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The space junk is forecast to reentry at UTC +/- 8 hours

Forecast of Reentry Location


Update Sat 24-Feb-2018 14:10 UTC

The map above shows the location of the possible reentry of the space junk () predicted by modeling of orbital evolution until the fragment or satellite reaches the altitude of nominal burst.

According to the forecast made by Satview.org, the object's reentry will occur in at UTC, above the coordinates shown on map.

Satellite Launch Norad Incl.
degrees
Apogee
Km
Perigee
Km
Period
min
Options
SL-23 R/B
Reentry: (YMD) 2018-01-28
201743090U5115512387Reentered!
Lat=-9.2   Lon=285.7
MINOTAUR R/B
Reentry: (YMD) 2018-02-3
200629053U7213612887Reentered!
Lat=68.9   Lon=147.4
GSLV R/B
Reentry: (YMD) 2018-02-8
201742748U21147997101Reentered!
Lat=21.1   Lon=341.9
SL-4 R/B
Reentry: (YMD) 2018-02-16
201843212U5215014087Reentered!
Lat=48.4   Lon=262
FLOCK 2E'-10
Reentry: (YMD) 2018-02-17
199841576U5218618088Reentered!
Lat=1   Lon=9.5
FLOCK 2E-10
Reentry: (YMD) 2018-02-28
199841572U5225123689Forecast
FLOCK 2E'-12
Reentry: (YMD) 2018-02-28
199841578U5224022589Forecast
STARS-C
Reentry: (YMD) 2018-03-2
199841895U5225124089Forecast
GSLV R/B
Reentry: (YMD) 2018-03-2
201540881U20105212996Forecast
FLOCK 2E-11
Reentry: (YMD) 2018-03-3
199841574U5226625290Forecast
FLOCK 2E-12
Reentry: (YMD) 2018-03-3
199841573U5226525390Forecast
FLOCK 2E-4
Reentry: (YMD) 2018-03-4
199841487U5227226090Forecast
COLUMBIA
Reentry: (YMD) 2018-03-6
199842702U5227926990Forecast
FLOCK 2E'-11
Reentry: (YMD) 2018-03-9
199841577U5228827790Forecast
GRACE-1
Reentry: (YMD) 2018-03-11
200227391U8924723889Forecast
AGGIESAT 4
Reentry: (YMD) 2018-03-11
199841313U5225224389Forecast
FLOCK 2E'-9
Reentry: (YMD) 2018-03-17
199841575U5227026090Forecast
ATLANTIS
Reentry: (YMD) 2018-03-24
199842737U5231330991Forecast
IRIDIUM 23 [P]
Reentry: (YMD) 2018-03-26
199724906U8666117993Forecast
HUMANITY STAR
Reentry: (YMD) 2018-03-26
201843168U8344027892Forecast
FLOCK 2E-3
Reentry: (YMD) 2018-04-1
199841486U5231130591Forecast
FLOCK 2E'-6
Reentry: (YMD) 2018-04-4
199841568U5231831091Forecast
PSLV R/B
Reentry: (YMD) 2018-04-7
201238249U9727727390Forecast
LEMUR-2-TRUTNA
Reentry: (YMD) 2018-04-7
199842067U5231531491Forecast
TIANGONG 1
Reentry: (YMD) 2018-04-8
201137820U4326724690Forecast
IRIDIUM 19 [-]
Reentry: (YMD) 2018-04-13
199724965U8653521892Forecast
FLOCK 2E'-1
Reentry: (YMD) 2018-04-26
199841479U5230229891Forecast
FLOCK 2E'-3
Reentry: (YMD) 2018-04-29
199841480U5230930691Forecast
FLOCK 2E'-8
Reentry: (YMD) 2018-04-30
199841569U5230129690Forecast
SGSAT
Reentry: (YMD) 2018-05-5
199842703U5233433391Forecast
FLOCK 2E-7
Reentry: (YMD) 2018-05-9
199841565U5230730191Forecast
TECHEDSAT 6
Reentry: (YMD) 2018-05-11
199843026U5237336992Forecast
FLOCK 2E'-19
Reentry: (YMD) 2018-05-12
199841777U5234234191Forecast
EAGLE 2
Reentry: (YMD) 2018-05-17
201339436U9839138292Forecast
FLOCK 2E'-16
Reentry: (YMD) 2018-05-21
199841763U5234233991Forecast
DELTA 2 R/B(2) (PAM-D)
Reentry: (YMD) 2018-05-22
200428476U39115818698Forecast
IRIDIUM 37 [P]
Reentry: (YMD) 2018-05-25
199724968U8665221993Forecast
FLOCK 2E'-17
Reentry: (YMD) 2018-06-4
199841776U5235134792Forecast
FLOCK 2E'-13
Reentry: (YMD) 2018-06-5
199841761U5234634291Forecast
FLOCK 2E-1
Reentry: (YMD) 2018-06-9
199841483U5232632491Forecast
SS-520-5 R/B
Reentry: (YMD) 2018-06-17
201843202U311844185105Forecast
CHALLENGER
Reentry: (YMD) 2018-07-12
199842721U5235935392Forecast
PSLV R/B
Reentry: (YMD) 2018-07-16
201742796U9532730091Forecast
DUTHSAT
Reentry: (YMD) 2018-07-24
199842724U5236135692Forecast
SL-4 R/B
Reentry: (YMD) 2018-07-28
201641395U9837528691Forecast
WASEDA-SAT3
Reentry: (YMD) 2018-08-7
199841933U5235334992Forecast
LINK
Reentry: (YMD) 2018-08-17
199842714U5236336192Forecast
LEMUR-2-AUSTINTACIOUS
Reentry: (YMD) 2018-08-22
199842068U5235735192Forecast
TRICOM-1R (TASUKI)
Reentry: (YMD) 2018-08-22
201843201U311879185106Forecast
LEMUR-2-TRUTNAHD
Reentry: (YMD) 2018-08-23
199842069U5236235692Forecast
AOBA-VELOX 3
Reentry: (YMD) 2018-08-27
199841935U5235635392Forecast
CZ-4B R/B
Reentry: (YMD) 2018-09-3
201742762U4343525391Forecast
IRIDIUM 40 [-]
Reentry: (YMD) 2018-09-4
199725041U8652127092Forecast
LEMUR-2-REDFERN-GOES
Reentry: (YMD) 2018-09-6
199842059U5236535892Forecast




