The Pleiades, M45
The Pleiades star cluster is also known as the Seven Sisters, and as Messier 45. It is a prominent object in the night sky with a conspicuous place in ancient mythology. The cluster is among the nearest to Earth, and the most obvious to the naked eye. Although only a handful are visible to the unaided eye, it contains hundreds of stars, some of them surrounded by swirls of nebulosity.
The Great Orion Nebula, M42
The Orion Nebula, catalogued as Messier 42 or NGC 1976, is one of the brightest nebulae in the sky, and one of the nearest star-forming regions to Earth. It is rewarding in telescopes of every size, and is perhaps the most studied and photographed object in the sky. M 42 is visible to the naked eye as a hazy patch surrounding Theta Orionis, the middle star in the Sword of Orion, just south of Orion's Belt.
The Moon
The Earth's companion in its orbit around the Sun is the Moon. The Moon orbits the Earth at an average distance of about 240,000 miles (384,000 km) over a period of about 29.5 days. Its monthly cycle of phases provided a natural clock for ancient societies; most human calendar systems are built around, or least contain units based on, the orbital period of the Moon. To this date, the Moon is the only object in the solar system other than the Earth that has been visited by humans.
M81
Messier 81 (NGC 3031) in Ursa Major is one of the most conspicuous spiral galaxies in the sky. It forms a physical pair with its neighbor, M 82, and is the dominant galaxy of the M81 group. Discovered along with M 82 by Johann Bode, and sometimes referred to as Bode's Nebula, M 81 is one of the easiest and most rewarding galaxies for amateur astronomers in the northern hemisphere.
M82
Messier 82 (NGC 3034) is a remarkable, peculiar galaxy in Ursa Major. M 82 was discovered along with its partner M 81 by Johann Bode, and both galaxies are sometimes known as Bode's Nebulae. Also called the Cigar Galaxy, M 82 has been spectacularly disturbed by a relatively recent encounter with M 81, and displays conspicuous dust lanes and heavy star formation. M 82 is the prototype irregular starburst disk galaxy.
Jupiter
Jupiter is the largest planet in the solar system, and by far the most massive. It contains over twice as much matter as all of the other planets combined. Jupiter is a very different planet from the Earth, or any of the other inner planets. It is composed mostly of liquid and gaseous hydrogen, and has no solid surface. For this reason, Jupiter is the first of the "gas giant" planets
Uranus
Uranus is the seventh planet from the Sun, and was the first to have been discovered in recorded history. It is unique because its rotational axis is radically tilted towards its orbital plane, and its moons also have orbits that are tilted with respect to Uranus's orbital plane.
Comet 12P/Pons-Brooks
12P/Pons-Brooks is a periodic comet discovered on July 12, 1812 by Jean-Louis Pons. It was later found independently by Vincent Wisniewski and Alexis Bouvard in August of the same year. Shortly after its initial discovery, Johann Franz Encke determined a definitive orbit for the comet, with a period of 70.68 years. This orbit was used to generate an ephemeris for the 1883 return. But searches were unsuccessful until the comet was accidentally rediscovered by William Robert Brooks on September 2nd, 1883, and later identified as the same object.
Pons-Brooks fits the classical definition of a Halley-type comet, with an orbital period between 20 and 200 years. With a steep orbital inclination of 74.2°, this comet does not spend a lot of time near the ecliptic, where it is easiest to interact with other bodies. The comet's orbit appears to be stable between 1740 and 2167, with no strong perturbations by any of the planets. It will next appear in 2024.
In 2011, Mexican astronomers suggested that this comet may have split into several pieces around 1883, and that Earth barely avoided multiple Tunguska events or even a mass extinction. On August 12-13, 1883, Mexican astronomer Jose Bonilla observed 447 bodies with a "bright mistiness" cross the solar disc from an observatory in Zacatecas. These objects were estimated to have had a size between 46 and 1022 meters, and to have passed only 538 to 8062 km from the Earth. The source of these objects could also have been comet C/1883 D1 (Brooks-Swift), or another unknown comet. The event also coincided with the annual Perseid meteor shower; even migrating birds cannot be ruled out.
September 2nd, 2023
The current Solar activity.
Globular clusters are gravitationally bound concentrations of approximately ten thousand to one million stars, spread over a volume of 30 to about 200 light years in diameter. M 13 is one of the most prominent and best known globular clusters of the northern celestial hemisphere, 165 light years away from Earth. Towards its center, stars are about 500 times more concentrated than in our solar neighborhood. Globular Clusters are among the oldest objects in the Universe, appearing to be formed of light elements more associated with the primordial universe. Scientists do not understand what formed globular clusters or why they survived so long. Image
M 11 is an Open cluster, about 24 light years away from Earth. Open (or galactic) clusters are physically related groups of stars held together by mutual gravitational attraction. They are believed to originate from large cosmic gas and dust clouds in the Milky Way, and to continue to orbit the galaxy throughout the disk. Most open clusters have only a short life as stellar swarms. As they drift along their orbits, some of their members escape the cluster, due to velocity changes in mutual close encounters, tidal forces in the galactic gravitational field, and encounters with field stars and interstellar clouds crossing their way. An average open cluster has spread most of its member stars along its path after several 100 million years; only a few of them have an age counted in billions of years. Most of the individual stars in the sky are thought to original from open clusters. Image
NGC 6826 is commonly referred to as the "Blinking Nebula" or "Blinking Planetary." When a star with an intermediate mass (80% of the Sun, but less than 8 times the Sun’s mass) runs out of sufficient fuel to maintain its equilibrium, it dies and, in the process, swells to form a red giant star. As the star expels gas, its core contracts and temporarily radiates energy again. This energy ionizes the expelled gas causing it to emit light. In the case of NGC-6826, the bright core overwhelms the human eye, preventing one from seeing the surrounding gas (the emission nebula). However, it can be viewed using averted vision, looking next to the central star, which causes it to "blink" in and out of view. Look carefully and you may see the two bright patches on opposite sides of the nebula. The Blinking Nebula is about 2,200 light years away from Earth. Image