New research shows the world’s ice is doing something not seen before

In this warming world, some parts of the planet are warming much faster than others.  The warming is causing large ice bodies to start to melt and move rapidly, in some cases sliding into the ocean. 

This movement is the topic of a very new scientific study that was just published in the journal Earth and Planetary Science Letters.  The Arctic is warming much faster than other parts of the planet and the ice there is showing the signs of rapid warming.  This fact has serious consequences. First, melting ice can cause sea levels to rise and inundate coastal areas – it also makes storms like hurricanes and typhoons more destructive.  Melting ice also causes a feedback loop, which can cause more future warming and then more ice loss.

It should be noted that there are different types of ice.  Some ice floats on water and is called sea ice.  When it melts, the ocean water level hardly budges because the ice is already in the sea displacing liquid water.  But, sea ice is really important for this feedback loop I mentioned above.

Other ice is on land and may be a large ice sheet or a smaller glacier.  These ice bodies sit atop the land and “rest” there.  In some cases, they extend out off the land and into the ocean where they partly float on liquid water.  When this land ice melts, the liquid flows into the oceans and can cause significant ocean level rising.

So, the importance of ice depends on what type it is, where it is located, and how fast it is melting. And this brings us to the new paper.

The researchers looked at a type of high latitude glacier in their study.  These glaciers hold enough water to cause about 1 foot (about a third of a meter) in sea level rise. Typically, they exist in cold and dry areas, where snowfall is limited. 

How do glaciers move?  Well really by either sliding over the underlying bedrock or surface that they sit on, or by deforming and stretching under their weight. The colder glaciers tend to move by the deforming and stretching process.  Glaciers that have wetter and more temperate regions involve more sliding.  But regardless of how they move, these glaciers, particularly the glaciers that have both cold and temperate parts, experience surges in their motion.  These surges are short duration times where the glacier moves a lot.  During a surge, ice is redistributed from one part of the glacier to another region.

The authors in this study observed such a glacier surge.  It happened at an outlet glacier that is mainly of the “cold” type in Russia.  At the Vavilov Ice Cap on October Revolution Island, the authors find it “is undergoing extraordinary acceleration and thinning but displays no previous evidence of surging.”  The authors write,

the 300-600 meter thick 1820 square kilometer Vavilov Ice Cap is frozen to its bed over the majority of its area, apart from a region along its western margin where basal sliding is potentially important for faster flow.

In 2010 the ice in the region began to accelerate and the next year, crevasses were observed that matched the patterns of ice acceleration. The researchers were able to watch this surge in ice motion in real-time using satellite images. They could track the motion and show the incredible speed of flow. 

What caused the rapid motion? This is an important question because if the motion is caused by human warming, we can expect the behavior to be repeated elsewhere as temperatures rise.  Importantly both air and ocean-water temperatures could be a factor.  One potential cause is surface meltwater.  The top of the ice can melt, and liquid water then can flow downwards, into the ice through cracks and holes.  This flowing water can precondition the ice for rapid motion.

This fact may be a contributing cause to the motion.  Basically, the melted water lubricated the ice/ground interface causing more sliding and more friction.  The friction caused some of the bottom ice to melt and released more liquid water, and a cycle had begun.

The researchers also took measurements of elevation to better understand areas where ice was becoming thicker or thinner.  In addition, they studied the forces that exist within the ice itself to help elucidate the cause of the increased speed. Obviously, this is an evolving area of study and all of the questions have not yet been answered.  However, I was impressed when I read that even though these types of surges are becoming more common, what the researchers observed in Russia was still unique.  They describe the rate of ice loss at Vavilov as “extreme.” The authors also point out,

Click here to read the rest



from Skeptical Science https://ift.tt/2y0iirQ

In this warming world, some parts of the planet are warming much faster than others.  The warming is causing large ice bodies to start to melt and move rapidly, in some cases sliding into the ocean. 

This movement is the topic of a very new scientific study that was just published in the journal Earth and Planetary Science Letters.  The Arctic is warming much faster than other parts of the planet and the ice there is showing the signs of rapid warming.  This fact has serious consequences. First, melting ice can cause sea levels to rise and inundate coastal areas – it also makes storms like hurricanes and typhoons more destructive.  Melting ice also causes a feedback loop, which can cause more future warming and then more ice loss.

It should be noted that there are different types of ice.  Some ice floats on water and is called sea ice.  When it melts, the ocean water level hardly budges because the ice is already in the sea displacing liquid water.  But, sea ice is really important for this feedback loop I mentioned above.

Other ice is on land and may be a large ice sheet or a smaller glacier.  These ice bodies sit atop the land and “rest” there.  In some cases, they extend out off the land and into the ocean where they partly float on liquid water.  When this land ice melts, the liquid flows into the oceans and can cause significant ocean level rising.

So, the importance of ice depends on what type it is, where it is located, and how fast it is melting. And this brings us to the new paper.

The researchers looked at a type of high latitude glacier in their study.  These glaciers hold enough water to cause about 1 foot (about a third of a meter) in sea level rise. Typically, they exist in cold and dry areas, where snowfall is limited. 

How do glaciers move?  Well really by either sliding over the underlying bedrock or surface that they sit on, or by deforming and stretching under their weight. The colder glaciers tend to move by the deforming and stretching process.  Glaciers that have wetter and more temperate regions involve more sliding.  But regardless of how they move, these glaciers, particularly the glaciers that have both cold and temperate parts, experience surges in their motion.  These surges are short duration times where the glacier moves a lot.  During a surge, ice is redistributed from one part of the glacier to another region.

The authors in this study observed such a glacier surge.  It happened at an outlet glacier that is mainly of the “cold” type in Russia.  At the Vavilov Ice Cap on October Revolution Island, the authors find it “is undergoing extraordinary acceleration and thinning but displays no previous evidence of surging.”  The authors write,

the 300-600 meter thick 1820 square kilometer Vavilov Ice Cap is frozen to its bed over the majority of its area, apart from a region along its western margin where basal sliding is potentially important for faster flow.

In 2010 the ice in the region began to accelerate and the next year, crevasses were observed that matched the patterns of ice acceleration. The researchers were able to watch this surge in ice motion in real-time using satellite images. They could track the motion and show the incredible speed of flow. 

What caused the rapid motion? This is an important question because if the motion is caused by human warming, we can expect the behavior to be repeated elsewhere as temperatures rise.  Importantly both air and ocean-water temperatures could be a factor.  One potential cause is surface meltwater.  The top of the ice can melt, and liquid water then can flow downwards, into the ice through cracks and holes.  This flowing water can precondition the ice for rapid motion.

This fact may be a contributing cause to the motion.  Basically, the melted water lubricated the ice/ground interface causing more sliding and more friction.  The friction caused some of the bottom ice to melt and released more liquid water, and a cycle had begun.

