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Observable comet count is 1957
Current exoplanet count is 6354
Current longitude II of the GRS is 90°
Today Monitor
Mars: January 16, 2025
Jupiter: January 10, 2026
Saturn: September 21, 2025
Uranus: November 21, 2025
Neptune: September 23, 2025
Evening: August 15, 2026 at 45.9°E
Morning: January 3, 2027 at 47.0°W
Morning: December 7, 2025 at 20.7°W
Evening: February 19, 2026 at 18.1°E
Morning: April 3, 2026 at 27.8°W
Evening: June 15, 2026 at 24.5°E
Morning: August 2, 2026 at 19.5°W
Evening: October 12, 2026 at 25.2°E
Morning: November 20, 2026 at 19.6°W
January 3: 225,130 mi (362,312 km)
November 24: 224,170 mi (360,768 km)
December 24: 221,667 mi (356,740 km)
given for 00:00 UT
| Date | Size | Age | Angle | Phase |
|---|---|---|---|---|
| 13 Apr 2026 | 30.89' | 24.94 | -6.797° | ![]() |
| 14 Apr 2026 | 31.37' | 25.94 | -6.885° | ![]() |
| 15 Apr 2026 | 31.85' | 26.94 | -6.540° | ![]() |
| 10 May 2026 | 30.42' | 22.51 | -7.002° | ![]() |
| 11 May 2026 | 30.85' | 23.51 | -7.546° | ![]() |
| 12 May 2026 | 31.34' | 24.51 | -7.695° | ![]() |
| 13 May 2026 | 31.86' | 25.51 | -7.381° | ![]() |
| 14 May 2026 | 32.37' | 26.51 | -6.565° | ![]() |
| 22 May 2026 | 32.03' | 5.17 | 6.635° | ![]() |
| 23 May 2026 | 31.56' | 6.17 | 7.101° | ![]() |
| 24 May 2026 | 31.11' | 7.17 | 7.159° | ![]() |
| 25 May 2026 | 30.71' | 8.17 | 6.868° | ![]() |
| 07 Jun 2026 | 30.39' | 21.17 | -7.053° | ![]() |
| 08 Jun 2026 | 30.79' | 22.17 | -7.626° | ![]() |
| 09 Jun 2026 | 31.25' | 23.17 | -7.834° | ![]() |
| 10 Jun 2026 | 31.75' | 24.17 | -7.603° | ![]() |
| 11 Jun 2026 | 32.25' | 25.17 | -6.885° | ![]() |
| 19 Jun 2026 | 32.20' | 3.88 | 6.768° | ![]() |
| 20 Jun 2026 | 31.68' | 4.88 | 7.364° | ![]() |
| 21 Jun 2026 | 31.18' | 5.88 | 7.508° | ![]() |
| 22 Jun 2026 | 30.71' | 6.88 | 7.253° | ![]() |
| 23 Jun 2026 | 30.31' | 7.88 | 6.670° | ![]() |
| 05 Jul 2026 | 30.48' | 19.88 | -6.530° | ![]() |
| 06 Jul 2026 | 30.82' | 20.88 | -7.017° | ![]() |
| 07 Jul 2026 | 31.21' | 21.88 | -7.189° | ![]() |
| 08 Jul 2026 | 31.64' | 22.88 | -6.986° | ![]() |
| 18 Jul 2026 | 31.76' | 3.60 | 6.894° | ![]() |
| 19 Jul 2026 | 31.25' | 4.60 | 7.142° | ![]() |
| 20 Jul 2026 | 30.77' | 5.60 | 6.982° | ![]() |
| 21 Jul 2026 | 30.35' | 6.60 | 6.469° | ![]() |
| 19 Nov 2026 | 30.64' | 9.71 | -6.939° | ![]() |
| 20 Nov 2026 | 31.11' | 10.71 | -7.238° | ![]() |
| 21 Nov 2026 | 31.62' | 11.71 | -7.063° | ![]() |
| 01 Dec 2026 | 31.73' | 21.71 | 6.670° | ![]() |
| 02 Dec 2026 | 31.32' | 22.71 | 6.898° | ![]() |
| 03 Dec 2026 | 30.93' | 23.71 | 6.823° | ![]() |
