When you purchase through links on our site , we may earn an affiliate commission . Here ’s how it works .

2018 was a big class for dark matter .

As usual , stargazer did n’t actually find any of the stuff and nonsense , which is inconspicuous to all our telescope but come out to make up at least 80 percentage of the universe by mass .

A photo shows the underground water tank where LUX-ZEPLIN will eventually sit.

A photo shows the underground water tank where LUX-ZEPLIN will eventually sit.

There were reports ofa dark matter hurricane , but we ca n’t really see it . A galaxy was find that seemed not to have any coloured matter , which funnily would haveproved dark matter existed . But then it turned out that the galaxymay have sullen matter after all — leaving the existence of colored thing in doubt for some physicist . Multipleexperimentsthat were suppose to directly notice dark matter here on Earth turned up nothing .

So , where does that impart scientists hunting for dark thing as we head into 2019 ? Pretty affirmative , all things considered . The hunt for dark topic push forward on all fronts .

From massive underground detector to immense sky surveys , here are the four major steps in the hunting for dark matter to depend forward to in 2019 .

The LIGO project operates two detector sites: one near Hanford in eastern Washington, and another near Livingston, Louisiana (shown here).

The LIGO project operates two detector sites: one near Hanford in eastern Washington, and another near Livingston, Louisiana (shown here).

LIGO comes back online

The Laser Interferometer Gravitational - Wave Observatory ( LIGO ) , the American sensor that directly observed the first gravitative waves in 2015 , will begin its third observation run in other 2019 , collecting more data than ever before after a series of upgrades to its equipment .

So what ’s a gravitational - undulation detector doing in an article about dark matter ? It turn out that there are a lot oftantalizing possibilitiesfor uncover hints of dark matter using gravitational - wave information — though none of them have yet been realized .

Researchers in 2018 proposedthat if a " dark photon " with a very little mass lurks somewhere in the universe , its signaling might sour up in LIGO data , do very specific irregularities in the signatures of gravitative waves .

A photo reveals the inside of the MiniBOONE detector.

A photo reveals the inside of the MiniBOONE detector.

“ We show that both undercoat - based and future space - base gravitational wave detectors have the capableness to make a [ conclusive dark matter ] discovery , ” the researchers wrote .

With LIGO back online , turning up grounds for glowering matter in gravitative - wafture data is very much a unrecorded opening .

Physicists will try to figure out whether MiniBooNE gave up the ghost of a neutrino

Throughout 2018 , scientists chattered excitedly about intriguing result from an experiment at Fermilab National Accelerator Laboratory , called MiniBooNE , suggesting the presence of particles that should n’t subsist . The best explanation so far is that there ’s a quaternary , as - yet - undiscovered neutrino out there , called the aseptic neutrino , that interacts with the rest of the universe even less than its other neutrino cousins .

Some researchersbelievethat the sterile neutrino could be a nominee particle for dark topic , and as 2018 do to a close , physicists arefirming up their perspectiveson this anomaly . take care for scientist think in young ways about that data and infertile neutrino in general in 2019 .

First light at the Large Synoptic Survey Telescope (LSST)

There ’s a scope being built in Chile that will make detailed images of vast regions of the sky every 15 bit , complete a full scan of the sky every three days . Over the course of 10 years , it will compare those images to one another again and again to track how the sky shifts and change , provide the most in - deepness - ever imagination for realize how sour thing pushing and clout on the cosmos .

scientist know , broadly speaking , that sinister matter shapes the way galaxies and their star move and interact with one another . LSST ’s goal is to fill out that picture , offering an unprecedented level of detail on how the cosmos functions . That should offer astrophysicists a riches of data on the nature of grim thing and the role it plays in the universe .

And in 2019,for the first time , research worker will afford the 6,200 - lb.(2,800 kilograms ) eye of that telescope and take in illumination . Science operations begin in 2022 .

A photo from Nov. 2018 shows ongoing construction at Cerro Pachón summit, where the LSST is coming together.

A photo from Nov. 2018 shows ongoing construction at Cerro Pachón summit, where the LSST is coming together.

The race to build a next-generation detector will heat up

atom physicists have speculated for a long time that the first unmediated sign of dark issue might be a sparkle . Here ’s how it might cultivate : As blue issue collides with sluggish substances in very glum rooms , those subject matter would utter swooning specks of brightness level . For decade , scientists have build detectors agree to this precept , but so far , none have produced a conclusive result .

In 2019 , scientists inChinawill be severe at work on the PandaX platform , which gaze at xenon all day and night looking for a twinkle . Those scientists are apace elevate the sensor to accommodate a 4 - ton ( 3.6 MT ) xenon target , reportingthat they expect to complete most of that study over the course of 2019 and 2020 . The new demodulator will be called PandaX - crosstalk .

Not to be surpass , researchers in South Dakota will be completing the most important phases of construction onLUX - ZEPLIN , which will observe a full 10 lashings ( 9 tonnes ) of xenon nearly a mile under the townspeople of Lead , South Dakota . Like PandaX - xt , the project will likely not enwrap up until 2020 .

Researchers are hard at work a mile underground putting LUX-ZEPLIN together.

Researchers are hard at work a mile underground putting LUX-ZEPLIN together.

Italy will also move forward on advance its detector , suitably named XENON , to an 8 - ton ( 7.2 tonne ) scale . The upgrade , calledXENON - nt , should be wrap up in 2019 .

The next phase

It ’s always possible that some experiment somewhere will twist up incontrovertible , specific evidence that a exceptional kind of possible dark matter particle really exists . But in the short term , in almost every country , physicist are focus on using the lessons of the past to inform bigger , better dark topic hunts in the future . Will an demonstrable non-white affair finding turn up in 2019 ? That might be a bit affirmative . But the physicists chasing that goal are head into the young year arming themselves to hunt with more precision and might than ever before .

Originally bring out onLive scientific discipline .

a photo of the Large Hadron Collider

The Dark Energy Spectroscopic Instrument maps the night sky from the Nicholas U. Mayall 4-meter Telescope in Arizona.

A grainy image of a galaxy

an illustration of the Milky Way in the center of a blue cloud of gas

Atomic structure, large collider, CERN concept.

An abstract illustration of lines and geometric shapes over a starry background

Scientists think that dark matter produces a bright and spherical halo of X-ray emission around the center of the Milky Way.

This glowing red map shows the universe as seen in high-energy gamma rays.

dark matter

Fermi�s All-Sky Gamma-Ray Map

A Spiral Galaxy in Leo

Hubble Finds Dark Matter Ring in Galaxy Cluster

An image comparing the relative sizes of our solar system�s known dwarf planets, including the newly discovered 2017 OF201

an illustration showing a large disk of material around a star

a person holds a GLP-1 injector

A man with light skin and dark hair and beard leans back in a wooden boat, rowing with oars into the sea

an MRI scan of a brain

A photograph of two of Colossal�s genetically engineered wolves as pups.

An abstract illustration of rays of colorful light