Celestial visitor - comet C/2023 A3 and how to see it

 

The ‘best comet of the year’ is finally here – here’s everything you need to know

AstroStar/Shutterstock

Jonti Horner, University of Southern Queensland

In January 2023, a new comet was discovered. Comets are found regularly, but astronomers quickly realised this one, called C/2023 A3 (Tsuchinshan-ATLAS), had the potential to be quite bright.

Some hyperbolic reports have suggested it might be the “comet of the century”, but any astronomer will tell you the brightness of comets is notoriously hard to predict. As I explained last year, we’d have to wait until it arrived to be sure how bright it would become.

Now, the time has come. Comet C/2023 A3 is currently visible with the naked eye in the morning sky in Australia and Aotearoa New Zealand, with its best yet to come in the next few weeks. And it does look promising. It’s unlikely to be the comet of the decade (never mind the comet of the century), but it will almost certainly become the best comet of the year.

So where, and when, should you look to get your best views of this celestial visitor?

A show in the morning, before sunrise

At the moment, comet C/2023 A3 (Tsuchinshan-ATLAS) is a morning object, rising around an hour and a half before sunrise. It is visible to the naked eye, but not yet spectacular. However, with binoculars you can easily see the comet’s dusty tail pointing away from the Sun.

The comet will remain at about the same altitude in the morning sky until around September 30. It will then get closer to the horizon on each consecutive morning until it’s lost in the glare of the approaching dawn by October 6 or 7.

If you want to spot the comet in the morning sky, look east. The sliders below will help you orient yourself and choose the best time to look, depending on your latitude.

During this period, the comet should slowly brighten. It reaches its closest approach to the Sun (perihelion) on September 27, when it will be 58 million kilometres from our star.

As it swings around the Sun, it will continue to approach Earth, and so should continue to brighten. The best show in the morning sky will likely be during the last couple of days of September and the first few days in October, before the comet is lost to view.

A potential daylight comet

Thanks to pure good fortune, comet C/2023 A3 (Tsuchinshan-ATLAS) will then pass almost directly between Earth and the Sun on October 9 and 10.

This could cause a spectacular brightening of the comet, thanks to “forward scattering” caused by its dust. Imagine looking towards a bright light source through a cloud of dust grains. The grains nearest to the light source will scatter light from the source back towards you.

As the comet swings between Earth and the Sun, it will be perfectly placed for this forward scattering process to occur. If the comet is particularly dusty, this could cause its apparent brightness to increase by up to 100 times.

If it does, there’s a small chance the comet could briefly become visible in the daylight sky on October 9 and 10.

However, it will be very close to the Sun in the sky, and incredibly hard to spot. Only the most experienced observers may be able to detect the comet at this time, and it requires a special technique. Do not try to stare at the Sun to see it.

The best show could be after October 12

After swinging between Earth and the Sun, the comet will appear in the evening sky. It will rapidly climb in the western sky, and should be a bright, naked-eye object for a few days from October 12. The sliders below will give you a sense of where to look.

For the first few days of this period, the comet will still benefit from the forward scattering of sunlight, but this will decrease as it moves away.

What about the tail?

The positioning of the comet, Earth and the Sun in the Solar System means the comet’s tail will be streaming outwards, past our planet. This means it could grow to prodigious lengths in the night sky.

The bulk of that tail will likely be too dim to see easily with the naked eye, but it could be a fantastic spectacle for photographers. Expect to see a wealth of comet images flooding the internet around the middle of October.

As the days pass and the comet climbs higher, it will fade quite rapidly. It will likely become too faint to see with the naked eye, even for seasoned and experienced observers, before the end of October.

At that point, the show will be over. Comet C/2023 A3 (Tsuchinshan-ATLAS) will continue to flee the inner Solar System, moving into the icy depths of space, never to return.

How reliable are the predictions?

At the moment, the comet is already bright enough to consider it the “comet of the year”, outshining comet 12P/Pons-Brooks from earlier this year.

But remember the classic saying – comets are like cats. They have tails and will often surprise us. For now, comet C/2023 A3 is behaving itself. It’s brightening predictably, and putting on a good show.

But comets that approach this closely to the Sun often fragment. This is impossible to predict, and far from guaranteed. If the comet did break up, it could become even more spectacular because of all the dust and gas it would release.

