Transient Experiment on the NRAO VLA. Optical (red and green) from the Sloan Digital Sky Survey. U.S. Naval Research Laboratory/Dr. Tracy Clarke/Released)



The primary scientific driver for VLITE is real-time monitoring of ionospheric weather conditions over the U.S. southwest.



“This new system allows for continuous specification of ionospheric disturbances with remarkable precision. VLITE can detect and characterize density fluctuations as small as 30 parts per million within the total electron content along the line of sight to a cosmic source. This is akin to being at the bottom of Lake Superior and watching waves as small as 1-cm in height pass overhead. This will have a substantial impact on our understanding of ionospheric dynamics, especially the coupling between fine-scale irregularities within the lower ionosphere and larger disturbances higher up,” says NRL ionospheric lead scientist Dr. Joseph Helmboldt.



Ionospheric disturbances represent one of the most significant limitations to the performance of many radio-frequency applications like satellite-based communication and navigation (including the GPS in your phone) as well as ground-based, over-the-horizon systems (think ham radio or AM radio). While the fine-scale irregularities that VLITE is especially sensitive to aren’t large enough to make your smart phone think you are at your neighbor’s house when you’re really at home, they are quite problematic for vital remote sensing surveillance systems like over-the-horizon radar. The additional insights provided by VLITE into the nature of these ionospheric ripples will help us to better understand how to cope with their effects on such systems.


“VLITE is also a powerful new tool in our arsenal for astrophysical research” says VLITE principle investigator Dr. Namir Kassim. He points out that “We know the Universe has many secrets including mysterious blips (so-called transients) that appear and vanish like fireflies in the night. Limited observing time at classical observatories hampers our ability to understand these intriguing objects. The power of VLITE is the nearly continual data stream over a large region of the sky. This opens up a new window on the transient Universe.” At any given time, the region of the sky that VLITE peers at is so large that nearly 20 full moons would fit inside it.


Astrophysics lead scientist Dr. Tracy Clarke of NRL describes VLITE as “a symbiotic instrument that piggybacks on world-class science at the VLA. It operates as a stand-alone tool for ionospheric and astrophysical studies while at the same time VLITE provides the opportunity for enhanced science in the research program running on the VLA.”


VLITE operations started with first light on July 17, 2014 but the real fun began two days before Thanksgiving, on November 25, 2014, when VLITE moved from a commissioning phase into full scientific operations. The system operates in real-time on 10 VLA antennas and provides 64 MHz of bandwidth centered on 352 MHz with a temporal resolution of 2s and a spectral resolution of 100 kHz.


This powerful new instrument operates in parallel with the VLA and is essentially ‘driven’ around the sky by the primary science observer. Data streams off the telescope through dedicated systems that bypass normal VLA operations. The data then take two roads, one through real-time processing on computers located at the VLA site, and the other through off-line processing at NRL’s facility in Washington.


Due to the large volume of nearly continuous incoming data, all data must be analyzed by an automated pipeline that was custom designed for VLITE. Pipeline designer Dr. Wendy Lane Peters of NRL describes this process as being like “sitting in the passenger seat of a Google car and not knowing where it is taking you. VLITE is along for the ride wherever the primary science program takes us. We have to anticipate what they might do so that our pipeline is smart enough to understand the incoming data.”


Professor Bryan Gaensler, Director of the Dunlap Institute for Astronomy and Astrophysics at the University of Toronto, says that this is going to become the new way of doing astronomy.



“It’s a tragedy and a travesty that most of the information our telescopes gather from the sky is ignored and discarded. VLITE is part of a new generation of experiments that fully utilize the massive data torrents collected by the world’s most powerful observatories.”



Over the first two months of science operations, VLITE has recorded observations of sources ranging from the Sun, nearby stars and galaxies, to some of the most distant sources in the Universe. NRL astronomers and their colleagues have been poring over the pipeline images, improving their analysis pipeline and exploring the scientific potential of the instrument.


Story and information provided by the Naval Research Laboratory

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from Armed with Science http://ift.tt/19w9vQf

Imagine taking the world’s most powerful radio telescope, used by scientists around the globe, and piping a nearly continuous data stream into your research laboratory.


That is exactly what scientists at the Naval Research Laboratory (NRL) in Washington, D.C. have done in collaboration with the National Radio Astronomy Observatory’s Karl G. Jansky Very Large Array (NRAO VLA). The newly-completed VLA Low Band Ionospheric and Transient Experiment (VLITE for short) has been built to piggyback on the $300 million dollar infrastructure of the VLA.