The researchers also took measurements of elevation to better understand areas where ice was becoming thicker or thinner.  In addition, they studied the forces that exist within the ice itself to help elucidate the cause of the increased speed. Obviously, this is an evolving area of study and all of the questions have not yet been answered.  However, I was impressed when I read that even though these types of surges are becoming more common, what the researchers observed in Russia was still unique.  They describe the rate of ice loss at Vavilov as “extreme.” The authors also point out,

Click here to read the rest



from Skeptical Science https://ift.tt/2y0iirQ

New research, September 17-23, 2018

A selection of new climate related research articles is shown below.

Climate change impacts 

Mankind

Bayesian estimates for the mapping of dengue hotspots and estimation of the risk of disease epidemic in Northeast Brazil

Effects of climate change-related heat stress on labor productivity in South Korea

Climatic preferences for beach tourism: an empirical study on Greek islands

Estimation of economic losses from tropical cyclones in China at 1.5 °C and 2.0 °C warming using the regional climate model COSMO‐CLM

Mapping the need for adaptation: assessing drought vulnerability using the livelihood vulnerability index approach in a mid-hill region of Nepal

Unavoidable solutions for coastal adaptation in Reunion Island (Indian Ocean)

Co-producing UK climate change adaptation policy: An analysis of the 2012 and 2017 UK Climate Change Risk Assessments

Behavioral adaptation to climate change in wildfire‐prone forests

Assessing real options in urban surface water flood risk management under climate change (open access)

Climate change impact on Mexico wheat production

Global Freshwater Availability Below Normal Conditions and Population Impact Under 1.5 and 2 °C Stabilization Scenarios

Climate change as a motivating factor for farm-adjustments: rethinking the link (open access)

Ratooning as an adaptive management tool for climatic change in rice systems along a north-south transect in the southern Mississippi valley

Biosphere

Corals sustain growth but not skeletal density across the Florida Keys Reef Tract despite ongoing warming

Depth‐Dependent Thermal Stress Around Corals in the Tropical Pacific Ocean

The influence of weather on avian spring migration phenology: What, where, and when?

Linking permafrost thaw to shifting biogeochemistry and food web resources in an arctic river

Temperature niche position and breadth of ectomycorrhizal fungi: reduced diversity under warming predicted by a nested community structure

Overlooked climate parameters best predict flowering onset: assessing phenological models using the elastic net

Moisture‐mediated responsiveness of treeline shifts to global warming in the Himalayas (open access)

Pushing the limit: Resilience of an Arctic copepod to environmental fluctuations (open access)

Resource limitation alters effects of phenological shifts on inter-specific competition

Climatically controlled reproduction drives interannual growth variability in a temperate tree species

Land‐surface greening suggests vigorous woody regrowth throughout European semi‐natural vegetation

Fire, fragmentation, and windstorms: a recipe for tropical forest degradation

Vegetation‐climate interactions on the Loess Plateau: a non‐linear Granger causality analysis

Cascading effects from plants to soil microorganisms explain how plant species richness and simulated climate change affect soil multifunctionality

Other impacts

Spatiotemporal trends of area burnt in the Iberian Peninsula, 1975–2013

Climate change mitigation 

Climate Policy

Renewable and low carbon technologies policy

Designing China’s national carbon emissions trading system in a transitional period (open access)

Energy production

From collapsed coal mines to floating solar farms, why China's new power stations matter

Emission savings

How big is the energy efficiency resource? (open access)

Multi‐year net ecosystem carbon balance of a restored peatland reveals a return to carbon sink

Chinese cropping systems are a net source of greenhouse gases despite soil carbon sequestration (open access)

Are capitalists green? Firm ownership and provincial CO2emissions in China

Geoengineering

Stopping the flood: could we use targeted geoengineering to mitigate sea level rise? (open access)

Climate change

Temperature, precipitation, wind

The Global Historical Climatology Network Monthly Temperature Dataset, Version 4

Quality control and homogenization of the Belgian historical temperature data

What caused the record‐breaking warming in East China Seas during August 2016? (open access)

Trends of climate change indices in some Mexican cities from 1980 to 2010

Extreme events

Exacerbation of the 2013–2016 Pan‐Caribbean Drought by Anthropogenic Warming

Characteristics and risk analysis of hydrological disaster events from 1949 to 2015 in Urumqi, China

Extreme temperature events on the Iberian Peninsula: Statistical trajectory analysis and synoptic patterns

Climate change risks for severe storms in developing countries in the context of poverty and inequality in Cambodia

Impact of forecasted land use changes on flood risk in the Polish Carpathians (open access)

Comparison of agricultural stakeholder survey results and drought monitoring datasets during the 2016 U.S. Northern Plains flash drought

Regime shift in the destructiveness of tropical cyclones over the western North Pacific

Effect of climatic oscillations on flood occurrence on Papaloapan River, México, during the 1550–2000 period

Tropical cyclone projections: Changing climate threats for Pacific Island defense installations

Likelihood of concurrent climate extremes and variations over China (open access)

A Recent Reversal in the Poleward Shift of Western North Pacific Tropical Cyclones

Changes in the spatial–temporal patterns of droughts in the Brazilian Northeast (open access)

Forcings and feedbacks

Globally significant CO2 emissions from Katla, a subglacial volcano in Iceland

Natural and anthropogenic contributions to long-term variations of SO2, NO2, CO, and AOD over East China

Can Climate Models Reproduce the Decadal Change of Dust Aerosol in East Asia?

Cryosphere

Massive destabilization of an Arctic ice cap

Surface pond energy absorption across four Himalayan glaciers accounts for 1/8 of total catchment ice loss

Atlantic salinity budget in response to Northern and Southern Hemisphere ice sheet discharge (open access)

Seasonal mass variations show timing and magnitude of meltwater storage in the Greenland Ice Sheet (open access)

Atmospheric and oceanic circulation

Transient Response of the Gulf Stream to Multiple Hurricanes in 2017

Gulf Stream variability in the context of quasi‐decadal and multi‐decadal Atlantic climate variability

Impact of the Atlantic Multidecadal Oscillation on Baltic Sea variability

The connection between the Atlantic Multidecadal Oscillation and the Indian Summer Monsoon since the Industrial Revolution is intrinsic to the climate system (open access)

A direct estimate of volume, heat and fresh water exchange across the Greenland‐Iceland‐Faroe‐Scotland Ridge

Carbon and nitrogen cycles

Seasonal asymmetry in the evolution of surface ocean pCO2 and pH thermodynamic drivers and the influence on sea‐air CO2 flux

Microbial decomposition processes and vulnerable arctic soil organic carbon in the 21st century (open access)

Other papers

Palaeoclimatology

Relative timing of precipitation and ocean circulation changes in the western equatorial Atlantic over the last 45 kyr (open access)



from Skeptical Science https://ift.tt/2NK0BaR

A selection of new climate related research articles is shown below.