The opposite could still happen, too. The comet could fail to brighten as much as we expect, although that seems unlikely at this stage.

Whatever happens, we’re in for a fascinating few weeks of comet watching. Hopefully, a real spectacle awaits us.

Jonti Horner, Professor (Astrophysics), University of Southern Queensland

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Australia and arms exports

 What we know about Australia’s arms exports: we’ve analysed the data

Lauren Sanders, The University of Queensland

Thousands of protesters have been out in force in Melbourne this week to disrupt the Land Forces International Land Defence Exposition, where defence companies from around the world are showcasing their latest designs in weapons and technology.

The activists are protesting the use of such weapons – in particular, allegations of use against Palestinian civilians by Israeli forces in Gaza.

With the expo in Melbourne this week, there is also renewed attention on Australia’s weapons exports and imports. So, how much do we know about where Australia is sending its arms, and how many arms it is importing?

What gets reported?

The government limits what information is made publicly available about arms exports and imports due to both security and commercial reasons.

Australian exports include both military-specific and dual-use goods and technologies, such as computer components used in weapons. There is a strict export control system that is intended to prevent weapons from getting into the hands of our adversaries and to ensure they meet our obligations under international law.

But this system has been criticised for being opaque. This is because Australia only publicly reports recipient countries for items it is obliged to disclose under the Arms Trade Treaty, or in some cases, during parliamentary hearings or other similar processes.

Separately, Australia’s Defence Export Office publishes quarterly reports with very basic information, such as the number and types of export applications it receives and the total value of permits it issues. It only specifies the export permits for “end users” by continent, not country.

In the year 2023–24, the office finalised more than 4,000 export defence permits, with the value of permits issued exceeding an estimated A$100 billion.

Unlike other countries, Australia does not specify exactly what types of goods it has approved for import or export.

The government also does not report how many issued permits are actually used by companies to trade goods. The movement of military goods to and from Australia is tracked through other processes, such as customs controls.

Finally, requests for further information are typically met with resistance from the government, on the basis such disclosures would breach security or commercial confidentiality arrangements.

However, while not authoritative, information about Australian exports can be pieced together from a variety of sources. This includes reports from exporting companies themselves, reports sent by exporters to the Department of Foreign Affairs and Trade, and statements made in parliament and in other government reporting.

The Stockholm International Peace Research Institute (SIPRI) also tracks arms shipments between countries by assessing public information. Some countries provide information directly to their analysts.

Here is some data we have compiled from SIPRI showing Australia’s exports and imports for the most recent five-year period from 2019–23, based on what is publicly known.

Australia’s arms exports

According to SIPRI, Australia ranked 13th in overall military expenditures globally in 2022–23, spending US$32.3 billion (A$49 billion), or about 1.9% of GDP.

Australia was also one of the top 20 arms exporters in the world from 2019–23, though its share of total global arms exports was just 0.6%, similar to Canada. This share was up from 0.3% in 2014–18.

The United States, meanwhile, accounted for 42% of global arms exports in 2019–23.

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The map below shows the top recipients for Australian arms during this five-year period. The top three recipients were Canada (32% of Australia’s total exports), Chile (28%) and the United States (11%).

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What do we know about Israel?

According to SIPRI, Israel’s arms imports for 2019–23 came primarily from the US (69%) and Germany (30%).

The Albanese government maintains Australia hasn’t supplied weapons or ammunition to Israel in the past five years. This week, it also explicitly backed the United Kingdom’s decision to curb arms exports to Israel.

Some of what we know about Australia’s exports to Israel has been the result of questions being put to parliamentarians.

In June, the government said it had granted eight permits to export defence-related equipment to Israel since the Gaza war began last October. It clarified that most of the items were being sent to Israel for repair and then returned to Australian defence and law enforcement for their use.

This reporting, however, does not capture sub-components that are manufactured in Australia and sent to a central repository overseas to be used in a larger platform, like an F-35 jet, which can then be sent to Israel from the US or Europe.

Parts made in Australia are used in the US to build the F-35, which is then sold globally. CC BY-SA

What do we know about Ukraine?

In the case of Ukraine, Australia has exported conventional arms such as Bushmaster armoured vehicles and artillery. Some of these have been included in its public reporting, given the type of equipment being provided.

According to SIPRI, the largest sources of military goods to Ukraine have been the US, Germany and Poland.