Radio (VLITE) and optical (SDSS) image showing the giant radio galaxy IC 711 and companions IC 708 and IC 712. All three systems are part of the distant galaxy cluster Abell 1314 and were serendipitously located in a field pointed at an unrelated low redshift galaxy. The radio data were fully processed through the VLITE pipeline and show the power of this new instrument. The field shown is the size of a full moon. (Credit: Radio (blue) from VLA Low Band Ionospheric and Transient Experiment on the NRAO VLA. Optical (red and green) from the Sloan Digital Sky Survey. U.S. Naval Research Laboratory/Dr. Tracy Clarke/Released)

Radio (VLITE) and optical (SDSS) image showing the giant radio galaxy IC 711 and companions IC 708 and IC 712. All three systems are part of the distant galaxy cluster Abell 1314 and were serendipitously located in a field pointed at an unrelated low redshift galaxy. The radio data were fully processed through the VLITE pipeline and show the power of this new instrument. The field shown is the size of a full moon.

(Photo: Radio (blue) from VLA Low Band Ionospheric and Transient Experiment on the NRAO VLA. Optical (red and green) from the Sloan Digital Sky Survey. U.S. Naval Research Laboratory/Dr. Tracy Clarke/Released)



The primary scientific driver for VLITE is real-time monitoring of ionospheric weather conditions over the U.S. southwest.



“This new system allows for continuous specification of ionospheric disturbances with remarkable precision. VLITE can detect and characterize density fluctuations as small as 30 parts per million within the total electron content along the line of sight to a cosmic source. This is akin to being at the bottom of Lake Superior and watching waves as small as 1-cm in height pass overhead. This will have a substantial impact on our understanding of ionospheric dynamics, especially the coupling between fine-scale irregularities within the lower ionosphere and larger disturbances higher up,” says NRL ionospheric lead scientist Dr. Joseph Helmboldt.



Ionospheric disturbances represent one of the most significant limitations to the performance of many radio-frequency applications like satellite-based communication and navigation (including the GPS in your phone) as well as ground-based, over-the-horizon systems (think ham radio or AM radio). While the fine-scale irregularities that VLITE is especially sensitive to aren’t large enough to make your smart phone think you are at your neighbor’s house when you’re really at home, they are quite problematic for vital remote sensing surveillance systems like over-the-horizon radar. The additional insights provided by VLITE into the nature of these ionospheric ripples will help us to better understand how to cope with their effects on such systems.


“VLITE is also a powerful new tool in our arsenal for astrophysical research” says VLITE principle investigator Dr. Namir Kassim. He points out that “We know the Universe has many secrets including mysterious blips (so-called transients) that appear and vanish like fireflies in the night. Limited observing time at classical observatories hampers our ability to understand these intriguing objects. The power of VLITE is the nearly continual data stream over a large region of the sky. This opens up a new window on the transient Universe.” At any given time, the region of the sky that VLITE peers at is so large that nearly 20 full moons would fit inside it.


Astrophysics lead scientist Dr. Tracy Clarke of NRL describes VLITE as “a symbiotic instrument that piggybacks on world-class science at the VLA. It operates as a stand-alone tool for ionospheric and astrophysical studies while at the same time VLITE provides the opportunity for enhanced science in the research program running on the VLA.”


VLITE operations started with first light on July 17, 2014 but the real fun began two days before Thanksgiving, on November 25, 2014, when VLITE moved from a commissioning phase into full scientific operations. The system operates in real-time on 10 VLA antennas and provides 64 MHz of bandwidth centered on 352 MHz with a temporal resolution of 2s and a spectral resolution of 100 kHz.


This powerful new instrument operates in parallel with the VLA and is essentially ‘driven’ around the sky by the primary science observer. Data streams off the telescope through dedicated systems that bypass normal VLA operations. The data then take two roads, one through real-time processing on computers located at the VLA site, and the other through off-line processing at NRL’s facility in Washington.


Due to the large volume of nearly continuous incoming data, all data must be analyzed by an automated pipeline that was custom designed for VLITE. Pipeline designer Dr. Wendy Lane Peters of NRL describes this process as being like “sitting in the passenger seat of a Google car and not knowing where it is taking you. VLITE is along for the ride wherever the primary science program takes us. We have to anticipate what they might do so that our pipeline is smart enough to understand the incoming data.”


Professor Bryan Gaensler, Director of the Dunlap Institute for Astronomy and Astrophysics at the University of Toronto, says that this is going to become the new way of doing astronomy.



“It’s a tragedy and a travesty that most of the information our telescopes gather from the sky is ignored and discarded. VLITE is part of a new generation of experiments that fully utilize the massive data torrents collected by the world’s most powerful observatories.”



