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Observable comet count is 1177
Current exoplanet count is 5834
Current longitude II of the GRS is 68°
Impact Probablity of 2024 YR4: 0.16%
Asteroid | Size | Probability | Date |
2024 YR4 | 40—90 m | 0.16% | 22 December 2032 |
Please do not let this worry you. The asteroid has been detected just recently meaning that the orbital elements are not yet accurately determined, while they can alter any time due to gravitational pulls.
Today Monitor
Mars: January 16, 2025
Jupiter: January 10, 2026
Saturn: September 21, 2025
Uranus: November 21, 2025
Neptune: September 23, 2025
Evening: January 10, 2025 at 47.2°E
Morning: June 1, 2025 at 45.9°W
Morning: December 25, 2024 at 22.0°W
Evening: March 8, 2025 at 18.2°E
Morning: April 21, 2025 at 27.4°W
Evening: July 4, 2025 at 25.9°E
Morning: August 19, 2025 at 18.6°W
Evening: October 29, 2025 at 23.9°E
Morning: December 7, 2025 at 20.7°W
Evening: Febrary 19, 2026 at 18.1°E
Wednesday, 5 November
Friday, 5 December
given for 00:00 UT
Date | Size | Age | Angle | Phase |
---|---|---|---|---|
23 Feb 2025 | 30.61' | 24.48 | -6.502° | ![]() |
24 Feb 2025 | 31.06' | 25.48 | -6.683° | ![]() |
25 Feb 2025 | 31.54' | 26.48 | -6.463° | ![]() |
22 Mar 2025 | 30.16' | 21.97 | -6.602° | ![]() |
23 Mar 2025 | 30.54' | 22.97 | -7.220° | ![]() |
24 Mar 2025 | 31.00' | 23.97 | -7.497° | ![]() |
25 Mar 2025 | 31.50' | 24.97 | -7.380° | ![]() |
26 Mar 2025 | 32.03' | 25.97 | -6.841° | ![]() |
04 Apr 2025 | 31.86' | 5.54 | 6.674° | ![]() |
05 Apr 2025 | 31.40' | 6.54 | 7.159° | ![]() |
06 Apr 2025 | 30.97' | 7.54 | 7.233° | ![]() |
07 Apr 2025 | 30.58' | 8.54 | 6.935° | ![]() |
19 Apr 2025 | 30.14' | 20.54 | -6.609° | ![]() |
20 Apr 2025 | 30.49' | 21.54 | -7.247° | ![]() |
21 Apr 2025 | 30.91' | 22.54 | -7.602° | ![]() |
22 Apr 2025 | 31.38' | 23.54 | -7.618° | ![]() |
23 Apr 2025 | 31.89' | 24.54 | -7.248° | ![]() |
24 Apr 2025 | 32.39' | 25.54 | -6.459° | ![]() |
02 May 2025 | 32.05' | 4.19 | 6.908° | ![]() |
03 May 2025 | 31.53' | 5.19 | 7.524° | ![]() |
04 May 2025 | 31.04' | 6.19 | 7.652° | ![]() |
05 May 2025 | 30.59' | 7.19 | 7.335° | ![]() |
06 May 2025 | 30.21' | 8.19 | 6.642° | ![]() |
18 May 2025 | 30.56' | 20.19 | -6.624° | ![]() |
19 May 2025 | 30.92' | 21.19 | -6.950° | ![]() |
20 May 2025 | 31.32' | 22.19 | -7.010° | ![]() |
21 May 2025 | 31.75' | 23.19 | -6.758° | ![]() |
30 May 2025 | 32.13' | 2.87 | 6.436° | ![]() |
31 May 2025 | 31.63' | 3.87 | 7.137° | ![]() |
01 Jun 2025 | 31.12' | 4.87 | 7.336° | ![]() |
02 Jun 2025 | 30.65' | 5.87 | 7.064° | ![]() |
29 Jun 2025 | 31.11' | 3.56 | 6.528° | ![]() |