Climate change impacts 

Mankind

Bayesian estimates for the mapping of dengue hotspots and estimation of the risk of disease epidemic in Northeast Brazil

Effects of climate change-related heat stress on labor productivity in South Korea

Climatic preferences for beach tourism: an empirical study on Greek islands

Estimation of economic losses from tropical cyclones in China at 1.5 °C and 2.0 °C warming using the regional climate model COSMO‐CLM

Mapping the need for adaptation: assessing drought vulnerability using the livelihood vulnerability index approach in a mid-hill region of Nepal

Unavoidable solutions for coastal adaptation in Reunion Island (Indian Ocean)

Co-producing UK climate change adaptation policy: An analysis of the 2012 and 2017 UK Climate Change Risk Assessments

Behavioral adaptation to climate change in wildfire‐prone forests

Assessing real options in urban surface water flood risk management under climate change (open access)

Climate change impact on Mexico wheat production

Global Freshwater Availability Below Normal Conditions and Population Impact Under 1.5 and 2 °C Stabilization Scenarios

Climate change as a motivating factor for farm-adjustments: rethinking the link (open access)

Ratooning as an adaptive management tool for climatic change in rice systems along a north-south transect in the southern Mississippi valley

Biosphere

Corals sustain growth but not skeletal density across the Florida Keys Reef Tract despite ongoing warming

Depth‐Dependent Thermal Stress Around Corals in the Tropical Pacific Ocean

The influence of weather on avian spring migration phenology: What, where, and when?

Linking permafrost thaw to shifting biogeochemistry and food web resources in an arctic river

Temperature niche position and breadth of ectomycorrhizal fungi: reduced diversity under warming predicted by a nested community structure

Overlooked climate parameters best predict flowering onset: assessing phenological models using the elastic net

Moisture‐mediated responsiveness of treeline shifts to global warming in the Himalayas (open access)

Pushing the limit: Resilience of an Arctic copepod to environmental fluctuations (open access)

Resource limitation alters effects of phenological shifts on inter-specific competition

Climatically controlled reproduction drives interannual growth variability in a temperate tree species

Land‐surface greening suggests vigorous woody regrowth throughout European semi‐natural vegetation

Fire, fragmentation, and windstorms: a recipe for tropical forest degradation

Vegetation‐climate interactions on the Loess Plateau: a non‐linear Granger causality analysis

Cascading effects from plants to soil microorganisms explain how plant species richness and simulated climate change affect soil multifunctionality

Other impacts

Spatiotemporal trends of area burnt in the Iberian Peninsula, 1975–2013

Climate change mitigation 

Climate Policy

Renewable and low carbon technologies policy

Designing China’s national carbon emissions trading system in a transitional period (open access)

Energy production

From collapsed coal mines to floating solar farms, why China's new power stations matter

Emission savings

How big is the energy efficiency resource? (open access)

Multi‐year net ecosystem carbon balance of a restored peatland reveals a return to carbon sink

Chinese cropping systems are a net source of greenhouse gases despite soil carbon sequestration (open access)

Are capitalists green? Firm ownership and provincial CO2emissions in China

Geoengineering

Stopping the flood: could we use targeted geoengineering to mitigate sea level rise? (open access)

Climate change

Temperature, precipitation, wind

The Global Historical Climatology Network Monthly Temperature Dataset, Version 4

Quality control and homogenization of the Belgian historical temperature data

What caused the record‐breaking warming in East China Seas during August 2016? (open access)

Trends of climate change indices in some Mexican cities from 1980 to 2010

Extreme events

Exacerbation of the 2013–2016 Pan‐Caribbean Drought by Anthropogenic Warming

Characteristics and risk analysis of hydrological disaster events from 1949 to 2015 in Urumqi, China

Extreme temperature events on the Iberian Peninsula: Statistical trajectory analysis and synoptic patterns

Climate change risks for severe storms in developing countries in the context of poverty and inequality in Cambodia

Impact of forecasted land use changes on flood risk in the Polish Carpathians (open access)

Comparison of agricultural stakeholder survey results and drought monitoring datasets during the 2016 U.S. Northern Plains flash drought

Regime shift in the destructiveness of tropical cyclones over the western North Pacific

Effect of climatic oscillations on flood occurrence on Papaloapan River, México, during the 1550–2000 period

Tropical cyclone projections: Changing climate threats for Pacific Island defense installations

Likelihood of concurrent climate extremes and variations over China (open access)

A Recent Reversal in the Poleward Shift of Western North Pacific Tropical Cyclones

Changes in the spatial–temporal patterns of droughts in the Brazilian Northeast (open access)

Forcings and feedbacks

Globally significant CO2 emissions from Katla, a subglacial volcano in Iceland

Natural and anthropogenic contributions to long-term variations of SO2, NO2, CO, and AOD over East China

Can Climate Models Reproduce the Decadal Change of Dust Aerosol in East Asia?

Cryosphere

Massive destabilization of an Arctic ice cap

Surface pond energy absorption across four Himalayan glaciers accounts for 1/8 of total catchment ice loss

Atlantic salinity budget in response to Northern and Southern Hemisphere ice sheet discharge (open access)

Seasonal mass variations show timing and magnitude of meltwater storage in the Greenland Ice Sheet (open access)

Atmospheric and oceanic circulation

Transient Response of the Gulf Stream to Multiple Hurricanes in 2017

Gulf Stream variability in the context of quasi‐decadal and multi‐decadal Atlantic climate variability

Impact of the Atlantic Multidecadal Oscillation on Baltic Sea variability

The connection between the Atlantic Multidecadal Oscillation and the Indian Summer Monsoon since the Industrial Revolution is intrinsic to the climate system (open access)

A direct estimate of volume, heat and fresh water exchange across the Greenland‐Iceland‐Faroe‐Scotland Ridge

Carbon and nitrogen cycles

Seasonal asymmetry in the evolution of surface ocean pCO2 and pH thermodynamic drivers and the influence on sea‐air CO2 flux

Microbial decomposition processes and vulnerable arctic soil organic carbon in the 21st century (open access)

Other papers

Palaeoclimatology

Relative timing of precipitation and ocean circulation changes in the western equatorial Atlantic over the last 45 kyr (open access)



from Skeptical Science https://ift.tt/2NK0BaR

‘My fiancee is gone but she’s still helping others fight cancer’

Zarah Harrison

Last week, sitting at my desk at work, I clicked on a newly arrived PDF with considerably more trepidation than usual. The draft expanded to fill my screen, and I nervously scrolled down past a list of authors’ names into a soup of acronyms and jargon. Is she in there? I wondered, my breath quickening.

As part of a global effort to diagnose and treat cancer more effectively, every year researchers analyse millions of patient samples in different ways. Cancer’s inner secrets, and its inherently destructive nature, are being laid out in increasing detail. New avenues open up, new vulnerabilities are exposed. Consequently, step by step, survival stats creep ever upwards.

These efforts lead to thousands of academic publications, each packed with data and punctuated with images, tables and graphs.

For more than a decade my inbox – like those of all my colleagues in the Cancer Research UK communications department – has filled up with these scholarly works. Almost every day we choose discoveries to share with the public to show the impact of our supporters’ generosity and to contextualise the unfolding progress for the wider public.

But this time it was different. Almost three years ago, out of the blue, my fiancee Zarah’s “persistent urinary tract infection” turned out to be bladder cancer – an often aggressive and surprisingly overlooked form of the disease. “It’s stage 4,” her oncologist had told us, gently. “We’ll be trying to contain the disease, not cure it.” I still remember minor details – a windowless, brightly lit ground-floor office in London’s Westmoreland Street hospital, a scrap of paper wedged under a foot of her chair, streaks of mascara running down her cheeks.