Over the first two months of science operations, VLITE has recorded observations of sources ranging from the Sun, nearby stars and galaxies, to some of the most distant sources in the Universe. NRL astronomers and their colleagues have been poring over the pipeline images, improving their analysis pipeline and exploring the scientific potential of the instrument.


Story and information provided by the Naval Research Laboratory

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Striped sunrises and the shadows they cast


View larger. | Photo by Peter Lowenstein.

View larger. | Striped sunrise by Peter Lowenstein.



Peter Lowenstein of Mutare, Zimbabwe – who recently contributed an interesting photo of straight lightning to these pages – has submitted another set of unusual photos for us. One is above, and the other is at the bottom of this post. The photos were taken a year apart, but might have been taken on the same day if two photographers had been standing back to back, one shooting a cloud-striped sunrise and the other shooting the sun’s first light – showing banded cloud shadow – shining on a nearby mountain slope. Peter wrote:



The first picture was taken almost a year ago from a high vantage point in the Bvumba Mountains looking east over Chikamba in Mozambique and shows a glorious sun striped by rising through thin layers of early morning cloud and mist on the horizon. I captured it at 5:57 a.m. using a Panasonic Lumix DMC-TZ10 compact camera in sunset mode and x16 zoom setting.


The second picture was taken at sunrise yesterday morning (March 29, 2015) from the verandah of my house and shows alternate stripes of bright orange sunlight and the dark shadows of a thin strip of cloud and the eastern horizon being projected by the sun onto Murawa Mountain a few kilometers to the west. This spectacle lasted less than a minute before being faded by larger clouds passing in front of the sun. It was captured at 6:10 a.m. using a Panasonic Lumix DMC-TZ60 compact camera in sunset mode and x2 zoom setting.



Thank you, Peter! Interesting indeed.


View larger. | Photo by Peter Lowenstein.

View larger. | Striped sunrise’s shadow by Peter Lowenstein.



Bottom line: Peter Lowenstein in Zimbabwe took these photos a year apart. One shows a sunrise striped with cloud, and the other shows cloud-striped sunrise’s cloud shadow.


Only two weeks left in our annual fund-raising campaign! Have you donated yet? Help EarthSky keep going.






from EarthSky http://ift.tt/1BGRC7Y

View larger. | Photo by Peter Lowenstein.

View larger. | Striped sunrise by Peter Lowenstein.



Peter Lowenstein of Mutare, Zimbabwe – who recently contributed an interesting photo of straight lightning to these pages – has submitted another set of unusual photos for us. One is above, and the other is at the bottom of this post. The photos were taken a year apart, but might have been taken on the same day if two photographers had been standing back to back, one shooting a cloud-striped sunrise and the other shooting the sun’s first light – showing banded cloud shadow – shining on a nearby mountain slope. Peter wrote:



The first picture was taken almost a year ago from a high vantage point in the Bvumba Mountains looking east over Chikamba in Mozambique and shows a glorious sun striped by rising through thin layers of early morning cloud and mist on the horizon. I captured it at 5:57 a.m. using a Panasonic Lumix DMC-TZ10 compact camera in sunset mode and x16 zoom setting.


The second picture was taken at sunrise yesterday morning (March 29, 2015) from the verandah of my house and shows alternate stripes of bright orange sunlight and the dark shadows of a thin strip of cloud and the eastern horizon being projected by the sun onto Murawa Mountain a few kilometers to the west. This spectacle lasted less than a minute before being faded by larger clouds passing in front of the sun. It was captured at 6:10 a.m. using a Panasonic Lumix DMC-TZ60 compact camera in sunset mode and x2 zoom setting.



Thank you, Peter! Interesting indeed.


View larger. | Photo by Peter Lowenstein.

View larger. | Striped sunrise’s shadow by Peter Lowenstein.



Bottom line: Peter Lowenstein in Zimbabwe took these photos a year apart. One shows a sunrise striped with cloud, and the other shows cloud-striped sunrise’s cloud shadow.


Only two weeks left in our annual fund-raising campaign! Have you donated yet? Help EarthSky keep going.






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Moon close to Regulus on March 31


Tonight – March 31, 2015 – can you find the star that’s shining close to the big and bright waxing gibbous moon? That’s Regulus, the brightest star in the constellation Leo the Lion. In sky lore, Regulus is considered to be the Lion’s Heart. Regulus is also the only first-magnitude star to sit almost exactly on the ecliptic – the Earth’s orbital plane projected outward onto the sphere of stars. We often show the ecliptic on our sky charts, because the moon and planets are always found on it, or near it.