Australia’s arms imports

SIPRI’s data shows that Australia was eighth-largest importer of arms from 2019–23, accounting for 3.7% of global arms imports.

The vast majority (80%) of its imports during this period came from the United States, followed by Spain at 15%.

The types of items that Australia has reported importing from the US include ships, aircraft, helicopters and missile defence systems. In addition, SIPRI noted that Australia ordered 300 long-range missiles from the US in 2023.

However, because it often takes years for these large defence items to be built, quite often there is a lag in the reporting of import data.

For example, Australia’s recently announced deal with Hanwha, a Korean defence company, to build artillery and armoured vehicles will not be featured in these statistics as some components of the vehicles and artillery will be built in a factory in Geelong, Australia, while others will not be delivered in this reporting period.

Also, while export control measures deal with goods that are built elsewhere and brought to Australia, some permits are required to import the know-how to build controlled defence goods in Australia. This is another reason imports like these might not appear on public reports.

Lauren Sanders, Senior Research Fellow on Law and the Future of War, The University of Queensland

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Asteroids and the threat to Earth

 

NASA just shut down a planetary defence mission that tracks asteroids. Now what?

Artist’s impression of NEOWISE spacecraft. NASA/Caltech-JPL

Steven Tingay, Curtin University

Launched in 2011, NASA’s NEOWISE mission operated in Earth’s orbit until late last week. It detected more than 3,000 near-Earth objects or NEOs – asteroids or comets whose orbits can bring them close to Earth, even with the possibility of a collision. NEOWISE was shut down on August 8.

Surveying the population of NEOs is central to the emerging concept of planetary defence. That is, understanding and mitigating the risk of collision from asteroids large enough to do significant damage to Earth.

NEOWISE has made fundamental contributions to establishing the knowledge base for planetary defence, with more than 200 of the 3,000 objects it studied not known to us previously.

Now at mission end, and commanded by NASA to shut itself down, NEOWISE will re-enter Earth’s atmosphere before the end of this year. Where does that leave us with defending our planet?

All Known Asteroids in the Solar System (1999–2018)

From astrophysics to planetary defence

NEOWISE started life as a different mission, simply called WISE (Wide-field Infrared Survey Explorer). It was designed to study the infrared radiation from distant galaxies in the universe.

Infrared means “beyond red” – infrared light sits just past the red end of the spectrum of colours humans can see. We know infrared radiation better as the heat from the Sun, for example, or from a radiator keeping us warm in winter.

Infrared light is just outside the part of the spectrum that the human eye can see. brgfx/Shutterstock

When the coolant on the WISE mission ran out and these sensitive observations of galaxies couldn’t be carried out any more, NASA granted a mission extension under the NEOWISE name. They realised the telescope system was still sensitive enough to detect asteroids and comets that come close to Earth and the Sun, thereby having a very strong infrared signal.

NASA has an extraordinary history of squeezing extra life out of missions that reach completion. In this case, NEOWISE represented an entire second life, in an entirely different area of research.

How will we defend Earth now?

As well as the discovery and study of thousands of NEOs, NEOWISE established the foundation of knowledge that has informed a new, dedicated planetary defence mission. NASA’s NEO Surveyor will be launched in 2027.

NEO Surveyor’s goal is to discover approximately two thirds of all NEOs larger than 140 metres in diameter, over a five year baseline survey. This is a big step toward fulfilling the mandate United States Congress has provided to NASA: to discover 90% of all NEOs in this size range.

If they hit Earth, asteroids of this size could cause mass casualties if the impact were over a large metropolitan region.

You might think this poses a bit of a risk – shutting down NEOWISE three years before launching NEO Surveyor. What happens if one of these big asteroids comes our way in the next few years?

The risks are very small, as estimates show asteroids 140 metres in diameter impact Earth only approximately every 20,000 years. So, we would have to be extremely unlucky to have one in any given three-year period, especially impacting a place that would cause a large amount of damage. Only around 3% of Earth’s surface is occupied by urban areas.

NASA doesn’t really have much of a choice with the end of NEOWISE. The Sun’s 11-year activity cycle is picking up and causing Earth’s upper atmosphere, the ionosphere, to thicken. NEOWISE is flying through this ionosphere and can’t raise its orbit, so the ionosphere is inevitably dragging NEOWISE back to Earth.