| 04 Dec 2026 | 30.59' | 24.71 | 6.497° | ![]() |
| 16 Dec 2026 | 30.14' | 6.96 | -6.743° | ![]() |
| 17 Dec 2026 | 30.53' | 7.96 | -7.511° | ![]() |
| 18 Dec 2026 | 30.98' | 8.96 | -7.903° | ![]() |
| 19 Dec 2026 | 31.49' | 9.96 | -7.840° | ![]() |
| 20 Dec 2026 | 32.03' | 10.96 | -7.269° | ![]() |
| 29 Dec 2026 | 31.92' | 19.96 | 7.182° | ![]() |
| 30 Dec 2026 | 31.41' | 20.96 | 7.556° | ![]() |
| 31 Dec 2026 | 30.94' | 21.96 | 7.540° | ![]() |
| Date | Size | Age | Angle | Phase |
|---|---|---|---|---|
| 06 Apr 2026 | 29.57' | 17.94 | 6.680° | ![]() |
| 07 Apr 2026 | 29.51' | 18.94 | 6.724° | ![]() |
| 08 Apr 2026 | 29.52' | 19.94 | 6.480° | ![]() |
| 20 Apr 2026 | 33.00' | 2.51 | -6.607° | ![]() |
| 21 Apr 2026 | 32.84' | 3.51 | -6.460° | ![]() |
| 03 May 2026 | 29.54' | 15.51 | 6.518° | ![]() |
| 04 May 2026 | 29.46' | 16.51 | 6.605° | ![]() |
| 05 May 2026 | 29.44' | 17.51 | 6.405° | ![]() |
| 17 May 2026 | 33.33' | 0.17 | -6.476° | ![]() |
| 18 May 2026 | 33.34' | 1.17 | -6.448° | ![]() |
| 30 May 2026 | 29.51' | 13.17 | 6.463° | ![]() |
| 31 May 2026 | 29.43' | 14.17 | 6.568° | ![]() |
| 13 Jun 2026 | 33.11' | 27.17 | -6.427° | ![]() |
| 14 Jun 2026 | 33.36' | 28.17 | -6.531° | ![]() |
| 26 Jun 2026 | 29.56' | 10.88 | 6.527° | ![]() |
| 27 Jun 2026 | 29.45' | 11.88 | 6.652° | ![]() |
| 28 Jun 2026 | 29.41' | 12.88 | 6.490° | ![]() |
| 10 Jul 2026 | 32.49' | 24.88 | -6.447° | ![]() |
| 11 Jul 2026 | 32.86' | 25.88 | -6.669° | ![]() |
| 12 Jul 2026 | 33.13' | 26.88 | -6.449° | ![]() |
| 23 Jul 2026 | 29.74' | 8.60 | 6.610° | ![]() |
| 24 Jul 2026 | 29.56' | 9.60 | 6.784° | ![]() |
| 25 Jul 2026 | 29.47' | 10.60 | 6.664° | ![]() |
| 06 Aug 2026 | 31.97' | 22.60 | -6.454° | ![]() |
| 07 Aug 2026 | 32.28' | 23.60 | -6.764° | ![]() |
| 08 Aug 2026 | 32.55' | 24.60 | -6.663° | ![]() |
| 19 Aug 2026 | 30.03' | 6.27 | 6.582° | ![]() |
| 20 Aug 2026 | 29.77' | 7.27 | 6.838° | ![]() |
| 21 Aug 2026 | 29.60' | 8.27 | 6.792° | ![]() |
| 22 Aug 2026 | 29.52' | 9.27 | 6.456° | ![]() |
| 03 Sep 2026 | 32.04' | 21.27 | -6.743° | ![]() |
| 04 Sep 2026 | 32.20' | 22.27 | -6.729° | ![]() |
| 16 Sep 2026 | 30.00' | 4.86 | 6.742° | ![]() |
| 17 Sep 2026 | 29.76' | 5.86 | 6.785° | ![]() |
| 18 Sep 2026 | 29.61' | 6.86 | 6.531° | ![]() |
| 30 Sep 2026 | 32.24' | 18.86 | -6.599° | ![]() |
| 01 Oct 2026 | 32.32' | 19.86 | -6.660° | ![]() |
| 13 Oct 2026 | 30.13' | 2.34 | 6.547° | ![]() |
| 14 Oct 2026 | 29.88' | 3.34 | 6.667° | ![]() |
| 15 Oct 2026 | 29.68' | 4.34 | 6.483° | ![]() |
| 27 Oct 2026 | 32.60' | 16.34 | -6.403° | ![]() |
| 28 Oct 2026 | 32.75' | 17.34 | -6.553° | ![]() |