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Don’t mistake the planet Jupiter, that much brighter starlike object in the moon’s vicinity, for Regulus. Although Regulus ranks as a first-magnitude star, it pales next to Jupiter, the fourth-brightest celestial object to adorn the heavens, after the sun, moon and Venus. (Venus is seen in the west after sunset.) In fact, Jupiter shines about 30 times more brightly than Regulus does.



An imaginary line drawn between the pointer stars in the Big Dipper – the two outer stars in the Dipper’s bowl – points in one direction toward Polaris, the North Star, and in the opposite direction toward Leo.



Use the moon to find Regulus tonight. Then you can refer to the “pointer stars” of the Big Dipper to locate Regulus on any night. The two outer stars making up the bowl of the Big Dipper point northward to Polaris, the North Star, and southward to the constellation Leo and its brightest star, Regulus. See illustration at left.


Regulus and three other 1st-magnitude stars reside close enough to the ecliptic to be occulted – covered over – by the moon on occasion: Regulus, Spica, Antares, and Aldebaran. In fact, the last lunar occultation of Regulus happened on May 12, 2008, and the next one will be on December 18, 2016.


Lunar occultations of bright stars are not terribly uncommon. A series of monthly occultations of Aldebaran began on January 29, 2015, and will end on September 3, 2018. Then Regulus will present a series of monthly occultations from December 18, 2016 to April 24, 2018, followed by a series of Antares’ occultations from August 25, 2023 to August 27, 2028.


An occultation of a first-magnitude star by a planet is extremely rare. The last time a planet occulted a first-magnitude star was when Venus occulted Regulus on July 7, 1959. The next time will be when Venus occults Regulus on October 1, 2044.


Before 1959, the most recent planet/first-magnitude star occultation took place on November 10, 1783, when Venus occulted Spica. Venus will again occult Spica on September 2, 2197.


Bottom line: Tonight – March 31, 2015 – the moon shines close to Leo’s brightest star, Regulus, the only 1st-magnitude star to sit almost exactly on the ecliptic.


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/1CrGjEe

Tonight – March 31, 2015 – can you find the star that’s shining close to the big and bright waxing gibbous moon? That’s Regulus, the brightest star in the constellation Leo the Lion. In sky lore, Regulus is considered to be the Lion’s Heart. Regulus is also the only first-magnitude star to sit almost exactly on the ecliptic – the Earth’s orbital plane projected outward onto the sphere of stars. We often show the ecliptic on our sky charts, because the moon and planets are always found on it, or near it.


Only two weeks left in our annual fund-raising campaign! Have you donated yet? Help EarthSky keep going.



Don’t mistake the planet Jupiter, that much brighter starlike object in the moon’s vicinity, for Regulus. Although Regulus ranks as a first-magnitude star, it pales next to Jupiter, the fourth-brightest celestial object to adorn the heavens, after the sun, moon and Venus. (Venus is seen in the west after sunset.) In fact, Jupiter shines about 30 times more brightly than Regulus does.



An imaginary line drawn between the pointer stars in the Big Dipper – the two outer stars in the Dipper’s bowl – points in one direction toward Polaris, the North Star, and in the opposite direction toward Leo.



Use the moon to find Regulus tonight. Then you can refer to the “pointer stars” of the Big Dipper to locate Regulus on any night. The two outer stars making up the bowl of the Big Dipper point northward to Polaris, the North Star, and southward to the constellation Leo and its brightest star, Regulus. See illustration at left.


Regulus and three other 1st-magnitude stars reside close enough to the ecliptic to be occulted – covered over – by the moon on occasion: Regulus, Spica, Antares, and Aldebaran. In fact, the last lunar occultation of Regulus happened on May 12, 2008, and the next one will be on December 18, 2016.


Lunar occultations of bright stars are not terribly uncommon. A series of monthly occultations of Aldebaran began on January 29, 2015, and will end on September 3, 2018. Then Regulus will present a series of monthly occultations from December 18, 2016 to April 24, 2018, followed by a series of Antares’ occultations from August 25, 2023 to August 27, 2028.


An occultation of a first-magnitude star by a planet is extremely rare. The last time a planet occulted a first-magnitude star was when Venus occulted Regulus on July 7, 1959. The next time will be when Venus occults Regulus on October 1, 2044.


Before 1959, the most recent planet/first-magnitude star occultation took place on November 10, 1783, when Venus occulted Spica. Venus will again occult Spica on September 2, 2197.


Bottom line: Tonight – March 31, 2015 – the moon shines close to Leo’s brightest star, Regulus, the only 1st-magnitude star to sit almost exactly on the ecliptic.