02 Oct 2025 | 30.80' | 10.17 | -6.602° | ![]() |
03 Oct 2025 | 31.28' | 11.17 | -6.712° | ![]() |
04 Oct 2025 | 31.79' | 12.17 | -6.413° | ![]() |
13 Oct 2025 | 32.01' | 21.17 | 6.426° | ![]() |
14 Oct 2025 | 31.60' | 22.17 | 7.017° | ![]() |
15 Oct 2025 | 31.20' | 23.17 | 7.219° | ![]() |
16 Oct 2025 | 30.83' | 24.17 | 7.068° | ![]() |
17 Oct 2025 | 30.51' | 25.17 | 6.617° | ![]() |
29 Oct 2025 | 30.28' | 7.48 | -6.622° | ![]() |
30 Oct 2025 | 30.70' | 8.48 | -7.213° | ![]() |
31 Oct 2025 | 31.18' | 9.48 | -7.461° | ![]() |
01 Nov 2025 | 31.71' | 10.48 | -7.298° | ![]() |
02 Nov 2025 | 32.24' | 11.48 | -6.672° | ![]() |
10 Nov 2025 | 32.23' | 19.48 | 7.097° | ![]() |
11 Nov 2025 | 31.72' | 20.48 | 7.804° | ![]() |
12 Nov 2025 | 31.23' | 21.48 | 8.024° | ![]() |
13 Nov 2025 | 30.78' | 22.48 | 7.808° | ![]() |
14 Nov 2025 | 30.39' | 23.48 | 7.230° | ![]() |
26 Nov 2025 | 30.27' | 5.72 | -6.459° | ![]() |
27 Nov 2025 | 30.63' | 6.72 | -7.095° | ![]() |
28 Nov 2025 | 31.05' | 7.72 | -7.447° | ![]() |
29 Nov 2025 | 31.52' | 8.72 | -7.439° | ![]() |
30 Nov 2025 | 32.02' | 9.72 | -7.008° | ![]() |
08 Dec 2025 | 32.44' | 17.72 | 6.680° | ![]() |
09 Dec 2025 | 31.91' | 18.72 | 7.561° | ![]() |
10 Dec 2025 | 31.38' | 19.72 | 7.916° | ![]() |
11 Dec 2025 | 30.87' | 20.72 | 7.788° | ![]() |
12 Dec 2025 | 30.43' | 21.72 | 7.247° | ![]() |
26 Dec 2025 | 31.06' | 5.93 | -6.615° | ![]() |
27 Dec 2025 | 31.43' | 6.93 | -6.624° | ![]() |
Date | Size | Age | Angle | Phase |
---|---|---|---|---|
12 Jan 2025 | 31.85' | 12.07 | -6.565° | ![]() |
13 Jan 2025 | 31.60' | 13.07 | -6.448° | ![]() |
26 Jan 2025 | 30.57' | 26.07 | 6.621° | ![]() |
27 Jan 2025 | 30.96' | 27.07 | 6.622° | ![]() |
08 Feb 2025 | 31.60' | 9.48 | -6.682° | ![]() |
09 Feb 2025 | 31.36' | 10.48 | -6.624° | ![]() |
22 Feb 2025 | 30.21' | 23.48 | 6.703° | ![]() |
23 Feb 2025 | 30.61' | 24.48 | 6.800° | ![]() |
24 Feb 2025 | 31.06' | 25.48 | 6.559° | ![]() |
07 Mar 2025 | 31.74' | 6.97 | -6.762° | ![]() |
08 Mar 2025 | 31.39' | 7.97 | -6.766° | ![]() |
09 Mar 2025 | 31.05' | 8.97 | -6.404° | ![]() |
21 Mar 2025 | 29.85' | 20.97 | 6.665° | ![]() |
22 Mar 2025 | 30.16' | 21.97 | 6.852° | ![]() |
23 Mar 2025 | 30.54' | 22.97 | 6.721° | ![]() |
03 Apr 2025 | 32.33' | 4.54 | -6.682° | ![]() |
04 Apr 2025 | 31.86' | 5.54 | -6.784° | ![]() |
05 Apr 2025 | 31.40' | 6.54 | -6.493° | ![]() |
17 Apr 2025 | 29.65' | 18.54 | 6.506° | ![]() |
18 Apr 2025 | 29.86' | 19.54 | 6.754° | ![]() |
19 Apr 2025 | 30.14' | 20.54 | 6.698° | ![]() |
30 Apr 2025 | 32.98' | 2.19 | -6.438° | ![]() |
01 May 2025 | 32.55' | 3.19 | -6.675° | ![]() |
