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Observable comet count is 1199
Current exoplanet count is 5903
Current longitude II of the GRS is 72°
Impact Probablity of 2024 YR4: Insignificant
Asteroid | Size | Probability | Date |
2024 YR4 | 40—90 m | Insignificant | 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
Another First: NASA Webb Identifies Frozen Water in Young Star System
May 14, 2025
An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at the top and at right. There’s a huge cavity between the star and the disk. The label Artist's Concept appears at lower left.
Source: stsci.edu/news
14 May 2025
A science team has combined data from the NASA/ESA/CSA James Webb Space Telescope and the Keck II telescope to see evidence of cloud convection on Saturn’s moon Titan in the northern hemisphere for the first time. Most of Titan’s lakes and seas are located in that hemisphere, and are likely replenished by an occasional rain of methane and ethane. Webb also has detected a key carbon-containing molecule that gives insight into the chemical processes in Titan’s complex atmosphere.
Source: esawebb.org
29 April 2025
This new Picture of the Month from the NASA/ESA/CSA James Webb Space Telescope features an astounding number of galaxies. The objects in this frame span an incredible range of distances, from stars within our own Milky Way, marked by diffraction spikes, to galaxies billions of light-years away. The star of this field is a group of galaxies, the largest concentration of which can be found just below the centre of this image. These galaxies glow with white-gold light. We see this galaxy group as it appeared when the Universe was 6.5 billion years old, a little less than half the Universe’s current age. The image on the left combines infrared data from both Webb and the NASA/ESA Hubble Space Telescope, showcasing the galaxy cluster against a backdrop of thousands of other galaxies. The image on the right adds X-ray data from ESA’s XMM-Newton space observatory and NASA’s Chandra X-ray Observatory …
Source: esawebb.org
Dr. Nancy Grace Roman, NASA's first Chief of Astronomy, briefs Astronaut Edwin "Buzz" Aldrin on celestial objects in 1965 in Washington, D.C.
Click to enlarge or show full screenFri, 16 May 2025 18:19 GMT
Source: www.nasa.gov
Image credit: Grok (modified with red star)
2025-04-18 Exoplanets
Thanks to NASA's JWST, astronomers have detected signatures of life on the exoplanet K2-18b, 124 light-years away in Leo, which is 2.6 times larger and 8.6 times more massive than the Earth. The planet's atmosphere contains dimethyl sulfide (DMS), naturally produced by living organisms. Already in September 2023 NASA reported that the JWST has revealed the presence of carbon-bearing molecules including methane and carbon dioxide. Link to source 🔗
Image credit: NASA, ESA, CSA, STScI, W. Balmer (JHU), L. Pueyo (STScI), M. Perrin (STScI)
2025-03-18 Exoplanets
HR 8799 is a young star with 1.5 solar masses, about 130 light-years away in Pegasus and known to have four giant gas planets rich in carbon dioxide gas. NASA’s James Webb Space Telescope took a spectrum and imaged the four planets while the light of the star has been blocked. Link to source 🔗
Image credit: International Gemini Observatory/NOIRLab/NSF/AURA/R. Proctor/J. Pollard
2025-03-14 Exoplanets
Next to the Alpha Centauri system, Barnard's star is the second nearest at 5.96 light-years away in Ophiuchus. As of March 2025, the red dwarf star, only 0.16 as massive as the sun, is home to four known (confirmed) planets each of them less than half the mass of Earth and none of them orbiting inside the habitable zone. Only between 2.8 and 4.1 million kilometers away from the star on 2.34 to 6.74 days orbits, their surfaces are supposed to be heat scorched with no outlook for life. Link to source 🔗
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 | Pictor |
Distance | 69.60 parsec |
Magnitude | 9.36 vis. |
Mass | 0.94 xSun |
Radius | 0.897 xSun |
Temperature | 5666°K |
Known planet(s) | 2 |
Pollux (78 Bet Gem) in Gem [HIP 37826]
Distance: 34 light-years, Magnitude: 1.16
Pollux, an orange giant star in Gemini, one of the heavenly twin stars, is believed to have a planet of 2.3 Jupiter masses in 1.65AU distance orbiting once in 590 days.
Star Chart | DSS IR Image 🔗GJ 35 (van Maanen's Star) in Pisces
Distance: 14 light-years, Magnitude: 12.4
Discovered in 1917 by the Dutch Adriaan van Maanen, Van Maanen's star is metal-rich white dwarf 0.633 times the mass and 1.3 percent the size of the Sun. The star moves at a rate of 2.98 arcseconds per year across the sky.
Star Chart | DSS IR Image 🔗
M15 (Globular Cluster) in Pegasus
Magnitude: 6.2
M15 is probably the most dense globular cluster in our entire Milky Way galaxy. This ball of stars measures about 210 light-years across, yet more than half of the stars you see are packed into the central area in a space just slightly more than 10 light-years in size.
Star Chart | DSS IR Image 🔗Antlia (southern), area rank: 62
Located opposite of Crater with Hydra in between, this constellation is merely made of 4th and 5th-magnitude stars which are difficult to glimpse in cities because of its low elevation in the south. Antlia is derived from vacuum pumps used in the 18th century for scientific experiments.
Star Chart9P/Tempel 1
Discovered in 1867, short-periodic 9P/Tempel 1 has a 7.6 km wide nucleus and orbits the sun once in 5.52 years. Due to its current aphelion distance of 4.7 AU, comet Tempel's orbit changes under gravitaional pulls by Jupiter and the inner planets. The last major change occurred in 1881, when Jupiter stretched Tempel's period to 6.5 years. On July 4, 2005, NASA's Deep Impact probe deliberately dropped an impactor which left a 150 meters wide and 30 meters deep crater on Tempel's surface. On February 15, 2011, NASA's Stardust probe passed the comet at 181km distance and imaged the crater.
Bennu (Asteroid)
Semi-major: 1.12888 AU, Size: 0.545 km
Discovered in 1999 by the LINEAR research, 101955 Bennu is an over 500 meters wide NEO/Apollo Asteroid and a planned target of NASA's OSIRIS-REx mission (launched in 2016) which is expected to return samples from the surface in 2023. Although its composition is unknown, the carbon-rich asteroid is most probably made up of materials present when the solar system formed. Bennu orbits once in 1.2 years in an average distance of 1.13AU between Venus and Mars, just like Earth inside the sun's habitable zone where the asteroid's surface is heated up to over 90°C. Bennu rotates retrograde in 4.3 hours with a spin vector between -70 and -90° ecliptic latitude. The rotation period suggests that it has not been greatly spun up by tidal or radiation forces.
Bianca (moon of Uranus)
Discovered in 1986 in Voyager 2 images, Bianca's surface probably consists of the dark, unprocessed, carbon-rich material found on the C-class of asteroids. Else not much is known about this moon of Uranus.
OGLE-2013-BLG-1761L b (in Sagittarius)
Mass: 2.7 xJup
SMA: 1.8 AU
Distance: 6900 parsec
Category: Jovian
ESI: 0