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/1CrGjEe

Ancient cancer [Respectful Insolence]

As I sat on my couch last night, laptop sitting in front of me, I awaited the Ken Burns adaptation of Siddartha Mukherjee’s excellent book The Emperor of All Maladies into a three part television documentary to air on PBS. I’m not sure whether I’ll blog the show or not, but if I do I’ll probably wait until all three episodes have aired. In the meantime, this seems as good a time as any to go back to a story that I saw a week ago but somehow, thanks to grants, traveling to Houston, and other distractions that I wanted to blog about more, never got around to. Since The Emperor of All Maladies, the book at least, is billed as “a biography of cancer,” I’d indulge my interest in ancient medicine, including ancient Egyptian medicine starting when I first wrote about the Edwin Smith papyrus, which I saw at the Metropolitan Museum of Art in New York nearly ten years ago.


If there’s one claim that irritates me that various proponents of alternative medicine like to make, it’s that cancer is a “modern” disease, that it was rare (or even didn’t exist) before the rise of modern societies, particularly the industrial revolution. This viewpoint bubbled up five years ago, when a commentary in Nature Reviews Cancer (yep, the same journal in which I published my opinion piece on integrative oncology a few months ago) that argued strongly that cancer was almost unknown (or at least very rare) in the ancient world based on the lack of finding it in mummies in Egypt and South America. They also looked at ancient texts and literature from Egypt and Greece, and say that there’s little sign that cancer was a common ailment. After all, cancer is mainly a disease of the elderly, with three-quarters of cases being diagnosed in people over 60 and more than a third of cases diagnosed in people 75 or older. Life expectancy was much shorter in ancient times; so relatively few people made it to cancer-prone ages. Most probably didn’t make it past age 40.



In any case, what caught my attention was a story reporting the finding of the oldest example of breast cancer:



Researchers working in Egypt say they have found the oldest example of breast cancer in the 4,200-year-old remains of an Egyptian woman — a discovery that casts further doubt on the common perception of cancer as a modern disease associated with today’s lifestyles.



Here’s the announcement from the Egyptian Ministry of Antiquities:







Ministry of AntiquitiesPress Office——————————–Evidenced in Egypt : the oldest breast cancer in…


Posted by Ministry of Antiquities on Tuesday, March 24, 2015





See:



Antiquities Minister, Dr. Mamdouh el-Damaty announces the discovery of the oldest evidence of breast cancer in the world. This discovery was made along the seventh archaeological season carried out by University of Jaen (Spain) in the necropolis of Qubbet el-Hawa (West Asuan). Dr. Miguel Botella (University of Granada) and his team of anthropologists have identified on the bones of an adult woman an extraordinary deterioration in all her skeleton. The study of her remains shows the typical destructive damages provoked by the extension of a breast cancer as a metastasis in the bones.


The team from University of Jaen has confirmed that the woman lived at the end of the 6th Dynasty (2200 BCE) and was part of the élite of the southernmost town of Egypt, Elephantine. The virulence of the disease impeded her to carry out any kind of labor, but she was treated and taken care during a long period until her death.



It turns out that the apparently low incidence of cancer in mummies, skeletons, and other ancient remains might be an illusion. For example, investigators from the United Kingdom reported a year ago on the case of 3,000 year old skeleton found in Sudan of a man who appeared to have had metastatic prostate cancer, which they published in PLoS One by Michaela Binder and colleagues. It was the oldest complete example of a skeleton of an ancient human with cancer. The authors wrote:



The apparent absence of cancer in archaeological remains may also partly be an illusion created by issues of bone preservation, and due to the fact that methods of analysis are inadequate to detect initial changes within bone. Due to financial, time and logistical reasons, human remains are usually not systematically radiographed, and bone metastases originating in cancellous tissue only penetrate the bone surface in their advanced stages. If the immune system was already compromised by other negative influences in a person’s life, people may not have survived long enough to develop full skeletal metastases. Thus, evidence for a large proportion of tumours could be missed when skeletal remains are analysed [72]. Another challenge in detecting cancer in ancient human remains is the poor preservation of bone which often prevents the clear identification of lytic lesions and precludes the diagnosis of incomplete remains [27]. With increasing numbers of skeletal collections and more detailed analysis, as well as more readily available standard radiographic equipment, the evidence for cancer in antiquity could increase significantly.



In other words, for the most part, archaeologists haven’t been looking carefully for evidence of cancer in ancient remains, and if you don’t look for something you aren’t very likely to find it. Moreover, it’s not at all straightforward to find and confirm evidence of cancer in remains that are usually just skeletons and usually just fragments of skeletons at that. Comparatively speaking, there aren’t that many mummies and not that many remains with soft tissue that can be examined for evidence of cancer. In this case, the Binder et al studied the skeleton of a man aged 25-35 years recovered in 2013 from Amara West. It was found in a tomb with characteristics that suggest what the authors referred to as a “sub-elite” buried according to Egyptian customs.


