C/1890 V1 (Zona)

Last updated

C/1890 V1 (Zona)
Discovery
Discovered by Temistocle Zona
Discovery site Palermo Astronomical Obs.
Discovery date15 November 1890
Designations
1890e
1890 IV
Orbital characteristics [1]
Epoch 7 December 1890 (JD 2411708.5)
Observation arc 6 days
Number of
observations
5
Aphelion 720.331 AU
Perihelion 2.0398 AU
Semi-major axis 361.185 AU
Eccentricity 0.994352
Orbital period 6,864.41 years
Inclination 154.264°
86.891°
Argument of
periapsis
330.879°
Last perihelion6 August 1890
TJupiter –1.579
Earth MOID 1.0892 AU
Jupiter MOID 1.8205 AU

C/1890 V1 (Zona) is a non-periodic comet discovered on November 15, 1890 by the Italian astronomer Temistocle Zona [2] with an equatorially mounted Merz telescope at the Osservatorio Astronomico di Palermo. [3] Whilst attempting to observe this comet, Rudolf F. Spitaler discovered the eponymous 113P/Spitaler in 1890.

Related Research Articles

<span class="mw-page-title-main">32P/Comas Solà</span> Periodic comet with 9 year orbit

32P/Comas Solà is a periodic comet with a current orbital period of 8.8 years.

<span class="mw-page-title-main">Comet West</span> Icy small Solar System body; passed closest to Earth in 1976

Comet West, formally designated C/1975 V1, 1976 VI, and 1975n, was a comet described as one of the brightest objects to pass through the inner Solar System in 1976. It is often described as a "great comet."

<span class="mw-page-title-main">Comet Donati</span> Non-periodic comet

Comet Donati, or Donati's Comet, formally designated C/1858 L1 and 1858 VI, is a long-period comet named after the Italian astronomer Giovanni Battista Donati who first observed it on June 2, 1858. After the Great Comet of 1811, it was the most brilliant comet that appeared in the 19th century. It was also the first comet to be photographed.

<span class="mw-page-title-main">Donald Machholz</span> American amateur astronomer (1952–2022)

Donald Edward Machholz was an American amateur astronomer who was credited with the discovery of 12 comets that bear his name.

<span class="mw-page-title-main">Comet Machholz</span>

Comet Machholz, formally designated C/2004 Q2, is a long-period comet discovered by Donald Machholz on August 27, 2004. It reached naked eye brightness in January 2005. Unusual for such a relatively bright comet, its perihelion was farther from the Sun than the Earth's orbit.

<span class="mw-page-title-main">Great Comet of 1680</span> First comet discovered by telescope

C/1680 V1, also called the Great Comet of 1680, Kirch's Comet, and Newton's Comet, was the first comet discovered by telescope. It was discovered by Gottfried Kirch and was one of the brightest comets of the seventeenth century.

<span class="mw-page-title-main">C/1948 V1</span> Non-periodic comet

The Eclipse Comet of 1948, formally known as C/1948 V1, was an especially bright comet discovered during a solar eclipse on November 1, 1948. Although there have been several comets that have been seen during solar eclipses, the Eclipse Comet of 1948 is perhaps the best-known; it was however, best viewed only from the Southern Hemisphere.

<span class="mw-page-title-main">C/2002 V1 (NEAT)</span> Sungrazing comet

Comet NEAT, formally designated as C/2002 V1, is a non-periodic comet that appeared in November 2002. The comet peaked with an apparent magnitude of approximately –0.5, making it the eighth-brightest comet seen since 1935. It was seen by SOHO in February 2003. At perihelion the comet was only 0.0992 AU (14.84 million km) from the Sun, where it was initially expected to be disintegrated, however reanalysis of its orbit has indicated that it has survived many of its previous perihelia, thus making breakup unlikely.

<span class="mw-page-title-main">113P/Spitaler</span> Periodic comet with 7 year orbit

Comet Spitaler is a periodic comet in the Solar System discovered by Rudolf Ferdinand Spitaler on November 17, 1890, while attempting to observe Comet Zona.

<span class="mw-page-title-main">Rudolf Ferdinand Spitaler</span> Austrian astronomer, geophysicist, meteorologist and climatologist

Rudolf Ferdinand Spitaler was an Austrian astronomer, geophysicist, meteorologist and climatologist.