02 May 2025 | 32.05' | 4.19 | -6.485° | ![]() |
15 May 2025 | 29.78' | 17.19 | 6.605° | ![]() |
16 May 2025 | 29.99' | 18.19 | 6.587° | ![]() |
28 May 2025 | 32.97' | 0.87 | -6.528° | ![]() |
29 May 2025 | 32.60' | 1.87 | -6.460° | ![]() |
11 Jun 2025 | 29.82' | 14.87 | 6.526° | ![]() |
12 Jun 2025 | 30.02' | 15.87 | 6.530° | ![]() |
24 Jun 2025 | 32.85' | 27.87 | -6.457° | ![]() |
25 Jun 2025 | 32.68' | 28.87 | -6.502° | ![]() |
08 Jul 2025 | 29.84' | 12.56 | 6.561° | ![]() |
09 Jul 2025 | 30.07' | 13.56 | 6.600° | ![]() |
21 Jul 2025 | 32.45' | 25.56 | -6.493° | ![]() |
22 Jul 2025 | 32.38' | 26.56 | -6.624° | ![]() |
04 Aug 2025 | 29.76' | 10.20 | 6.646° | ![]() |
05 Aug 2025 | 29.99' | 11.20 | 6.748° | ![]() |
06 Aug 2025 | 30.28' | 12.20 | 6.541° | ![]() |
17 Aug 2025 | 32.23' | 23.20 | -6.553° | ![]() |
18 Aug 2025 | 32.11' | 24.20 | -6.755° | ![]() |
19 Aug 2025 | 31.94' | 25.20 | -6.550° | ![]() |
31 Aug 2025 | 29.61' | 7.75 | 6.661° | ![]() |
01 Sep 2025 | 29.78' | 8.75 | 6.848° | ![]() |
02 Sep 2025 | 30.05' | 9.75 | 6.733° | ![]() |
13 Sep 2025 | 32.46' | 20.75 | -6.508° | ![]() |
14 Sep 2025 | 32.22' | 21.75 | -6.794° | ![]() |
15 Sep 2025 | 31.95' | 22.75 | -6.665° | ![]() |
27 Sep 2025 | 29.47' | 5.17 | 6.540° | ![]() |
28 Sep 2025 | 29.56' | 6.17 | 6.805° | ![]() |
29 Sep 2025 | 29.74' | 7.17 | 6.779° | ![]() |
30 Sep 2025 | 30.01' | 8.17 | 6.453° | ![]() |
11 Oct 2025 | 32.77' | 19.17 | -6.687° | ![]() |
12 Oct 2025 | 32.41' | 20.17 | -6.652° | ![]() |
25 Oct 2025 | 29.42' | 3.48 | 6.651° | ![]() |
26 Oct 2025 | 29.52' | 4.48 | 6.681° | ![]() |
27 Oct 2025 | 29.69' | 5.48 | 6.423° | ![]() |
07 Nov 2025 | 33.37' | 16.48 | -6.472° | ![]() |
08 Nov 2025 | 33.10' | 17.48 | -6.565° | ![]() |
21 Nov 2025 | 29.39' | 0.72 | 6.513° | ![]() |
22 Nov 2025 | 29.46' | 1.72 | 6.567° | ![]() |
05 Dec 2025 | 33.44' | 14.72 | -6.511° | ![]() |
18 Dec 2025 | 29.42' | 27.72 | 6.502° | ![]() |
19 Dec 2025 | 29.48' | 28.72 | 6.570° | ![]() |
Source: NASA/GSFC
Webb Reveals Rapid-Fire Light Show From Milky Way's Central Black Hole
February 18, 2025
A large, black circle representing a black hole occupies the right third of the frame in this illustration. Thick, clumpy orange streaks arc above and below it, essentially surrounding it. The top arc extends down to the lower left and then curves around in front of the black hole to form a disk that is tilted toward the viewer. Near the inner edge of the disk, several bright, whiter spots have blue filaments looping above them, representing flares. The words “Artist’s Concept” appear in the bottom left corner in gray.
