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Observable comet count is 1178
Current exoplanet count is 5806
Current longitude II of the GRS is 62°
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
"> NASA's Webb Finds Planet-Forming Disks Lived Longer in Early Universe
December 16, 2024
Twisted pink and orange filaments lie against a black background speckled with white and pink stars. Five small, yellow circles overlaid on the left side of the image and one small, yellow circle at the top right corner indicate the positions of six of the ten stars surveyed in this study.
Source: stsci.edu/news
16 December 2024
The NASA/ESA/CSA James Webb Space Telescope just solved a conundrum by proving a controversial finding made with the NASA/ESA Hubble Space Telescope more than 20 years ago.
Source: esawebb.org
18 December 2024
The galaxy filling the frame in this NASA/ESA/CSA James Webb Space Telescope Picture of the Month is NGC 2566, a spiral galaxy located in the constellation Puppis. The image combines observations from two of Webb’s instruments, the Near-InfraRed Camera (NIRCam) and Mid-InfraRed Instrument (MIRI), to show off NGC 2566’s well-defined spiral arms, long central bar and delicate tracery of gas, dust and stars. At 76 million light-years away, NGC 2566 is considered a nearby galaxy, making it an excellent target for studying fine details like star clusters and gas clouds. The new Webb images of NGC 2566 were collected as part of an observing programme (#3707) dedicated to understanding the connections between stars, gas and dust in nearby star-forming galaxies. NGC 2566 is just one of the 55 galaxies in the local Universe examined by Webb for this programme. The mid-infrared wavelengths captured by MIRI highlight NGC 2566’s warm interstellar …
Source: esawebb.org
During the morning of March 20, 2015, a total solar eclipse was visible from parts of Europe, and a partial solar eclipse from northern Africa and northern Asia. NASA's Terra satellite passed over the Arctic Ocean on March 20 at 10:45 UTC (6:45 a.m. EDT) and captured the eclipse's shadow over the clouds in the Arctic Ocean.
Click to enlarge or show full screenFri, 20 Dec 2024 19:34 GMT
Source: www.nasa.gov
Image credit: NASA/Goddard/University of Arizona/Lockheed Martin
2024-10-07 solar system
Just for info, no danger posed. This year, NEO asteroid 2024 TR4, estimated 14 meters across flew past Earth on October 7 at 01:07 UTC at a distance of approximately 112,000 km at a speed of 15 km/sec. The distance equals to 0.3 lunar distances which is a very close encounter (the image shows asteroid Bennu). Link to source 🔗
Image credit: ESO/M. Kornmesser
2024-10-05 Exoplanets
High proper motion, single star, Barnard's Star is only about 6 light-years away in Ophiuchus. Using ESO's VLT astronomers have detected a rocky planet orbiting at a distance 20 times closer than Mercury is to the sun resulting in a short 3.15 days orbit and a scorching 125°C surface temperature. Link to source 🔗
Image credit: NASA/JPL
2024-03-15 solar system
According to NASA, on April 13, 2029, Apophis will pass less than 20,000 miles (32,000 kilometers) from Earth's surface, closer than the distance of geosynchronous satellites. Although previously dubbed the Doomsday Asteroid, about 340 meters wide Apophis does not pose any danger of impact during close approach in 2029 as it will be visible with the unaided eye. Link to source 🔗
Image credit: NASA/LRO/LROC/ASU/Smithsonian Institution
2024-01-27 solar system
Moon is shrinking and torn by tidal forces from Earth. Evidence for seismic activity has been detected near candidate regions for the Artemis III mission scheduled for a crewed lunar landing. Such quakes can produce ground shaking strong enough for faults to slide or for piling up new thrust faults. The LROC image shows a cluster of lobate scarps (left pointing arrows) near the lunar south pole. A thrust fault scarp cut across an approximately 1-km diameter degraded crater (right pointing arrow). Link to source 🔗
Image credit: NASA/Goddard/Arizona State University
2024-01-27 solar system
NASA’s Lunar Reconnaissance Orbiter captured this image of the JAXA SLIM lander on the Moon’s surface on Jan. 24, 2024. SLIM landed at -13.316° south latitude, +25.2510° east longitude, at an elevation of minus 912 meters. The image is 880 meters wide and lunar north is up. Link to source 🔗
Image credit: NASA, ESA, Leah Hustak (STScI), Ralf Crawford (STScI)
2024-01-26 Exoplanets
Discovered in 2017, the Superterran planet GJ 9827 d is located some 97 light-years away in Pisces and may have a water-rich atmosphere in spite of being hotter than Venus because it orbits extremely close to it host star alongside two further known inner planets. Astronomers will further investigate with the help of the Hubble and James Webb space telescopes. Link to source 🔗
Image credit: JAXA/タカラトミー/ソニーグループ(株)/ 同志社大学)
2024-01-25 solar system
JAXAs lunar lander SLIM has been photographed by its small rover, the Lunar Excursion Vehicle 2 (LEV-2). The soft landing about 55 meters east of target point was completed at 1.4m/sec surpassing specifications. Though the solar panels were supposed to face upwards after landing, on the photo SLIM is shown with its main engine facing upwards, but JAXA hopes it will gather sunlight and restore power until local sunset on Feb 1st. Analysis so far has also revealed that one of the two main engines was lost due to some abnormality at an altitude of 50 meters just before landing. Both exploration rover robots are in good working condition. SLIM landed on the moon at 15:20 on January 19 UTC. Link to source 🔗
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If anybody is interested in the night life of bats, here is a funny 1-minute MP4 video (24MB).