The authors examined the bones and found lytic lesions (lesions that eat away bone tissue) affecting the ribs, vertebrae, clavicle, scapulae, pelvis, sternum, humeral and femoral heads of skeleton. Such lesions are very characteristic of some sorts of cancer metastases to bone. Radiographic, scanning electron microscope (SEM) images, and microscopic images were taken of the lesions, and a differential diagnosis constructed. The lesions were most consistent with bony metastases, but the authors had to rule out other potential causes of lytic lesions. These include metastatic carcinoma, multiple myeloma (a cancer of the plasma cells of the bone marrow that can produce lesions very similar to metastatic carcinoma), fungal infections, and taphonomic damage. Taphonomy is the study of what happens to an organism after its death and until its discovery as a fossil, including decomposition, post-mortem transport, burial, compaction, and other chemical, biologic, or physical activity which affects the remains of the organism. About this last possibility, the authors noted that “mall round holes similar to metastatic lesions can be caused by a variety of factors including roots, water, and termites [68] or dermatid beetles [69].” SEM examination, however, found characteristics more consistent with metastatic carcinoma than with any of the other things that can cause taphonomic damage.


The authors also reiterate:



The lack of evidence for cancer in antiquity may to a large extent, be the result of reduced life expectancy, and thus less time to develop skeletal lesions if the immune system is already compromised by an inadequate supply of nutrients and diseases. This represents one of the major problems in inferring the absence or presence of disease in the past in general [87]. The archaeological and historical record certainly provides plenty of evidence for possible causes of developing cancer. Despite recent advances, the genetic background for cancer predisposition is still far from being understood today [88], [89]. Even though it may perhaps remain unknown, there is no reason to assume that predisposing genetic factors were not present in the past. The man from Amara West does indicate that it was indeed possible to develop skeletal lesions of cancer, provides a glimpse into one individual’s life experience, and cautions against claims for the absence, or presence, of any disease based on skeletal evidence alone.



Besides, there’s also evidence that cancer has been with us since prehistoric times. For instance, there was Kanam Man, whose fossilized jawbone was found by Louis Leakey back in 1932, who called it, “Not only the oldest known human fragment from Africa, but the most ancient fragment of true Homo yet discovered anywhere in the world.” Kanam Man was controversial at the time, specifically whether it was what Leakey proclaimed it, but it also had an unusual feature:



At the time of the discovery, it had seemed like a bother, detracting from Leakey’s find. He was working in his rooms at St. John’s College at the University of Cambridge, carefully cleaning the specimen, when he felt a lump. He thought it was a rock. But as he kept picking, he could see that the lump was part of the fossilized jaw. He sent it to a specialist on mandibular abnormalities at the Royal College of Surgeons of England, who diagnosed it as osteosarcoma — a cancer of the bone.


Others have not been as certain. As recently as 2007, scientists scanning the mandible with an electron microscope concluded that this was indeed a case of “bone run amok” while remaining neutral on the nature of the pathology.



Of course, from a science-based perspective, none of this should be surprising. We might argue over how large a contribution of random chance there is to the development of cancer, but there’s little doubt that there is a large random component to it, a component of what can be called, for lack of a better term, “bad luck.” And, although cancer is primarily a disease of the elderly, young people can and do get it. As for cancer caused by the environment, there were also a lot of things that ancient humans encountered that could cause cancer: Sunlight leading to melanoma, infections that can cause cancer, radon, naturally occurring chemicals. The ancient world was hardly as pristine as it’s envisioned.


It’s not just cancer, either. Advocates of “paleo” diets, which, accurately or not, are designed to mimic what our paleolithic ancestors ate, frequently claim that heart disease would be virtually nonexistent if we all ate that way. Of course, as I’ve described on more than one occasion, ancient humans were prone to atherosclerotic heart disease as well. In fact, the evidence we have suggests that, for example, ancient Egyptians were prone to all manner of illnesses.


When it comes to cancer, in 1600 BC the Egyptian physician who wrote the Edwin Smith papyrus recommended cauterization of breast cancer with a tool called the “fire drill.” He also wrote about the disease, “There is no treatment.” If there’s one big difference between humans now and humans thousands of years ago, it was not biology or the factors that cause us to develop cancer. It was that there was no treatment. Now there is. What I’ve seen of The Emperor of All Maladies thus far demonstrates this.