Source: stsci.edu/news
13 January 2025
Astronomers using the NASA/ESA/CSA James Webb Space Telescope have identified two stars responsible for generating carbon-rich dust a mere 5000 light-years away in our own Milky Way galaxy. As the massive stars in Wolf-Rayet 140 swing past one another on their elongated orbits, their winds collide and produce the carbon-rich dust. For a few months every eight years, the stars form a new shell of dust that expands outward — and may eventually go on to become part of stars that form elsewhere in our galaxy.
Source: esawebb.org
4 February 2025
This new NASA/ESA/CSA James Webb Space Telescope Picture of the Month presents HH 30 in unprecedented resolution. This target is an edge-on protoplanetary disc that is surrounded by jets and a disc wind, and is located in the dark cloud LDN 1551 in the Taurus Molecular Cloud. Herbig-Haro objects are small nebulae found in star formation regions, marking the locations where gas outflowing from young stars is heated into luminescence by shockwaves. HH 30 is an example of where this outflowing gas takes the form of a narrow jet. The source star is located on one end of the jet, hidden behind an edge-on protoplanetary disc that the star is illuminating. HH 30 is of particular interest to astronomers. In fact, the HH 30 disc is considered the prototype of an edge-on disc, thanks to its early discovery with the NASA/ESA Hubble Space Telescope. Discs seen from this view are …
Source: esawebb.org
Engineers with NASA’s Exploration Ground Systems complete stacking operations on the twin SLS (Space Launch System) solid rocket boosters for Artemis II by integrating the nose cones atop the forward assemblies inside the Vehicle Assembly Building’s High Bay 3 at NASA’s Kennedy Space Center in Florida on Wednesday, Feb. 19, 2025. The twin solid boosters will help support the remaining rocket components and the Orion spacecraft during final assembly of the Artemis II Moon rocket and provide more than 75 percent of the total SLS thrust during liftoff from NASA Kennedy’s Launch Pad 39B.
Click to enlarge or show full screenThu, 20 Feb 2025 17:03 GMT
Source: www.nasa.gov
Image credit: European Space Agency
2025-02-07 solar system
2024 YR4 is an extremely faint asteroid with a low albedo of 5% to 25% and is 40 to 90 meters in size which, as of today, has a minute 2.2% probability of impacting Earth at 14:02 UTC on December 22, 2032. The asteroid rotates around its axis every 19.5 minutes and travels around the sun on a highly 0.662 eccentric orbit plane once in about 4 years at a mean distance of 2.5165 AU. Its last perihelion (sun passage) occurred on 2024-Nov-22. The iron-nickel asteroid that created the Barringer Crater in Arizona 50,000 years ago was about 50 meters wide. Link to source 🔗
Image credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)
2025-02-01 Exoplanets
Gliese 12 (TOI-6251) is a red dwarf star some 40 light-years away in Pisces. Its known planet, b, about the same size as Venus and, because a red dwarf is much cooler than our sun, the planet also receives the same amount of energy from its host star although orbiting much closer and once in about 12.8 days. In astronomical terms, the planet lies nearby and is a potentially terrestrial, temperate exoplanet inviting further investigations, such as atmospheric spectroscopy with the help of the JWST. Link to source 🔗
Image credit: NASA/JPL-Caltech
2025-01-31 Universe
Scheduled for launch past February 2025, SPHEREx is NASA's latest orbiting space telescope, designed for a spectral survey of the entire sky for a duration of tentatively two years in order to explore the origins of the universe. Link to source 🔗
Image credit: NASA / CXC / A. Hobart / Josh Barnes, University of Hawaii / John Hibbard, NRAO
2025-01-20 galaxies
Astronomers at the University of Tokyo discovered a rare quasar-like object with a long-term periodic luminosity variation with a cycle of about 190 days. Two black holes moving periodically at high speed may be the cause of the variability, hypothetically a supermassive blackhole binary. The extremely luminous object lies in the constellation of Hydra and is designated J0909+0002 in short. Link to source 🔗
Image credit: NAOJ
2025-01-15 Exoplanets
Using the James Webb Space Telescope, astronomers scanned the atmosphere of the planet GJ1214 b located 48 light-years away in Ophiuchus. Instead of a hydrogen rich super-Earth, or a water world, the new data, in spite of many uncertainties, revealed concentrations of carbon-dioxide (CO2) comparable to the levels found in the dense CO2 atmosphere of Venus. Link to source 🔗
Backlog
No, we are not on Facebook but proudly on AstroBin with Mille Gracie to the author Salvatore Iovene:
If anybody is interested in the night life of bats, here is a funny 1-minute MP4 video (24MB).