Days earlier, Zarah had undergone an operation to remove as much of the tumour as possible. But the surgeon discovered that it had grown into the wall of her bladder, and from there into her lymph nodes. Chemotherapy would buy some time, but just how much was unknowable. The average, I accidentally discovered through late-night Googling, was about nine months. But we felt we’d do much better than that: Zarah was just 37, far younger than an average patient. This gave us hope.

We drew further hope from the fact that, thanks to a call to an academic I’d come to know well, samples of her tumour would be sent off to the UCL Cancer Institute and the Francis Crick Institute, where they’d be scrutinised alongside monthly blood and urine samples for molecular weak spots that might open up experimental options down the line.

There were none. After six months of chemotherapy, and a few months more of what, in retrospect, is best described as an ever-accelerating decline, she died peacefully in my arms in a hospice near our London flat. Nine months. Probably the only average thing about her.

Now, two years later, I’m staring through blurry eyes at a paper authored by the researchers who had analysed Zarah’s samples. Their discovery is not, in media terms, a “breakthrough” – it is, however, a small, important step forward. Thanks to a series of bladder cancer patients who donated urine samples during their illness, the research team has found that the white blood cells floating in patients’ urine contain important information about how the disease might respond to treatment – information that could normally only be obtained with a full-tissue biopsy. It’s the sort of insight that will help others – perhaps profoundly – in the future. And it’s characteristic of Zarah, a Quaker with a burning sense of justice and charity, that she’s still helping others, even now, after her death.

Being able to contribute to research was vitally important to Zarah and has, in turn, helped me and her family come to terms with things, too. This is not surprising. The vast majority of patients say they want to be able to help others by sharing data or samples, and want to know about subsequent findings. Yet according to the 2017 cancer patient experience survey, only a third of patients report having had a conversation about doing so.

When thinking about research, most people imagine drug trials, which can have strict eligibility criteria. Yet, as Zarah’s story shows, there are so many more ways people can take part. There’s a constant need for tissue, urine, blood and other biological material – linked to medical records – to advance our knowledge. And yet far too few patients get the chance to contribute. In a relatively centralised healthcare system such as the NHS, this is a huge missed opportunity.

What’s standing in the way? For a start, researchers may need to think bigger – small, local sample projects are all very well, but larger, nationally coordinated, collaborative studies would be much better. Clinicians working in a cash-strapped, target-driven NHS can struggle to keep abreast of programmes their patients might take part in, and to find time to have sensitive discussions – let alone train to become future researchers. Finally, there needs to be greater public awareness of existing opportunities for patients to take part in research in this way. The UCL team tell me that to take their work further, they need to recruit many more people.

So much, rightly, is made of the need to improve waiting times, and increase staffing levels and funding. But there is a bigger prize: an NHS in which everyone is able to contribute to improving things for those who will inevitably come after them, just like Zarah did.

Henry is part of the communications department at Cancer Research UK

This article originally appeared in The Guardian

Read the research

Wong, et al. (2018). Urine-derived lymphocytes as a non-invasive measure of the bladder tumor immune microenvironment. JEM. DOI: 10.1084/jem.20181003



from Cancer Research UK – Science blog https://ift.tt/2ImkkaL
Zarah Harrison

Last week, sitting at my desk at work, I clicked on a newly arrived PDF with considerably more trepidation than usual. The draft expanded to fill my screen, and I nervously scrolled down past a list of authors’ names into a soup of acronyms and jargon. Is she in there? I wondered, my breath quickening.

As part of a global effort to diagnose and treat cancer more effectively, every year researchers analyse millions of patient samples in different ways. Cancer’s inner secrets, and its inherently destructive nature, are being laid out in increasing detail. New avenues open up, new vulnerabilities are exposed. Consequently, step by step, survival stats creep ever upwards.

These efforts lead to thousands of academic publications, each packed with data and punctuated with images, tables and graphs.

For more than a decade my inbox – like those of all my colleagues in the Cancer Research UK communications department – has filled up with these scholarly works. Almost every day we choose discoveries to share with the public to show the impact of our supporters’ generosity and to contextualise the unfolding progress for the wider public.

But this time it was different. Almost three years ago, out of the blue, my fiancee Zarah’s “persistent urinary tract infection” turned out to be bladder cancer – an often aggressive and surprisingly overlooked form of the disease. “It’s stage 4,” her oncologist had told us, gently. “We’ll be trying to contain the disease, not cure it.” I still remember minor details – a windowless, brightly lit ground-floor office in London’s Westmoreland Street hospital, a scrap of paper wedged under a foot of her chair, streaks of mascara running down her cheeks.

Days earlier, Zarah had undergone an operation to remove as much of the tumour as possible. But the surgeon discovered that it had grown into the wall of her bladder, and from there into her lymph nodes. Chemotherapy would buy some time, but just how much was unknowable. The average, I accidentally discovered through late-night Googling, was about nine months. But we felt we’d do much better than that: Zarah was just 37, far younger than an average patient. This gave us hope.

We drew further hope from the fact that, thanks to a call to an academic I’d come to know well, samples of her tumour would be sent off to the UCL Cancer Institute and the Francis Crick Institute, where they’d be scrutinised alongside monthly blood and urine samples for molecular weak spots that might open up experimental options down the line.

There were none. After six months of chemotherapy, and a few months more of what, in retrospect, is best described as an ever-accelerating decline, she died peacefully in my arms in a hospice near our London flat. Nine months. Probably the only average thing about her.

Now, two years later, I’m staring through blurry eyes at a paper authored by the researchers who had analysed Zarah’s samples. Their discovery is not, in media terms, a “breakthrough” – it is, however, a small, important step forward. Thanks to a series of bladder cancer patients who donated urine samples during their illness, the research team has found that the white blood cells floating in patients’ urine contain important information about how the disease might respond to treatment – information that could normally only be obtained with a full-tissue biopsy. It’s the sort of insight that will help others – perhaps profoundly – in the future. And it’s characteristic of Zarah, a Quaker with a burning sense of justice and charity, that she’s still helping others, even now, after her death.

Being able to contribute to research was vitally important to Zarah and has, in turn, helped me and her family come to terms with things, too. This is not surprising. The vast majority of patients say they want to be able to help others by sharing data or samples, and want to know about subsequent findings. Yet according to the 2017 cancer patient experience survey, only a third of patients report having had a conversation about doing so.

When thinking about research, most people imagine drug trials, which can have strict eligibility criteria. Yet, as Zarah’s story shows, there are so many more ways people can take part. There’s a constant need for tissue, urine, blood and other biological material – linked to medical records – to advance our knowledge. And yet far too few patients get the chance to contribute. In a relatively centralised healthcare system such as the NHS, this is a huge missed opportunity.

