All About Space - UK (2020-02)

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NASA’s solar probe spots ‘stealth’


outburst on the Sun


Coronalmassejections(CMEs)aren’tknownfor
beingsubtle:eacheventcanf linghugeamountsof
thesoupofchargedparticlescalledplasmaoffthe
SunandoutintotheSolarSystem.InNovember
2018,asseenfromEarthandcertainspacecraft,
theSunseemedtobecalm...butitwasn’t.Itwas
experiencingwhatscientistscalla ‘stealth’coronal
massejection.Conveniently,NASA’sParkerSolar
Probewascompletingitsfirstclosepassbehindthe
Sunatthetime,puttingitsinstrumentsina perfect
positiontoseewhatwashappeningon 11 and 12
Novemberduringthisusuallycrypticevent.
“Ifyou’veeverseena CMEimage,younormally
seea lotofactivityintheseimages,”KellyKorreck,
a solarphysicistattheSmithsonianAstrophysical
Observatory,said.“Youwouldseea largeblowout;
youwouldprobablyseeoneoftheseexploding.But
therewasn’tmuchthere.”

EveninsomeoftheParkerSolarProbedata,it
wasn’tobviousatfirstwhatwashappeningduring
theincident,Korrecksaid.“Whenwelookedat
thisinitially– justthethermaldata– wedidn’t
necessarilythinkthattherewasa coronalmass
ejectionthere.”Butotherobservationstargeting
energeticparticlesdidincludethefingerprintofa
shock,a phenomenonthatusuallyaccompanies
a coronalmassejection.Scientistscouldalso
confirmtheprobewasflyingthrougha coronal
massejectionbasedondataitsinstrumentswere
gatheringaboutthemagneticfield.
Seeinga stealthcoronalmassejectionisa stepin
therightdirection.“They’resomethingthatwe’re
nottraditionallyabletoseeinthewaysthatwe’ve
previouslydetectedcoronalmassejections,”Korreck
said.“We’restartingtoseehintsofthemwithbetter
andbettertelescoperesolution.”

WordsbyMeg ha nBa r tels

Pluto’s heart


powers
icy winds
Words by M i ke Wa l l
The dwarf planet’s famous
heart-shaped feature, which
NASA’sNewHorizons
discoveredduringitsepic
July 2015 f lyby,drives
atmosphericcirculation
patternsonPluto.
Mostoftheactioncomes
courtesyoftheheart’sleft
lobe,a 1,000-kilometre(600-
mile)widenitrogen-iceplain
calledSputnikPlanitia.This
exoticicevaporisesduring
thedayandcondensesinto
iceagainatnight,causing
nitrogenwindstoblow.
Thesewindscarryheat,
particlesofhazeandgrains
oficewestward,stainingthe
icestherewithdarkstreaks.
“Thishighlightsthefact
thatPluto’satmosphereand
winds– evenifthedensity
oftheatmosphereisvery
low– canimpactthesurface,”
saidTanguyBertrand,an
astrophysicistandplanetary
scientistatNASA’sAmes
ResearchCenterinCalifornia.
Andthatwestward
directionisinteresting
initself,consideringthat
Plutospinseastwardon
itsaxis.Thedwarfplanet’s
atmospherethereforeexhibits
anodd‘retrorotation’.
Thisworkrevealedthe
likelypresenceofwesterly
winds– a high-altitude
varietythatracesalongat
leastfourkilometres(2.
miles)abovethesurfaceand
a fast-movingtypecloser
tothegroundthatfollows
Sputnik’swesternedge.

Stellar showdown spawns


spectacular rainbow cloud
WordsbySamanthaMathewson

UsingtheAtacamaLargeMillimeter/submillimeter
Array(ALMA),astronomersobservedthebinary
starsystemcalledHD101584,revealinga peculiar
gascloudthatisbelievedtobetheresultofa
confrontationbetweenthetwostars,accordingto
theEuropeanSouthernObservatory.
DatafromALMAandtheAtacamaPathfinder
EXperiment(APEX)showsthatoneofthestars
grewsolargethatitengulfedtheother.Asthe
smallerstarspiralledtowardsitsgiantstellar
companion,itcausedthelarger,Sun-likestarto
sheditsouterlayers,resultingintheexpanding
cloudsofgascapturedinthenewlyreleased
ALMAimages.
BasedontheALMAobservations,theresearchers
suggestthelow-masscompanionstarwascaptured
bytheredgiantstarwhenitreacheda criticalsize
onlya fewhundredyearsago.

Above:The
ParkerSolar
Probewasin
therightplace
attheright
timetospot
thissecretive
outburst

Left:Nitrogen
winds
havebeen
discovered
blowing
onPluto

Right:The
rainbow
resulted
froma binary
starmerger

© ALMA/ESO


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