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As I sat on my couch last night, laptop sitting in front of me, I awaited the Ken Burns adaptation of Siddartha Mukherjee’s excellent book The Emperor of All Maladies into a three part television documentary to air on PBS. I’m not sure whether I’ll blog the show or not, but if I do I’ll probably wait until all three episodes have aired. In the meantime, this seems as good a time as any to go back to a story that I saw a week ago but somehow, thanks to grants, traveling to Houston, and other distractions that I wanted to blog about more, never got around to. Since The Emperor of All Maladies, the book at least, is billed as “a biography of cancer,” I’d indulge my interest in ancient medicine, including ancient Egyptian medicine starting when I first wrote about the Edwin Smith papyrus, which I saw at the Metropolitan Museum of Art in New York nearly ten years ago.


If there’s one claim that irritates me that various proponents of alternative medicine like to make, it’s that cancer is a “modern” disease, that it was rare (or even didn’t exist) before the rise of modern societies, particularly the industrial revolution. This viewpoint bubbled up five years ago, when a commentary in Nature Reviews Cancer (yep, the same journal in which I published my opinion piece on integrative oncology a few months ago) that argued strongly that cancer was almost unknown (or at least very rare) in the ancient world based on the lack of finding it in mummies in Egypt and South America. They also looked at ancient texts and literature from Egypt and Greece, and say that there’s little sign that cancer was a common ailment. After all, cancer is mainly a disease of the elderly, with three-quarters of cases being diagnosed in people over 60 and more than a third of cases diagnosed in people 75 or older. Life expectancy was much shorter in ancient times; so relatively few people made it to cancer-prone ages. Most probably didn’t make it past age 40.



In any case, what caught my attention was a story reporting the finding of the oldest example of breast cancer:



Researchers working in Egypt say they have found the oldest example of breast cancer in the 4,200-year-old remains of an Egyptian woman — a discovery that casts further doubt on the common perception of cancer as a modern disease associated with today’s lifestyles.



Here’s the announcement from the Egyptian Ministry of Antiquities:







Ministry of AntiquitiesPress Office——————————–Evidenced in Egypt : the oldest breast cancer in…


Posted by Ministry of Antiquities on Tuesday, March 24, 2015





See:



Antiquities Minister, Dr. Mamdouh el-Damaty announces the discovery of the oldest evidence of breast cancer in the world. This discovery was made along the seventh archaeological season carried out by University of Jaen (Spain) in the necropolis of Qubbet el-Hawa (West Asuan). Dr. Miguel Botella (University of Granada) and his team of anthropologists have identified on the bones of an adult woman an extraordinary deterioration in all her skeleton. The study of her remains shows the typical destructive damages provoked by the extension of a breast cancer as a metastasis in the bones.


The team from University of Jaen has confirmed that the woman lived at the end of the 6th Dynasty (2200 BCE) and was part of the élite of the southernmost town of Egypt, Elephantine. The virulence of the disease impeded her to carry out any kind of labor, but she was treated and taken care during a long period until her death.



It turns out that the apparently low incidence of cancer in mummies, skeletons, and other ancient remains might be an illusion. For example, investigators from the United Kingdom reported a year ago on the case of 3,000 year old skeleton found in Sudan of a man who appeared to have had metastatic prostate cancer, which they published in PLoS One by Michaela Binder and colleagues. It was the oldest complete example of a skeleton of an ancient human with cancer. The authors wrote:



The apparent absence of cancer in archaeological remains may also partly be an illusion created by issues of bone preservation, and due to the fact that methods of analysis are inadequate to detect initial changes within bone. Due to financial, time and logistical reasons, human remains are usually not systematically radiographed, and bone metastases originating in cancellous tissue only penetrate the bone surface in their advanced stages. If the immune system was already compromised by other negative influences in a person’s life, people may not have survived long enough to develop full skeletal metastases. Thus, evidence for a large proportion of tumours could be missed when skeletal remains are analysed [72]. Another challenge in detecting cancer in ancient human remains is the poor preservation of bone which often prevents the clear identification of lytic lesions and precludes the diagnosis of incomplete remains [27]. With increasing numbers of skeletal collections and more detailed analysis, as well as more readily available standard radiographic equipment, the evidence for cancer in antiquity could increase significantly.



In other words, for the most part, archaeologists haven’t been looking carefully for evidence of cancer in ancient remains, and if you don’t look for something you aren’t very likely to find it. Moreover, it’s not at all straightforward to find and confirm evidence of cancer in remains that are usually just skeletons and usually just fragments of skeletons at that. Comparatively speaking, there aren’t that many mummies and not that many remains with soft tissue that can be examined for evidence of cancer. In this case, the Binder et al studied the skeleton of a man aged 25-35 years recovered in 2013 from Amara West. It was found in a tomb with characteristics that suggest what the authors referred to as a “sub-elite” buried according to Egyptian customs.


