Riskli Değil2026-09-10
(2014 FV32)
- Geçiş Mesafesi
- 12.283.851 km
- Çap
- 179 m
- Hız
- 38.120 km/h
Evrenin Sırlarını
Keşfet
Amatör astronomlar için nihai gözlem takvimi. Yaklaşan meteor yağmurları, gezegen sıralanmaları, uzay istasyonu geçişleri, atmosferik şartlar ve NASA canlı verileri tek yerde.
Günün Görseli2026-09-08
Hubble: Decagon Around Saturn's South Pole
Why are Saturn’s poles geometric? Saturn’s North Pole has been known to be surrounded by a hexagonal (6 sides) cloud since discovery in 1987 in data taken by NASA’s Voyager spacecr...
NASA Bugün
Yaklaşan Gökyüzü Olayları
Tümünü GörMeteor Yagmuru12/13 Agu
Perseid Meteor Yagmuru Zirvesi
Her yil guvenilir sekilde gozlenen, parlak ve sik meteorlar uretebilen yillik meteor yagmurlarindan biridir.
Meteor Yagmuru13/14 Ara
Geminid Meteor Yagmuru Zirvesi
Geminidler genellikle yilin en guclu meteor yagmurlarindan biri olarak kabul edilir.
Bu Gece Gözlem Şartları
Canlı gözlem verisi yükleniyor...
Yakın Dünya Cisimleri
KaynakRiskli Değil2026-09-09
(2013 TG135)
- Geçiş Mesafesi
- 15.999.594 km
- Çap
- 54 m
- Hız
- 47.017 km/h
Riskli Değil2026-09-08
(2013 OY3)
- Geçiş Mesafesi
- 16.552.739 km
- Çap
- 66 m
- Hız
- 24.152 km/h
Riskli Değil2026-09-09
(2020 CN1)
- Geçiş Mesafesi
- 27.159.650 km
- Çap
- 171 m
- Hız
- 39.469 km/h
Uzay Havası Uyarıları
KaynakCME07.09.2026 09:23:00
Coronal Mass Ejection
This CME is visible to the northeast in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery. The source may be related to an eruption from Active Region 14524 (N12E22) starting around 2026-09-07T08:00Z as seen in SDO AIA 131/171/193/304, GOES SUVI 131/171/195/284/304, and STEREO A EUVI 195/304 imagery. Dimming is observed north of the eruption site in SDO AIA 193 imagery, with an opening of field lines visible over the northeast limb in STEREO A EUVI 195 imagery, indicating northern deflection.
Kaynak: N12E22
Kaynağı AçCME07.09.2026 02:48:00
Coronal Mass Ejection
This CME is visible to the northwest in SOHO LASCO C2/C3, GOES CCOR-1 (partially obscured by the pylon), and STEREO A COR2 imagery. The source is a slow-to-lift-off filament eruption visible over the northwest limb in SDO AIA 171/304 and GOES SUVI 171/284/304 imagery starting around 2026-09-06T22:00Z. This same filament is visible lifting off north of disk center as seen in STEREO A EUVI 195/304 imagery.
Kaynak: Solar corona
Kaynağı AçCME07.09.2026 01:48:00
Coronal Mass Ejection
This CME is visible to the east in SOHO LASCO C2/C3 and GOES CCOR-1 imagery, and to the west in STEREO A COR2 imagery. The source is far-sided and likely related to an opening of field lines visible over eastern limb in SDO AIA 171/193 and GOES SUVI 171/195/284 imagery starting around 2026-09-07T00:50Z.
Kaynak: Solar corona
Kaynağı AçCME06.09.2026 21:53:00
Coronal Mass Ejection
Very faint feature seen only seen to the NE part way into the FOV of STEREO A COR2 after a data gap ending at 2026-09-06T21:53Z. A possible source candidate is a small amount of ejecta seen over the ENE limb in SDO AIA 304 beginning around 2026-09-06T18:35Z.
Kaynak: Solar corona
Kaynağı AçCME06.09.2026 10:53:00
Coronal Mass Ejection
This CME is visible to the east in STEREO A COR2 imagery only. This event is not seen in SOHO LASCO C2/C3 or GOES CCOR-1 in real-time due to data gaps starting around 2206-09-06T03:30Z. The source is an eruption and C5.0 flare from Active Region 14524 (N12E32) starting around 2026-09-06T10:36Z as seen in SDO AIA 131/171/193/304, GOES SUVI 131/171/195/284/304, and STEREO A EUVI 304 imagery. An EUV wave and subsequent dimming is observed moving south of the eruption site, seen in SDO AIA 193 and GOES SUVI 195 imagery.
Kaynak: N12E32
Kaynağı AçFLR06.09.2026 10:31:00
Solar Flare C5.0
Class C5.0 flare detected from N12E32.
Kaynak: N12E32
Kaynağı Aç