What’s standing in the way? For a start, researchers may need to think bigger – small, local sample projects are all very well, but larger, nationally coordinated, collaborative studies would be much better. Clinicians working in a cash-strapped, target-driven NHS can struggle to keep abreast of programmes their patients might take part in, and to find time to have sensitive discussions – let alone train to become future researchers. Finally, there needs to be greater public awareness of existing opportunities for patients to take part in research in this way. The UCL team tell me that to take their work further, they need to recruit many more people.

So much, rightly, is made of the need to improve waiting times, and increase staffing levels and funding. But there is a bigger prize: an NHS in which everyone is able to contribute to improving things for those who will inevitably come after them, just like Zarah did.

Henry is part of the communications department at Cancer Research UK

This article originally appeared in The Guardian

Read the research

Wong, et al. (2018). Urine-derived lymphocytes as a non-invasive measure of the bladder tumor immune microenvironment. JEM. DOI: 10.1084/jem.20181003



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

Mercury’s strange chemistry revealed

Mercury in false color, to visually enhance the chemical, mineralogical and physical differences between the rocks that make up Mercury’s surface. Image via NASA/JHU-APL/Carnegie Institution of Washington.

Mercury, the smallest terrestrial (rocky) planet and closest to the sun, is relatively close to Earth, yet there is much that we still don’t know about it. Next month, the joint ESA-JAXA BepiColombo mission will be launched to this enigmatic world – but in the meantime, there are two new peer-reviewed studies that will help to shed more light on Mercury’s mysteries. The new findings were announced by Europlanet on September 18, 2018 and presented at the European Planetary Science Congress 2018 in Berlin by Bastien Brugger and Thomas Ronnet, both of whom are scientists at the University of Aix Marseille in France.

Scientists have known for some time that Mercury is rather strange – it is significantly smaller than the other terrestrial planets, it is very dense, it has an oversized molten core and it was formed under chemical conditions that determined it would contain much less oxidized material than the other rocky planets. Mercury even has ice deposits near the north pole – most of the surface is hot enough to melt lead, but because there is virtually no atmosphere to speak of, permanently shadowed areas can be as cold as -274° F (-170° C). Brrr! This is due to the fact that Mercury’s axis of rotation is perpendicular to the plane in which it orbits the sun. In other words, Mercury has almost no axial tilt, compared to Earth’s axial tilt of 23.4 degrees.

The interior structure of Mercury, based on current data. Image via Brugger/ University of Aix Marseille/NASA/JPL/JHU-APL.

The first study helps to explain why Mercury is so weird. The research, by a team at the University of Aix Marseille, shows that the planet may have formed very early in the solar system’s history, from condensed vapor from planetesimals. There may also be more iron within Mercury’s mantle than measurements of the surface had previously suggested. Earlier studies, thanks to the MESSENGER mission, had suggested that Mercury is very rich in iron, but also contains more sulphur than should have been available in the material from which the bulk of the solar system formed – another puzzle. As explained by Ronnet:

We think that very early in the Solar System, planetesimals in the innermost region of the solar system could have formed from reprocessed material that was vaporized due to the extreme temperature there and subsequently recondensed. In addition, we are able to rule out a scenario where Mercury formed from a pile-up of planetesimals coming from further out in the solar system since, in this case, Mercury would contain more oxidized material than we actually find.

One of the most surprising discoveries on Mercury has been deposits of water ice at the north pole. On most of the surface, the temperature is hot enough to melt lead, but because there is virtually no atmosphere, permanently shadowed areas can be as cold as -274° F (-170° C). Yellow regions in the composite image are ice deposits. Image via NASA.

Computer simulations of Mercury’s interior, conducted by Brugger, and compared to gravity data gathered by the MESSENGER, showed that Mercury has a dense mantle with substantial amounts of iron. As he noted:

MESSENGER revealed very low abundances of silicate iron on the surface of Mercury, and this element would instead be present in metallic or sulphide phases. Our study suggests that iron abundances in the mantle could be higher than values measured on the surface. With the launch of BepiColombo, we will have a whole new suite of instruments to continue the investigation of Mercury’s unique properties, and try to better understand the structure and origin of the planet.

The second study mentioned at the conference does not have a formal published paper, but is listed along with the first one on the Oral programme TP1 page of the conference. It focuses on the outreach, mission and instruments of BepiColombo, the next mission to Mercury launching next month.

Artist’s concept of BepiColombo approaching Mercury. Image via ESA/ATG medialab, NASA/JPL.

BepiColombo will be Europe’s first-ever mission to Mercury, and is a joint mission between the European Space Agency (ESA) and ESA and the Japan Aerospace Exploration Agency (JAXA). Two orbiters will study Mercury in great detail, building on the data sent back by the previous MESSENGER mission. It will take seven years to travel to Mercury after its scheduled October 19 launch, using a combination of ion propulsion and gravity assist flybys at Earth, Venus and Mercury itself, arriving at Mercury in late 2025.

Bottom line: There is still a lot we don’t know about Mercury, but new research is starting to shed light on the planet’s mysteries, and along with the upcoming BepiColombo mission, we will finally learn more about the origin and evolution of this intriguing little world.

Source: Characterizing the deviations of Mercury’s bulk composition from solar abundances

Via Europlanet



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Mercury in false color, to visually enhance the chemical, mineralogical and physical differences between the rocks that make up Mercury’s surface. Image via NASA/JHU-APL/Carnegie Institution of Washington.

Mercury, the smallest terrestrial (rocky) planet and closest to the sun, is relatively close to Earth, yet there is much that we still don’t know about it. Next month, the joint ESA-JAXA BepiColombo mission will be launched to this enigmatic world – but in the meantime, there are two new peer-reviewed studies that will help to shed more light on Mercury’s mysteries. The new findings were announced by Europlanet on September 18, 2018 and presented at the European Planetary Science Congress 2018 in Berlin by Bastien Brugger and Thomas Ronnet, both of whom are scientists at the University of Aix Marseille in France.

Scientists have known for some time that Mercury is rather strange – it is significantly smaller than the other terrestrial planets, it is very dense, it has an oversized molten core and it was formed under chemical conditions that determined it would contain much less oxidized material than the other rocky planets. Mercury even has ice deposits near the north pole – most of the surface is hot enough to melt lead, but because there is virtually no atmosphere to speak of, permanently shadowed areas can be as cold as -274° F (-170° C). Brrr! This is due to the fact that Mercury’s axis of rotation is perpendicular to the plane in which it orbits the sun. In other words, Mercury has almost no axial tilt, compared to Earth’s axial tilt of 23.4 degrees.

The interior structure of Mercury, based on current data. Image via Brugger/ University of Aix Marseille/NASA/JPL/JHU-APL.

The first study helps to explain why Mercury is so weird. The research, by a team at the University of Aix Marseille, shows that the planet may have formed very early in the solar system’s history, from condensed vapor from planetesimals. There may also be more iron within Mercury’s mantle than measurements of the surface had previously suggested. Earlier studies, thanks to the MESSENGER mission, had suggested that Mercury is very rich in iron, but also contains more sulphur than should have been available in the material from which the bulk of the solar system formed – another puzzle. As explained by Ronnet:

We think that very early in the Solar System, planetesimals in the innermost region of the solar system could have formed from reprocessed material that was vaporized due to the extreme temperature there and subsequently recondensed. In addition, we are able to rule out a scenario where Mercury formed from a pile-up of planetesimals coming from further out in the solar system since, in this case, Mercury would contain more oxidized material than we actually find.