| 09 Nov 2026 | 30.10' | 29.34 | 6.404° | ![]() |
| 10 Nov 2026 | 29.88' | 0.71 | 6.566° | ![]() |
| 11 Nov 2026 | 29.70' | 1.71 | 6.425° | ![]() |
| 24 Nov 2026 | 32.95' | 14.71 | -6.524° | ![]() |
| 06 Dec 2026 | 30.03' | 26.71 | 6.414° | ![]() |
| 07 Dec 2026 | 29.82' | 27.71 | 6.594° | ![]() |
| 08 Dec 2026 | 29.65' | 28.71 | 6.474° | ![]() |
| 21 Dec 2026 | 32.55' | 11.96 | -6.593° | ![]() |
| 22 Dec 2026 | 32.99' | 12.96 | -6.555° | ![]() |
Source: NASA/GSFC
Source: apod.nasa.gov
Mirror: star.ucl.ac.uk
STScI Scientists Part of Collaboration Receiving 2027 Berkeley Prize

September 17, 2026
A crowded galaxy field on a black background, with one large star dominating the image just right of center. Three areas are concentrated with larger white hazy blobs on the left, lower right, and upper right above the single star. Scattered between these areas are many smaller sources of light; some also have a hazy white glow, while many other are red or orange. Even without zooming in, different galaxy shapes are detectable, like spirals, ovals, and arcs.
Source: stsci.edu/news
15 September 2026
This starry view of the nearby star-forming region IC 348 is one of the largest images from the NASA/ESA/CSA James Webb Space Telescope released to the public so far. Using Webb, astronomers searched IC 348 for brown dwarfs, which are less massive than the smallest stars. The researchers discovered brown dwarfs just twice the mass of Jupiter, bringing the study of these curious objects into a new mass range.
Source: esawebb.org
27 August 2026
The latest ESA/Webb Picture of the Month is a new, infrared look into the strange final phase of a galactic merger. Arp 263, an irregular galaxy, lies in the constellation Leo at a relatively nearby distance of around 25 million light-years. Originally discovered in 1784 and also catalogued as NGC 3239, this galaxy was included in American astronomer Halton Arp’s Atlas of Peculiar Galaxies in 1966, as possibly one of the most remarkable and strange galaxies in the sample. Arp categorised it with the galaxies featuring “irregular clumps”. In 2023, the galaxy was featured in an image from the NASA/ESA Hubble Space Telescope, where these clumps are revealed to be bright nebulae between the galaxy’s dense clouds of gas, where stars are forming. Arp 263 is believed to result from a past galactic merger. Apart from its unusual distorted shape, astronomers have noticed a few features that point to this. …
Source: esawebb.org
Using NASA’s Chandra X-ray Observatory, scientists have discovered a new class of objects behaving unlike any they have seen before.
