Riskli Değil2026-07-08
(2019 AM12)
- Geçiş Mesafesi
- 10.787.227 km
- Çap
- 49 m
- Hız
- 18.135 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 Görseli2026-07-07
NGC 6188: Dragons of Ara
Where can you find dragons fighting in the night sky? In the southern constellation of the Altar: Ara. The dragons are, of course, actually made of suggestively shaped gas and dus...
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
KaynakPotansiyel Riskli2026-07-09
250680 (2005 QC5)
- Geçiş Mesafesi
- 30.472.665 km
- Çap
- 705 m
- Hız
- 54.708 km/h
Riskli Değil2026-07-07
(2016 XR1)
- Geçiş Mesafesi
- 38.966.151 km
- Çap
- 85 m
- Hız
- 37.299 km/h
Riskli Değil2026-07-07
(2015 DC1)
- Geçiş Mesafesi
- 42.457.614 km
- Çap
- 65 m
- Hız
- 19.032 km/h
Uzay Havası Uyarıları
KaynakFLR07.07.2026 14:09:00
Solar Flare M4.0
Class M4.0 flare detected from S11E50.
Kaynak: S11E50
Kaynağı AçCME07.07.2026 08:12:00
Coronal Mass Ejection
CME visible to the NW in SOHO LASCO C2/C3 and GOES CCOR-1 imagery. Not clearly visible in STEREO A COR2 imagery. The potential source may be an eruption from AR 14479 (approximately N15W105) as seen in STEREO A EUV 195/304 imagery starting around 2026-07-07T05:45Z. The eruption is best seen as brightening in both wavelengths.
Kaynak: N15W105
Kaynağı AçCME07.07.2026 05:00:00
Coronal Mass Ejection
Narrow, faint CME visible to the NE in SOHO LASCO C2/C3. Not clearly visible in GOES CCOR-1 or STEREO A COR2 imagery. The potential source is an eruption with dimming around N20E40 starting at 2026-07-07T03:52Z best seen in SDO AIA 193 imagery.
Kaynak: N20E40
Kaynağı AçCME06.07.2026 21:09:00
Coronal Mass Ejection
Faint CME observed to the SE only in STEREO A COR2, not observed in SOHO LASCO C2/C3 or GOES CCOR-1. The source is likely AR 14483 with field line movement and brightening centered ~S07W40, followed by dimming, starting around 2026-07-06T18:58Z in SDO AIA 171/193.
Kaynak: S07W40
Kaynağı AçCME06.07.2026 19:12:00
Coronal Mass Ejection
Faint CME observed to the W only in SOHO LASCO C2. Source is likely former AR 14479, with brightening and filament ejecta in STEREO A EUVI 195/304 at 2026-07-06T18:25Z centered approximately ~N10W110. Also observed in SDO AIA 171/193/304 as filament ejecta and field line movement around the west limb.
Kaynak: N10W110
Kaynağı AçCME06.07.2026 17:36:00
Coronal Mass Ejection
Faint CME observed to the NW in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. No distinct source on the disk is observed, but loop brightening on/beyond the west limb in SDO AIA 171 starting around 2026-07-06T17:18Z suggests former AR 14479 over the west limb is a likely weak eruptive source.
Kaynak: Solar corona
Kaynağı Aç