One of the most surprising discoveries on Mercury has been deposits of water ice at the north pole. On most of the surface, the temperature is hot enough to melt lead, but because there is virtually no atmosphere, permanently shadowed areas can be as cold as -274° F (-170° C). Yellow regions in the composite image are ice deposits. Image via NASA.

Computer simulations of Mercury’s interior, conducted by Brugger, and compared to gravity data gathered by the MESSENGER, showed that Mercury has a dense mantle with substantial amounts of iron. As he noted:

MESSENGER revealed very low abundances of silicate iron on the surface of Mercury, and this element would instead be present in metallic or sulphide phases. Our study suggests that iron abundances in the mantle could be higher than values measured on the surface. With the launch of BepiColombo, we will have a whole new suite of instruments to continue the investigation of Mercury’s unique properties, and try to better understand the structure and origin of the planet.

The second study mentioned at the conference does not have a formal published paper, but is listed along with the first one on the Oral programme TP1 page of the conference. It focuses on the outreach, mission and instruments of BepiColombo, the next mission to Mercury launching next month.

Artist’s concept of BepiColombo approaching Mercury. Image via ESA/ATG medialab, NASA/JPL.

BepiColombo will be Europe’s first-ever mission to Mercury, and is a joint mission between the European Space Agency (ESA) and ESA and the Japan Aerospace Exploration Agency (JAXA). Two orbiters will study Mercury in great detail, building on the data sent back by the previous MESSENGER mission. It will take seven years to travel to Mercury after its scheduled October 19 launch, using a combination of ion propulsion and gravity assist flybys at Earth, Venus and Mercury itself, arriving at Mercury in late 2025.

Bottom line: There is still a lot we don’t know about Mercury, but new research is starting to shed light on the planet’s mysteries, and along with the upcoming BepiColombo mission, we will finally learn more about the origin and evolution of this intriguing little world.

Source: Characterizing the deviations of Mercury’s bulk composition from solar abundances

Via Europlanet



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Pink lagoon provides clues to possible Mars life

This lagoon in central Spain – called Laguna de Peña Hueca – has pink-colored water, derived from the red cells of an extremophile microorganism. Scientists say it can provide clues to Mars life. Image via Europlanet/F. Gómez/R. Thombre.

Is there – or has there – been life on Mars? We still don’t conclusively know the answer to that question, but scientists keep finding new clues suggesting that maybe life on the planet did, or even still does, exist. For example, the Curiosity Mars rover has found evidence for an ancient lake and preserved organic material in Gale crater, although direct evidence of life itself is still elusive. Now, a new study describes a remarkable microorganism in a candy-pink lagoon in central Spain, about 60 miles (100 km) south of Madrid. The study suggests that similar kinds of life could survive in highly salty conditions on Mars.

Scientists presented the findings last week (September 16-21) at the European Planetary Science Congress 2018. They also reported them via Europlanet, which is the Congress’s parent organization.

The pink lagoon is called Laguna de Peña Hueca (Wikipedia entry here. It’s part of the Lake Tirez system in La Mancha, Spain. Its water has very high concentrations of salt and sulphur.

Because of its salt and sulphur deposits, this lagoon in Spain is considered a good analog for chloride deposits found in the southern highlands of Mars and the briny ocean water beneath Europa’s icy crust.

Closer view of the pinkish water in the lagoon. Image via Europlanet/F. Gómez/R. Thombre.

The researchers wanted to know what gives the lagoon its distinctive pink color. Biochemist Felipe Gómez of the Centro de Astrobiologia in Spain and Rebecca Thombre of Modern College in Pune, India collected samples of lagoon water for the study. After isolating the microbes, they studied their physical characteristics and genetic sequences. They found that the red cells of a sub-genus of the salt-loving algae Dunaliella were responsible for the pinkish color of the water. Dunaliella is an algal strain found in the lagoon and has been named Dunaliella salina EP-1 after the Europlanet 2020 Research Infrastructure. As explained by Dr. Thombre:

Dunaliella salina EP-1 is one of the most salt-tolerant extremophiles that we’ve found. Microbes find it difficult to tolerate hypersaline environments because water needed for the cell to function tends to flow out through the cell-membrane into the salty surroundings. The algae survive the conditions at Peña Hueca by producing molecules like glycerol that mimic the external salt concentrations within the cell and counteract water-loss.

The results add to previous studies showing how such extremophiles could survive on Mars even today, when conditions are much harsher than they used to be billions of years ago. The martian surface is considered extremely hostile even to extremophiles, but many researchers think that such organisms could easily still exist below the surface, especially given the recent discovery of a salty subsurface lake deep below ice near the south pole, the first time that liquid water has been confirmed to currently exist on Mars. As Dr. Gómez noted:

The resilience of extremophiles to the conditions of Mars analogs on Earth demonstrate their potential to thrive in martian soils. This has implications for planetary protection, as well as how algae might be used to terraform Mars.

Samples of the extremophile algae Dunaliella salina EP-1 in a salt crystal. Image via Europlanet/F. Gómez/R. Thombre.

A closer view of a sample of the extremophilic algal strain from Laguna de Peña Hueca, which has been named Dunaliella salina EP-1. Image via Europlanet/F. Gomez/R. Thombre.

From the new paper:

The tolerance of this extremophile to high concentration of epsomite, salinity, sulphate and perchlorate demonstrates its ability of growth in Martian soils. The current study highlights the resilience of extremophiles from planetary field analogues to Martian conditions and its implications and concerns in Planetary protection as these extremophiles may contaminate spacecraft and can thrive in Martian conditions.

The discovery of this microbe also has applications beyond the search for life on other planets or moons. The cells of Dunaliella algae are used in many countries for the industrial production of carotenoids – ß-carotene, glycerol, bioactives, biofuel and antioxidants – so the strain EP-1 could be used for a wide range of biotechnologies. According to Dr. Thombre:

Considering the commercial and economic significance of this organism, future studies are warranted to gain a complete picture of its physiology, ecology and biotechnological potential.

A salty subsurface lake has been found deep under the ice near the martian south pole. Such an environment could be ideal for microorganisms similar to the ones discovered in the lagoon in Spain. Image via ESA/DLR/FU BERLIN (CC BY-SA 3.0 IGO).

Besides Dunaliella salina EP-1, the researchers also found another halophilic bacteria, Halomonas gomseomensis PLR-1, in a pink rock embedded in the sulphate-rich brine of the lagoon. The scientists say that it will help them understand the role of sulphates in microbial growth and lithopanspermia – the theory that organisms can be transferred in rocks from one planet to another.

The candy-pink lagoon – Laguna de Peña Hueca – is in central Spain, about 60 miles (100 km) south of Madrid.