NEO Surveyor started construction in 2023, so a 2027 launch is pretty impressively rapid, which is minimising the gap between NEOWISE and NEO Surveyor.

NEOWISE is scheduled to enter Earth’s atmosphere before the end of the year, but we don’t know precisely when.

Weighing almost 700kg, some of NEOWISE itself is likely to impact the surface of Earth. Hopefully it stays away from populated areas in the process – some recent re-entry events have resulted in space debris falling reasonably close to populated areas.

An asteroid is coming! What next?

Knowing about an asteroid on a collision course with Earth is one thing. Doing something about it is another thing altogether.

Huge steps toward planetary defence occurred two years ago, when the DART mission flew to an asteroid, impacted it, and changed its trajectory. This demonstrated it’s possible to change the course of asteroids, which could be used in the future to protect Earth from a collision.

Predicting potential Earth impacts as far as possible in advance, years preferably, gives the DART-style technology approach a chance.

The pioneering work of NEOWISE, and the upcoming comprehensive observations of NEO Surveyor, will place an enormous amount of information in our scientific bank, which will never go out of date and will be the basis for planetary defence for perhaps hundreds of years into the future.

Steven Tingay, John Curtin Distinguished Professor (Radio Astronomy), Curtin University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Polling on American perceptions of internal conflict in the United States

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With the US presidential election this year, public opinion polling has been prolific particularly since the annoucnement of US president, Joe Biden that he would not be seeking a second term and nominating Vice President, Kamala Harris to be the Democratic Party candidate.

Other polls on general sentiment have been conducted and underscore the level of unease that is found in the United States at the moment.  The Marist Poll is one such survey that identified that around 50 per cent of people polled had a pessimistic outlook on the current situation of possible internal conflict n the US. The poll was conducted prior to the announcement of President Biden's withdrawal from the election on 21 July 2024.

How was the survey done ?

The survey of 1,192 adults was conducted April 16th through April 18th, 2024 by the Marist Poll. Adults 18 years of age and older residing in the United States were contacted through a multi-mode design: By phone using live interviewers or online. 

Results

More than 160 years after the Civil War began, nearly half of Americans think that it is either very likely or likely that they will see a second civil war. Perceptions about the possibility of another domestic conflict break along partisan, generational, racial and gender lines.

Link to the poll: Marist Poll: a nation divided

The value of Unions and the right to protest

Electrical Trades Union protest 2024 (c) Sentinel Owl

The formation and evolution of modern trade unions in the workplace dates back to the late 19th Century and the rapid changes in society brought by the Industrial Revolution. Prior to this, trade guilds of artisans have been shown to have existed as far back as the first century AD of the Roman Empire.  The advent of modern capitalism through the industrial revolution brought about significant changes in the basis of ''work' whereby the owners of capital engaged workers to provide labour for services and/or production of goods. The workers surrendered part of their rights of freedom and agency to take instructions from their employer (or master) in order to earn a wage. This process and unequal level of power for workers in turn led to the organisation of labour into unions to enable workers to protect themselves from complete exploitation. Over the past two centuries, these organisations have envolved and changed with the ebb and flow of economies, technological innovation and changing industrial relations laws.

Australia has long history of trade unions, derived in part from the influence of Mother England and the previous colonial period. Membership of trade unions has been declining as shown by research data from the Australian Bureau of Statistics. As at December 2022 -

• 12.5% of employees in the total workforce were trade union members
• Since 1992, the proportion of employees who were trade union members has fallen from 41% to 12.5%
• The Education and training industry (30%) and the Professionals occupation group (19%) had the highest rates of trade union membership.

Source link: Trade union membership  

Nonetheless these organisations remain a potent and relevant party in the industrial relations landscape.

This year, the Electrical Trades Union (ETU) representing the electricians and power industry workers has staged their campaign for higher wages via a Log of Claims to energy provider, Ausgrid and placed their protest outside the television studios of the Australian Broadcasting Corporation (ABC) in Ultimo, Sydney. It's a visually impactful and almost humourous presentation with large inflatables, even as the topic is a serious one (as shown in the images in this posting).

   

A Star is born

 Look up! A once-in-a-lifetime explosion is about to create a ‘new’ star in the sky

Stellarium Web Online Star Map

Tanya Hill, Museums Victoria Research Institute and Amanda Karakas, Monash University

Any night now, a “new star” or nova will appear in the night sky. While it won’t set the sky ablaze, it’s a special opportunity to see a rare event that’s usually difficult to predict in advance.