Click to enlarge or show full screenTue, 22 Sep 2026 15:44 GMT
Source: www.nasa.gov
Image/illustration credit: NASA/JPL-Caltech/ASU
2026-03-13 Exoplanets
On Feb 6, 2026, NASAs SPARCS Mission returned first images of an exoplanet, HD 71262, in both, near-UV and far-UV. SPARCS' mission is for monitoring flares and sunspot activity on low-mass stars about 30% to 70% the mass of the Sun which are likely to host rocky planets inside their habitable zones. Link to source 🔗
Image/illustration credit: astropical.space
2026-02-08 solar system
AR4366 stands out as the most active sunspot of early 2026, producing an extraordinary sequence of high‑energy flares and posing meaningful space‑weather risks as it faces Earth. Its behavior is characteristic of a highly unstable, rapidly evolving magnetic system capable of generating the strongest solar eruptions of the cycle. Ø71mm APO, IMX178 camera.
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).
Now on YouTube
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| Constellation | Draco |
| Distance | 6.84 parsec (22.32ly) |
| Magnitude | 9.70 vis. |
| Mass | 0.25 xSun |
| Radius | 0.28 xSun |
| Temperature | 3379°K |
| Known planet(s) | 1 |
Daytime Sextantids
9 Sep - 9 Oct, Peak: 9/27
Radiant: Star Chart, Rating: bright
Deneb el Okab (17 Zet Aql) in Aql [HIP 93747]
Distance: 83 light-years, Magnitude: 2.99
Deneb el Okab, Arabic for 'the tail of the falcon' is the primary of a system of three stars. It is 2.4x more massive, 2.3x larger and 40 times more luminous than the sun. The star is no older than 150 million years and is rotating at 317 km/s stretching its equatorial radius over 30.7% greater than its polar radius.
Star Chart | DSS IR Image 🔗GJ 169.1 A (Stein 2051) in Camelopadalis
Distance: 18 light-years, Magnitude: 11
Stein 2051 (Gliese 169.1, G 175-034, LHS 26/27) is a nearby binary star system, containing a red dwarf (component A) and a degenerated star, a white dwarf (component B), located in the constellation of Camelopardalis at about 18 light-years away. Stein 2051 B is the 6th nearest white dwarf after Sirius B, Procyon B, van Maanen's star, LP 145-141 and 40 Eridani B.
Star Chart | DSS IR Image 🔗

M66 (Galaxy) in Leo
Magnitude: 9.7
M66 is an intermediate spiral galaxy, 95000 light-years across with striking dust lanes and bright star clusters along sweeping spiral arms. M66 is part of the famous Leo Triplet, a small group of galaxies that also includes M65 and NGC 3628.
Star Chart | DSS IR Image 🔗Bootes (northern), area rank: 13

Marked by the 1st-magnitude star Arcturus, this constellation resembles the shape of a necktie. Arcturus is found in the northern spring sky by drawing a curve southwards from the leftmost star of the handle of the Big Dipper.
Star Chart153P/Ikeya-Zhang

Discovered in 2002, 153P/Ikeya-Zhang is a long-periodic comet with the longest known period (366.5 years) for returning comets. On March 18, 2002, the comet last passed perihelion and became the brightest comet since 1997 shining at 3.5 magnitudes. The comets aphelion distance is at over 100 AU away through the Kuiper Belt reaching into the innermost section of the Oort Cloud.
Flora (Asteroid)
Semi-major: 2.20122 AU, Size: 136 km

Discovered on October 18, 1847 by J. R. Hind , 8 Flora is a bright S-type main belt asteroid. Flora's spectrum indicates that its surface composition is a mixture of silicate rock (including pyroxene and olivine) and nickel-iron metal. Flora is the innermost known large asteroid, rotates around its axis in 12.8 hours and has a mass of 8.47x1018kg.
Rhea (moon of Saturn)

Discovered in 1672, Rhea is the second largest moon of Saturn, a small, cold, airless body that is very similar to sister moons Dione and Tethys. Rhea is three quarters ice and one quarter rock. Models suggest that Rhea could be capable of sustaining an internal liquid water ocean through heating by radioactive decay.
BD-10 3166 b (in Crater)
Mass: 0.59 xJup
SMA: 0.04 AU
Period: 3.48777 days
Distance: 84.4069 parsec
Category: Hot Jovian
ESI: 0.07