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Constellation | Canes Venatici |
Distance | 73.48 parsec |
Magnitude | 12.41 vis. |
Mass | 0.64 xSun |
Radius | 0.62 xSun |
Temperature | 4034°K |
Known planet(s) | 1 |
Merak (48 Bet UMa) in UMa [HIP 53910]
Distance: 79 light-years, Magnitude: 2.34
Designated BETA in the constellation Ursa Major, Merak is one of the stars forming the Big Dipper. A line connecting Merak with Dubhe (ALPHA) extends to the Northern Pole Star.
Star Chart | DSS IR Image 🔗279 G. Sagittarii (GJ 783 A ) in Microscopium
Distance: 20 light-years, Magnitude: 5.3
Gliese 783 (279 G. Sagittarii) is a binary star system which is approaching the sun at a velocity of about 129 km/s. At this rate, it will be 6.7 light years away in 41,100 years, and ten times brighter than now. The A-B pair's masses are 65%/24% solar and measure 66%/28% the radius of the sun. The two stars are separated by a semi-major axis of 56.3 AUs.
Star Chart | DSS IR Image 🔗
M36 (Open Cluster) in Auriga
Magnitude: 6
Located a little more than 4000 light years away, this group of about 60 stars spans about 14 light-years. One star in kit seems brighter than the rest. It is a spectral type B2 and about 360 more luminous than our Sun. Some 25 million years old, M36 shares a lot in common with another nearby star cluster, the Pleiades.
Star Chart | DSS IR Image 🔗Cygnus (northern), area rank: 16
Delegating summer, Cygnus is also called the "Northern Cross", owing to its cross-like shape. At the tail of the "swan" shines the 1st-magnitude star Deneb. The binary star Albireo shines beautifully in yellow and blue at the nib. Cygnus is home to the majority of confirmed Kepler planets and the popular 'North America' nebula (NGC 7000).
Star Chart45P/Honda-Mrkos-Pajdusakova
Discovered on December 3, 1948, 45P/Honda-Mrkos-Pajdusakova is a short-period comet on an elliptical orbit with a period of 5.26 years. Its nucleus is estimated to be 0.5-1.6 kilometers in diameter. The comet made a close approach of only 0.06 AU (8,980,000 km) from the Earth on August 15, 2011.
Myrrha (Asteroid)
Semi-major: 3.21900 AU, Size: 120.58 km
Discovered on Jan 10, 1894 by French astronomer Auguste Charlois, 381 Myrrha is an over 120km wide large C-type main belt asteroid, probably composed of carbonaceous materials and rotating around its axis once in 6.572 hours.
Puck (moon of Uranus)
Discovered in 1985 in Voyager 2 images, Puck is the largest of Uranus' lesser moons. The orbit of Puck lies between the rings of Uranus and the first of Uranus' large moons, Miranda. It has a dark, heavily cratered surface, which shows spectral signs of water ice.
TOI-500 b (in Puppis)
Mass: 0.00447 xJup
Radius: 0.104 xJup
SMA: 0.01189 AU
Period: 0.548177 days
Distance: 47.3924 parsec
Category: Hot Terran
ESI: 0.291816