The star in question is T Coronae Borealis (T CrB, pronounced “T Cor Bor”). It lies in the constellation of the northern crown, prominent in the Northern Hemisphere but also visible in the northern sky from Australia and Aotearoa New Zealand over the next few months.

Most of the time T CrB, which is 3,000 light years away, is much too faint to be seen. But once every 80 years or so, it brightly erupts.

A brand new star suddenly seems to appear, although not for long. Just a few nights later it will have rapidly faded, disappearing back into the darkness.

A burst of life

During the prime of their lives, stars are powered by nuclear fusion reactions deep inside their cores. Most commonly, hydrogen is turned into helium creating enough energy to keep the star stable and shining for billions of years.

But T CrB is well past its prime and is now a stellar remnant known as a white dwarf. Its internal nuclear fire has been quenched, allowing gravity to dramatically compress the dead star.

T CrB also has a stellar companion – a red giant that has puffed up as it enters old age. The white dwarf mops up the swollen red giant’s gas, and this forms what’s known as an accretion disc around the dead star.

The matter keeps piling up on a star that’s already compressed to its limit, forcing a continual rise in pressure and temperature. Conditions become so extreme, they mimic what once would’ve been found inside the star’s core. Its surface ignites in a runaway thermonuclear reaction.

When this happens, the energy released makes T CrB shine 1,500 times brighter than usual. Here on Earth, it briefly appears in the night sky. With this dramatic reset, the star has then expelled the gas and the cycle can begin all over again.

Animation of a nova erupting as thermonuclear reactions ignite on the smaller white dwarf star. Credit: NASA/Conceptual Image Lab/Goddard Space Flight Center.

How do we know it’s due?

T CrB is the brightest of a rare class of recurrent novae that repeat within a hundred years – a time scale that allows astronomers to detect their recurrent nature.

Only ten recurrent novae are currently known, although more novae may be recurrent – just on much greater timescales that aren’t as easily tracked.

The earliest known date of T CrB erupting is from the year 1217, based on observations recorded in a medieval monastic chronicle. It’s remarkable that astronomers can now predict its eruptions so precisely as long as the nova follows its usual pattern.

The star’s two most recent eruptions – in 1866 and 1946 – showed the exact same features. About ten years prior to the eruption, T CrB’s brightness increased a little (known as a high state) followed by a short fading or dip about a year out from the explosion.

T CrB entered its high state in 2015 and the pre-eruption dip was spotted in March 2023, setting astronomers on alert. What causes these phenomena are just some of the current mysteries surrounding T CrB.

How can I see it?

Start stargazing now! It’s a good idea to get used to seeing Corona Borealis as it is now, so that you get the full impact of the “new” star.

Corona Borealis currently reaches its best observing position (known as a meridian transit) around 8:30pm to 9pm local time across Australia and Aotearoa. The farther north you are located, the higher the constellation will be in the sky.

The nova is expected to be a reasonable brightness (magnitude 2.5): about as bright as Imai (Delta Crucis), the fourth brightest star in the Southern Cross. So it will be easy to see even from a city location, if you know where to look.

We won’t have much time

We won’t have long once it goes off. The maximum brightness will only last a few hours; within a week T CrB will have faded and you’ll need binoculars to see it.

It almost certainly will be an amateur astronomer that alerts the professional community to the moment when T CrB outbursts.

These dedicated and knowledgeable people routinely monitor stars from their backyards on the chance of “what if” and therefore fill an important gap in night sky observations.

The American Association of Variable Star Observing (AAVSO) has a log of over 270,000 submitted observations on T CrB alone. Amateur astronomers are collaborating here and around the world to continually monitor T CrB for the first signs of eruption.

Hopefully the nova will erupt as expected sometime before October, because after that Corona Borealis leaves our evening sky in the Southern Hemisphere.

Tanya Hill, Senior Curator (Astronomy), Museums Victoria and Honorary Fellow at University of Melbourne, Museums Victoria Research Institute and Amanda Karakas, Associate Professor, School of Physics and Astronomy, Monash University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Coral reefs in jeopardy

Devastating coral bleaching will be more common, start earlier and last longer unless we cut emissions

Sarah_lewis/Shutterstock

Camille Mellin, University of Adelaide and Damien Fordham, University of Adelaide

Coral bleaching is becoming much more common as a result of increasingly severe and frequent marine heatwaves. Four global mass bleaching events have happened since 1998. Two of these were in the past decade.