Bottom line: Extremophiles such as Dunaliella salina EP-1 are providing valuable clues as to what kind of microorganisms could have existed on Mars or could still thrive there today. Underground pockets or lakes of water, even if highly salty, may be the best places to look, if their analogs on Earth are any indication.

Source: Extremophiles from Tirez and Peña Hueca: Implications for exploring habitability of Mars and Europa

Via Europlanet



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This lagoon in central Spain – called Laguna de Peña Hueca – has pink-colored water, derived from the red cells of an extremophile microorganism. Scientists say it can provide clues to Mars life. Image via Europlanet/F. Gómez/R. Thombre.

Is there – or has there – been life on Mars? We still don’t conclusively know the answer to that question, but scientists keep finding new clues suggesting that maybe life on the planet did, or even still does, exist. For example, the Curiosity Mars rover has found evidence for an ancient lake and preserved organic material in Gale crater, although direct evidence of life itself is still elusive. Now, a new study describes a remarkable microorganism in a candy-pink lagoon in central Spain, about 60 miles (100 km) south of Madrid. The study suggests that similar kinds of life could survive in highly salty conditions on Mars.

Scientists presented the findings last week (September 16-21) at the European Planetary Science Congress 2018. They also reported them via Europlanet, which is the Congress’s parent organization.

The pink lagoon is called Laguna de Peña Hueca (Wikipedia entry here. It’s part of the Lake Tirez system in La Mancha, Spain. Its water has very high concentrations of salt and sulphur.

Because of its salt and sulphur deposits, this lagoon in Spain is considered a good analog for chloride deposits found in the southern highlands of Mars and the briny ocean water beneath Europa’s icy crust.

Closer view of the pinkish water in the lagoon. Image via Europlanet/F. Gómez/R. Thombre.

The researchers wanted to know what gives the lagoon its distinctive pink color. Biochemist Felipe Gómez of the Centro de Astrobiologia in Spain and Rebecca Thombre of Modern College in Pune, India collected samples of lagoon water for the study. After isolating the microbes, they studied their physical characteristics and genetic sequences. They found that the red cells of a sub-genus of the salt-loving algae Dunaliella were responsible for the pinkish color of the water. Dunaliella is an algal strain found in the lagoon and has been named Dunaliella salina EP-1 after the Europlanet 2020 Research Infrastructure. As explained by Dr. Thombre:

Dunaliella salina EP-1 is one of the most salt-tolerant extremophiles that we’ve found. Microbes find it difficult to tolerate hypersaline environments because water needed for the cell to function tends to flow out through the cell-membrane into the salty surroundings. The algae survive the conditions at Peña Hueca by producing molecules like glycerol that mimic the external salt concentrations within the cell and counteract water-loss.

The results add to previous studies showing how such extremophiles could survive on Mars even today, when conditions are much harsher than they used to be billions of years ago. The martian surface is considered extremely hostile even to extremophiles, but many researchers think that such organisms could easily still exist below the surface, especially given the recent discovery of a salty subsurface lake deep below ice near the south pole, the first time that liquid water has been confirmed to currently exist on Mars. As Dr. Gómez noted:

The resilience of extremophiles to the conditions of Mars analogs on Earth demonstrate their potential to thrive in martian soils. This has implications for planetary protection, as well as how algae might be used to terraform Mars.

Samples of the extremophile algae Dunaliella salina EP-1 in a salt crystal. Image via Europlanet/F. Gómez/R. Thombre.

A closer view of a sample of the extremophilic algal strain from Laguna de Peña Hueca, which has been named Dunaliella salina EP-1. Image via Europlanet/F. Gomez/R. Thombre.

From the new paper:

The tolerance of this extremophile to high concentration of epsomite, salinity, sulphate and perchlorate demonstrates its ability of growth in Martian soils. The current study highlights the resilience of extremophiles from planetary field analogues to Martian conditions and its implications and concerns in Planetary protection as these extremophiles may contaminate spacecraft and can thrive in Martian conditions.

The discovery of this microbe also has applications beyond the search for life on other planets or moons. The cells of Dunaliella algae are used in many countries for the industrial production of carotenoids – ß-carotene, glycerol, bioactives, biofuel and antioxidants – so the strain EP-1 could be used for a wide range of biotechnologies. According to Dr. Thombre:

Considering the commercial and economic significance of this organism, future studies are warranted to gain a complete picture of its physiology, ecology and biotechnological potential.

A salty subsurface lake has been found deep under the ice near the martian south pole. Such an environment could be ideal for microorganisms similar to the ones discovered in the lagoon in Spain. Image via ESA/DLR/FU BERLIN (CC BY-SA 3.0 IGO).

Besides Dunaliella salina EP-1, the researchers also found another halophilic bacteria, Halomonas gomseomensis PLR-1, in a pink rock embedded in the sulphate-rich brine of the lagoon. The scientists say that it will help them understand the role of sulphates in microbial growth and lithopanspermia – the theory that organisms can be transferred in rocks from one planet to another.

The candy-pink lagoon – Laguna de Peña Hueca – is in central Spain, about 60 miles (100 km) south of Madrid.

Bottom line: Extremophiles such as Dunaliella salina EP-1 are providing valuable clues as to what kind of microorganisms could have existed on Mars or could still thrive there today. Underground pockets or lakes of water, even if highly salty, may be the best places to look, if their analogs on Earth are any indication.

Source: Extremophiles from Tirez and Peña Hueca: Implications for exploring habitability of Mars and Europa

Via Europlanet



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What is a waning gibbous moon?

Ilija Desic in Belgrade, Serbia caught the waning gibbous moon with seagulls on the morning of September 28, 2018.

In the days after full moon, do you sometimes look for the moon and not find it? At that time, the moon is in a waning gibbous phase: less than full but more than half-lighted. A full moon rises at sunset, but a waning gibbous moon rises later at night and appears in the morning sky.

A waning gibbous moon can surprise you if you happen to be out late in the evening. It rises eerily some hours after sunset, glowing red like a full moon when it’s near the horizon.

Sometimes it looks like a misshapen clone of a full moon.

Wonderful photo of a waning gibbous moonrise over Toronto, via our friend Lunar 101-Moon Book.

A waning gibbous moon also initiates a rash of questions about seeing the moon during the day.

If it rises late at night, you know the waning gibbous moon must set after sunrise.

In fact, in the few days after full moon, you’ll often see the waning gibbous moon in the west in early morning, floating against the pale blue sky.

Jenney Disimon caught this daytime moon – a waning gibbous moon, 94.7% illuminated – from Sabah, North Borneo.

As the moon orbits Earth, it changes phase in an orderly way. Follow the link below to understand the phases of the moon.

New moon
Waxing crescent moon
First quarter moon
Waxing gibbous moon
Full moon
Waning gibbous moon
Last quarter moon
Waning crescent moon

Read more: 4 keys to understanding moon phases

Bottom line: A waning gibbous moon is up from late night until early morning. It’s between full moon and last quarter moon. The last full moon was September 24-25. The next last quarter moon will be October 2.

Check out EarthSky’s guide to the bright planets.

Help EarthSky keep going! Please donate.