The Satellite Path


The path to be followed by satellite (dotted line) does not change due to the fact that the satellite is falling and can be used to assess the trajectory of the object before and after possible fall. In the graph, each point marks the range of 1 minute.

Solar Flux and Other Variables


As much as the institutes and space agencies strive to provide correct data of the point where the space debris will fall, several factors may interfere with the accuracy of the prediction. Among the most important, the solar flux is the most critical because it determines the conditions of the upper atmosphere, increasing or decreasing the drag on the object.

Besides the solar flux acting on the aerodynamic characteristics, another variable rather difficult to be computed is the resistance of materials used in the construction of the object and the shape of the structure. Combined, these factors may determine different altitudes for the moment of rupture, causing errors of more than 30 km in altitude reentry provided.

Other variables that affect the calculation of reentry, although less important, are the gravitational perturbations of the Sun and Moon and also those exercised by large mountain ranges, above or below sea level.

The modeling used by Satview to compute the time of reentry uses solar flux data obtained at the time of modeling, and prediction of the behavior of the sun for the next 5 days. With this, the margin of error of prediction is + / - 3 revolutions for satellites or debris in uncontrolled reentry.

Altitude of Reentry


Spacecraft reentering the atmosphere without control usually break between 72 and 84 km altitude due to temperature and aerodynamic forces acting on the structure.

The nominal breakup altitude is 78 km, but big satellites that have larger and denser structures survive longer and break down at lower altitudes. Usually, solar panels are destroyed before any component, at altitudes between 90 and 95 km.

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