Unless greenhouse gas emissions are cut to slow global warming, our new research shows that, by 2080, coral bleaching will start in spring, rather than late summer. Some events will last into autumn. The Great Barrier Reef’s maximum annual heat stress will double by 2050 if emissions do not slow.

Marine heatwaves stress corals, which then expel the symbiotic algae living in their tissue. These corals are left white and weakened. While not all bleached corals die immediately, prolonged heat stress harms their health and reproduction.

Our research used daily data on sea surface temperatures (instead of monthly data that models typically use) and supercomputing to produce high-resolution projections of marine heatwaves. We showed the risk of coral bleaching will be greatest along the equator. That’s also where the most biodiverse coral reefs are found.

Coral reefs cover only 1% of our oceans, but host at least 25% of all marine species. More than half a billion people worldwide depend on coral reefs for food.

So coral reefs are vital for the health of the ocean and people. They are also among the ecosystems most at risk from climate change.

Longer bleaching season will hit spawning

The US National Oceanic and Atmospheric Administration monitors marine heatwaves globally. Seasonal coral bleaching alerts are based on this data. Predicting coral bleaching risk over entire decades has proved much more challenging.

Recent improvements in climate modelling now allow marine heatwaves and coral bleaching risks to be predicted with high accuracy. Using daily projections of heat stress from many global climate models, we show the severity and duration of coral bleaching will soon reach uncharted territory.

By mid-century coral bleaching is expected to start in spring for most of Earth’s reefs, rather than late summer as is typical today. In equatorial regions, corals will be at high risk of bleaching all year round by the end of the century.

In many regions, corals spawn only once a year. These spectacular mass spawning events happen in a single week following a full moon in spring.

By 2040, this spawning event could coincide with severe bleaching risk. This would greatly reduce their reproductive success, causing large-scale coral loss.

Acropora coral spawning on Magnetic Island in Queensland, Australia. Coral Brunner/Shutterstock

Equatorial regions most at risk

We show the future risk of severe coral bleaching is uneven globally.

The greatest risk is along the equator. Equatorial regions are home to the most biodiverse coral reefs, including conservation hotspots such as the Coral Triangle. To make matters worse, marine life in these regions is particularly vulnerable to accelerated climate change.

Many equatorial species are already living at temperatures near their upper tolerance. They also generally have low abilities to move to track shifting climates. This leaves them at high risk of extinction.

Future risk of coral bleaching under a high-emission scenario (top) and benefit from climate mitigation (bottom). Adapted from Mellin et al. Science Advances 2024

Our research shows equatorial regions are set to benefit least from efforts to curb emissions. We expect significant emission cuts will reduce the annual duration of severe bleaching conditions in all areas except these regions.

The projected highest climate impacts coincide with highest social reliance on coral reefs. This will challenge human populations that rely heavily on their local reefs for their livelihoods and nutrition.

Improving coral reef management

Our research identifies Earth’s reef regions that are at lowest risk of increased bleaching. This will help conservation managers and policymakers prioritise efforts to limit loss of coral reef biodiversity.

We predict much less risk of coral bleaching in regions such as the northern coasts of Venezuela and Colombia, Socotra Island (opposite the Gulf of Aden) and Alor Kecil in Indonesia. Seasonal upwellings occur here, bringing cooler water to the surface that’s likely to limit the severity of heatwaves.

Identifying these future havens for coral reefs will help maximise the success of coral conservation strategies such as assisted evolution, coral restoration or transplantation.

These strategies can help maintain healthy coral populations at local scales, particularly if used on reefs where future climate impacts will be lower. By pinpointing these havens, our research will strengthen coral conservation.

Our research includes a user-friendly web-based tool for mapping future coral bleaching. It will help pinpoint locations for effective management interventions.

Curbing greenhouse gas emissions is the main solution to reduce future climate impacts on corals. However, other strategies are also vital to maximise coral reefs’ adaptation to climate change.

Camille Mellin, Senior Lecturer and ARC Future Fellow, School of Biological Sciences, University of Adelaide and Damien Fordham, Associate Professor of Global Change Ecology, University of Adelaide

This article is republished from The Conversation under a Creative Commons license. Read the original article.