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Constellation | Taurus |
Distance | 159.24 parsec |
Magnitude | 15.64 vis. |
Mass | 0.7 xSun |
Radius | 1.45 xSun |
Temperature | 4080°K |
Known planet(s) | 1 |
Menkent (5 The Cen) in Cen [HIP 68933]
Distance: 61 light-years, Magnitude: 2.06
Alpha Ceti, or Menkar (Arabic for nose of the whale), or Menkab is a red giant expanding to 90 times the Sun's size. Having exhausted its helium, the star is now burning its carbon core, while becoming highly unstable. In its next phase, Menkar will shed its outer layers forming a planetary nebula, leaving a large white dwarf remnant.
Star Chart | DSS IR Image 🔗GJ 411 (Lalande 21185) in Ursa Major
Distance: 8 light-years, Magnitude: 7.4
Lalande 21185 is a type-M red dwarf main sequence star with about 46% solar masses and 3383°K cool, emitting most of its energy as infrared radiation. The proportion of elements other than hydrogen and helium is estimated based on the ratio of iron to hydrogen in the star when compared to the Sun, indicating that the proportion of iron is about 63% of the Sun. Lalande 21185 is also listed as a BY Draconis type variable star in the General Catalogue of Variable Stars, designated NSV 18593.
Star Chart | DSS IR Image 🔗
M75 (Globular Cluster) in Sagittarius
Magnitude: 8.5
M75 is one of the most remote of of all globular clusters, positioned 67,500 light-years beyond the Milky Way's galactic center. Spanning 180 light-years across, it blazes with the brightness of 180,000 suns.
Star Chart | DSS IR Image 🔗Ursa Major (northern), area rank: 3
Characterized by the seven stars that form the Big Dipper. Taking this for the tail and connecting a number of faint stars below, the constellation of the "bear" becomes apparent. Five of the Big Dipper stars are actually near each other in space and were likely formed at nearly the same time. Connecting two stars in the far part of the Big Dipper (Merak and Dubhe) will lead one to Polaris, the North Star, which is part of the Little Dipper. Relative stellar motions will cause the Big Dipper to slowly change its apparent configuration over the next 100,000 years. Likewise well known is the binary pair Mizar and Alcor.
Star Chart103P/Hartley 2 (2010)
Comet Hartley 2 is a small periodic comet with an orbital period of 6.47 years. It was discovered by Malcolm Hartley in 1986 at the Schmidt Telescope Unit, Siding Spring Observatory, Australia. Its diameter is estimated to be 1.2 to 1.6 km while its mass is estimated to be about 300 megatons. The comet was the target of a flyby of the Deep Impact spacecraft, as part of the EPOXI mission, on 4 November 2010, which was able to approach within 700 km as part of its extended mission. As of November 2010 Hartley 2 is the smallest comet which has been visited.
Ikufumi (Asteroid)
Semi-major: 2.30240 AU, Size: 0 km
Discovered 1990 Sept. 27 by T. Urata at the Nihondaira Observatory. Named in honor of Ikufumi Makino (born 1944), a telecommunications systems engineer and active amateur astronomer. His extensive knowledge of computer technologies has enabled him to contribute to astronomical magazines many articles about systems for making observations. He has played an important role in introducing and spreading the data-reduction tool Astrometrica in Japan. He is a collaborating member of the Nihondaira Observatory.
Methone (moon of Saturn)
Discovered in 2004, Methone, orbiting between Mimas and Enceladus. is an egg-shaped moonlet with a remarkably smooth surface and no visible craters.
GJ 682 b (in Scorpius)
Mass: 0.01384 xJup
SMA: 0.08 AU
Period: 17.478 days
Distance: 5.00671 parsec
Category: Warm Superterran
ESI: 0.567606