The authors examined the bones and found lytic lesions (lesions that eat away bone tissue) affecting the ribs, vertebrae, clavicle, scapulae, pelvis, sternum, humeral and femoral heads of skeleton. Such lesions are very characteristic of some sorts of cancer metastases to bone. Radiographic, scanning electron microscope (SEM) images, and microscopic images were taken of the lesions, and a differential diagnosis constructed. The lesions were most consistent with bony metastases, but the authors had to rule out other potential causes of lytic lesions. These include metastatic carcinoma, multiple myeloma (a cancer of the plasma cells of the bone marrow that can produce lesions very similar to metastatic carcinoma), fungal infections, and taphonomic damage. Taphonomy is the study of what happens to an organism after its death and until its discovery as a fossil, including decomposition, post-mortem transport, burial, compaction, and other chemical, biologic, or physical activity which affects the remains of the organism. About this last possibility, the authors noted that “mall round holes similar to metastatic lesions can be caused by a variety of factors including roots, water, and termites [68] or dermatid beetles [69].” SEM examination, however, found characteristics more consistent with metastatic carcinoma than with any of the other things that can cause taphonomic damage.


The authors also reiterate:



The lack of evidence for cancer in antiquity may to a large extent, be the result of reduced life expectancy, and thus less time to develop skeletal lesions if the immune system is already compromised by an inadequate supply of nutrients and diseases. This represents one of the major problems in inferring the absence or presence of disease in the past in general [87]. The archaeological and historical record certainly provides plenty of evidence for possible causes of developing cancer. Despite recent advances, the genetic background for cancer predisposition is still far from being understood today [88], [89]. Even though it may perhaps remain unknown, there is no reason to assume that predisposing genetic factors were not present in the past. The man from Amara West does indicate that it was indeed possible to develop skeletal lesions of cancer, provides a glimpse into one individual’s life experience, and cautions against claims for the absence, or presence, of any disease based on skeletal evidence alone.



Besides, there’s also evidence that cancer has been with us since prehistoric times. For instance, there was Kanam Man, whose fossilized jawbone was found by Louis Leakey back in 1932, who called it, “Not only the oldest known human fragment from Africa, but the most ancient fragment of true Homo yet discovered anywhere in the world.” Kanam Man was controversial at the time, specifically whether it was what Leakey proclaimed it, but it also had an unusual feature:



At the time of the discovery, it had seemed like a bother, detracting from Leakey’s find. He was working in his rooms at St. John’s College at the University of Cambridge, carefully cleaning the specimen, when he felt a lump. He thought it was a rock. But as he kept picking, he could see that the lump was part of the fossilized jaw. He sent it to a specialist on mandibular abnormalities at the Royal College of Surgeons of England, who diagnosed it as osteosarcoma — a cancer of the bone.


Others have not been as certain. As recently as 2007, scientists scanning the mandible with an electron microscope concluded that this was indeed a case of “bone run amok” while remaining neutral on the nature of the pathology.



Of course, from a science-based perspective, none of this should be surprising. We might argue over how large a contribution of random chance there is to the development of cancer, but there’s little doubt that there is a large random component to it, a component of what can be called, for lack of a better term, “bad luck.” And, although cancer is primarily a disease of the elderly, young people can and do get it. As for cancer caused by the environment, there were also a lot of things that ancient humans encountered that could cause cancer: Sunlight leading to melanoma, infections that can cause cancer, radon, naturally occurring chemicals. The ancient world was hardly as pristine as it’s envisioned.


It’s not just cancer, either. Advocates of “paleo” diets, which, accurately or not, are designed to mimic what our paleolithic ancestors ate, frequently claim that heart disease would be virtually nonexistent if we all ate that way. Of course, as I’ve described on more than one occasion, ancient humans were prone to atherosclerotic heart disease as well. In fact, the evidence we have suggests that, for example, ancient Egyptians were prone to all manner of illnesses.


When it comes to cancer, in 1600 BC the Egyptian physician who wrote the Edwin Smith papyrus recommended cauterization of breast cancer with a tool called the “fire drill.” He also wrote about the disease, “There is no treatment.” If there’s one big difference between humans now and humans thousands of years ago, it was not biology or the factors that cause us to develop cancer. It was that there was no treatment. Now there is. What I’ve seen of The Emperor of All Maladies thus far demonstrates this.






from ScienceBlogs http://ift.tt/1GI3TQ5

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