Hubble Peers at Peculiar Pair of Galaxies

Images

Friday, 25 February 2022

This striking image from the NASA/ESA Hubble Space Telescope showcases Arp 298, a stunning pair of interacting galaxies. Arp 298 – which comprises the two galaxies NGC 7469 and IC 5283 – lies roughly 200 million light-years from Earth in the constellation Pegasus.

Planetary Positions

21.11.2024 at 22:30:38 UTC

Planet	Longitude
The Sun	00 Sag 06' 29"
The Moon	17 Leo 23' 46"
Mercury	21 Sag 24' 47"
Venus	12 Cap 04' 29"
Mars	04 Leo 44' 32"
Jupiter	18 Gem 21' 46" R
Saturn	12 Pis 43' 41"
Uranus	25 Tau 02' 26" R
Neptune	27 Pis 12' 15" R
Pluto	00 Aqu 02' 18"

Solar Status

BZ Status:	0
Proton Density:	5.23
Proton Speed:	422.1 k/sec
KP Status:	3.00

Type	Nov 22	Nov 23	Nov 24
Active	25%	25%	25%
Minor	15%	15%	15%
Moderate	1%	1%	1%
Strong	1%	1%	1%
Kp Index Prediction
00-03UT	2.00	2.33	2.33
03-06UT	1.67	3.00	2.67
06-09UT	2.33	2.33	2.33
09-12UT	1.00	2.00	2.33
12-15UT	1.33	1.33	2.00
15-18UT	1.67	1.33	2.00
18-21UT	3.00	1.67	2.00
21-00UT	3.00	2.33	1.67
Solar Activity
Solar activity reached moderate levels following a long-duration M1.1 flare at 20/1948 UTC from Region 3897 (S12W90, Dao/beta) as it transited the west limb. This region also produced the majority of the C-class flare activity during the period. Region 3898 (S16W27, Cao/beta) exhibited slight decay early in the period, but then had some redevelopment later and managed to produced a C3.5 flare at 20/0632 UTC. Region 3901 (S07E35, Dao/beta-gamma) added a pair of low-level C-class flares, but remained mostly unchanged. The remaining regions were quiescent. New Region 3902 (S17E70, Cso/beta) was numbered. While several CMEs were observed in SOHO/LASCO coronagraph imagery, none were deemed Earth-directed.
Solar Wind
Solar wind parameters reflected a weakly enhanced solar wind regime early, before transitioning to background levels the latter half of the period. Solar wind speeds ranged between 350 km/s - 400 km/s. Total field strength averaged near 10nT, reached a peak of 13 nT, then decreased to remain near 5-8 nT the last half of the period. The Bz component fluctuated between +9/-10 nT before turning mostly north, and the phi angle was predominantly in a positive orientation.
Energetic Particle
The greater than 2 MeV electron flux was normal to moderate and the greater than 10 MeV proton flux was at background levels.

Hubble Peers at Peculiar Pair of Galaxies

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