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Ilija Desic in Belgrade, Serbia caught the waning gibbous moon with seagulls on the morning of September 28, 2018.

In the days after full moon, do you sometimes look for the moon and not find it? At that time, the moon is in a waning gibbous phase: less than full but more than half-lighted. A full moon rises at sunset, but a waning gibbous moon rises later at night and appears in the morning sky.

A waning gibbous moon can surprise you if you happen to be out late in the evening. It rises eerily some hours after sunset, glowing red like a full moon when it’s near the horizon.

Sometimes it looks like a misshapen clone of a full moon.

Wonderful photo of a waning gibbous moonrise over Toronto, via our friend Lunar 101-Moon Book.

A waning gibbous moon also initiates a rash of questions about seeing the moon during the day.

If it rises late at night, you know the waning gibbous moon must set after sunrise.

In fact, in the few days after full moon, you’ll often see the waning gibbous moon in the west in early morning, floating against the pale blue sky.

Jenney Disimon caught this daytime moon – a waning gibbous moon, 94.7% illuminated – from Sabah, North Borneo.

As the moon orbits Earth, it changes phase in an orderly way. Follow the link below to understand the phases of the moon.

New moon
Waxing crescent moon
First quarter moon
Waxing gibbous moon
Full moon
Waning gibbous moon
Last quarter moon
Waning crescent moon

Read more: 4 keys to understanding moon phases

Bottom line: A waning gibbous moon is up from late night until early morning. It’s between full moon and last quarter moon. The last full moon was September 24-25. The next last quarter moon will be October 2.

Check out EarthSky’s guide to the bright planets.

Help EarthSky keep going! Please donate.



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Moon in Taurus September 28-30

On September 28, 29 and 30, 2018, watch as the waning gibbous moon sweeps eastward through the constellation Taurus the Bull. The bright moon might make it tough to see all of the starlit figure of the Bull on these nights. But you should be able to make out Aldebaran, Taurus’ brightest star, as well as the tiny, misty, dipper-shaped Pleiades star cluster.

Taurus is a far-northern constellation of the zodiac. That fact causes these stars to rise at an earlier hour in the Northern Hemisphere than in the Southern Hemisphere. The farther north you live, the earlier that Taurus climbs above your northwest horizon; and the farther south you live, the later that Taurus come up.

If you’re not one to stay up late, get up before daybreak to view the moon and Taurus in the predawn sky.

Taurus the Bull via Urania’s Mirror/© Ian Ridpath.

From the Northern Hemisphere, the moon and Taurus’ two major signposts – Aldebaran and the Pleaides – may well be up before your bedtime.

From temperate latitudes in the Southern Hemisphere, Taurus won’t be up until very late evening, or fairly close to the midnight hour.

Click here and check the moonrise and moonset box to find out when the moon rises into your sky.

Click here and check Aldebaran as your celestial object of interest to find out when Aldebaran rises into your sky.

The ecliptic - the sun's yearly path through the constellations of the zodiac - passes through the constellation Taurus the Bull, to the north of the star Aldebaran and to the south of the Pleiades star cluster. The sun shines in front of Taurus from about May 14 to June 21.

The ecliptic – the sun’s yearly path through the constellations of the Zodiac – passes through the constellation Taurus the Bull, to the north of the star Aldebaran and to the south of the Pleiades star cluster. The sun shines in front of Taurus from about May 14 to June 21, every year.

When the moon travels in front of Taurus (or any constellation of the zodiac, for that matter), the moon can travel anywhere from 5 degrees north to 5 degrees south of the ecliptic. For the next several years, the moon will remain south of the ecliptic as in its monthly travels in front of Taurus the Bull.

Recently, on September 3, 2018, the moon occulted (passed in front of) Aldebaran, presenting the final occultation of a monthly occultation series that started on January 29, 2015. But month by month, and year by year, the moon’s trajectory will slowly but surely shift northward as it goes through Taurus the Bull. In fact, for the next 15 years, the moon will be sweeping in between Aldebaran and Alcyone, Pleiades’ brightest star.

The monthly occultation series involving the moon and Alcyone will take place from September 5, 2023, till July 7, 2029.

When the moon moves away, try this. The 3 stars of Orion’s Belt always point to the star Aldebaran and the Pleiades star cluster. Image via Janne/Flickr.

Bottom line: On September 28, 29 and 30, 2018, watch the bright waning gibbous moon journey eastward through the constellation Taurus the Bull.



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On September 28, 29 and 30, 2018, watch as the waning gibbous moon sweeps eastward through the constellation Taurus the Bull. The bright moon might make it tough to see all of the starlit figure of the Bull on these nights. But you should be able to make out Aldebaran, Taurus’ brightest star, as well as the tiny, misty, dipper-shaped Pleiades star cluster.

Taurus is a far-northern constellation of the zodiac. That fact causes these stars to rise at an earlier hour in the Northern Hemisphere than in the Southern Hemisphere. The farther north you live, the earlier that Taurus climbs above your northwest horizon; and the farther south you live, the later that Taurus come up.

If you’re not one to stay up late, get up before daybreak to view the moon and Taurus in the predawn sky.

Taurus the Bull via Urania’s Mirror/© Ian Ridpath.

From the Northern Hemisphere, the moon and Taurus’ two major signposts – Aldebaran and the Pleaides – may well be up before your bedtime.

From temperate latitudes in the Southern Hemisphere, Taurus won’t be up until very late evening, or fairly close to the midnight hour.

Click here and check the moonrise and moonset box to find out when the moon rises into your sky.

Click here and check Aldebaran as your celestial object of interest to find out when Aldebaran rises into your sky.

The ecliptic - the sun's yearly path through the constellations of the zodiac - passes through the constellation Taurus the Bull, to the north of the star Aldebaran and to the south of the Pleiades star cluster. The sun shines in front of Taurus from about May 14 to June 21.

The ecliptic – the sun’s yearly path through the constellations of the Zodiac – passes through the constellation Taurus the Bull, to the north of the star Aldebaran and to the south of the Pleiades star cluster. The sun shines in front of Taurus from about May 14 to June 21, every year.

When the moon travels in front of Taurus (or any constellation of the zodiac, for that matter), the moon can travel anywhere from 5 degrees north to 5 degrees south of the ecliptic. For the next several years, the moon will remain south of the ecliptic as in its monthly travels in front of Taurus the Bull.

Recently, on September 3, 2018, the moon occulted (passed in front of) Aldebaran, presenting the final occultation of a monthly occultation series that started on January 29, 2015. But month by month, and year by year, the moon’s trajectory will slowly but surely shift northward as it goes through Taurus the Bull. In fact, for the next 15 years, the moon will be sweeping in between Aldebaran and Alcyone, Pleiades’ brightest star.

The monthly occultation series involving the moon and Alcyone will take place from September 5, 2023, till July 7, 2029.

When the moon moves away, try this. The 3 stars of Orion’s Belt always point to the star Aldebaran and the Pleiades star cluster. Image via Janne/Flickr.

Bottom line: On September 28, 29 and 30, 2018, watch the bright waning gibbous moon journey eastward through the constellation Taurus the Bull.



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