<span class="mw-page-title-main">Great Comet of 1577</span> Non-periodic comet

The Great Comet of 1577 is a non-periodic comet that passed close to Earth with first observation being possible in Peru on November 1 1577. Final observation was made on January 26, 1578. Tycho Brahe was one the most distinguished observers of this comet, making thousands of precise measurements about it. The observations made by Brahe led him to believe the comet was outside of the orbit of the sun and moon. There were many independent observers of the comet from across the world. Many had different explanations for the comet. Some, such as Sultan Murad III, saw the comet as an evil omen. Others took a scientific approach, like Michael Mästlin who used the comet to fill gaps in Copernicus's model of the universe. It inspired artists, like Jiri Dschitzky, who made an engraving of the comet as it passed over Prague. Currently, using JPL Horizons, it is believed that the comet is 324 AU from the sun.

<span class="mw-page-title-main">332P/Ikeya–Murakami</span>

332P/Ikeya–Murakami is a short-period comet with period of approximately 5.4 years first identified independently by the two Japanese amateur astronomers Kaoru Ikeya and Shigeki Murakami on November 3, 2010. Ikeya identified the comet using a 25-centimeter (10-inch) reflector at 39×, while Murakami used a 46 cm (18-inch) reflector at 78×. Photographic confirmation of the comet was obtained by Ernesto Guido and Giovanni Sostero using a Global-Rent-a-Scope (GRAS) telescope in New Mexico. Both Ikeya and Murakami discovered the comet using manual observation through optical telescopes. Such visual discoveries have become rare in recent years.

<span class="mw-page-title-main">C/2010 X1 (Elenin)</span> Oort cloud comet

Comet C/2010 X1 (Elenin) is an Oort cloud comet discovered by Russian amateur astronomer Leonid Elenin on December 10, 2010, through remote control of the International Scientific Optical Network's robotic observatory near Mayhill in the U.S. state of New Mexico. The discovery was made using the automated asteroids discovery program CoLiTec. At the time of discovery, the comet had an apparent magnitude of 19.5, which made it about 150,000 times fainter than can be seen with the naked eye. The discoverer, Leonid Elenin, originally estimated that the comet nucleus was 3–4 km in diameter, but more recent estimates place the pre-breakup size of the comet at 2 km. Comet Elenin started disintegrating in August 2011, and as of mid-October 2011 was not visible even using large ground-based telescopes.

Leonid Vladimirovich Elenin is a Russian amateur astronomer working with the ISON-NM observatory (H15) via the International Scientific Optical Network (ISON), which is the first Russian remote observatory in the West.

In observational astronomy, the observation arc of a Solar System body is the time period between its earliest and latest observations, used for tracing the body's path. It is usually given in days or years. The term is mostly used in the discovery and tracking of asteroids and comets. Arc length has the greatest influence on the accuracy of an orbit. The number, spacing of intermediate observations, and timestamps have a lesser effect.

Temistocle Zona was an Italian astronomer.

<span class="mw-page-title-main">273P/Pons–Gambart</span>

273P/Pons–Gambart, also called Comet Pons-Gambart, is a periodic comet in a retrograde orbit first discovered on June 21, 1827 by Jean-Louis Pons and Jean-Félix Adolphe Gambart. It has a 186 year orbit and it fits the classical definition of a Halley-type comet. Its last perihelion was in December 2012 and will next come to perihelion around August 2191.

<span class="mw-page-title-main">C/2018 V1 (Machholz–Fujikawa–Iwamoto)</span> Comet

Comet C/2018 V1 (Machholz–Fujikawa–Iwamoto) is a minor body that follows a slightly hyperbolic orbit. It was visually discovered on 7 November 2018 by Donald Machholz using an 18.5-inch reflecting telescope and it reached perihelion on 3 December 2018.

<span class="mw-page-title-main">C/2018 Y1 (Iwamoto)</span> Non-periodic comet

C/2018 Y1 (Iwamoto) is a long period comet with a retrograde orbit discovered on December 18, 2018, by Japanese amateur astronomer Masayuki Iwamoto. Its period is estimated to be 1,733 years. It passed closest to Earth on February 13, 2019. It was expected to reach a magnitude of between 6.5 and 7.5, visible in binoculars or a small telescope and was reported to reach a magnitude of 5.5 by Juan Jose Gonzalez on February 13, before fading to 7.6 two weeks later.

Comet Donati–van Arsdale, formally designated as C/1857 V1, is a parabolic comet co-discovered by Giovanni Battista Donati and Robert van Arsdale a few hours apart on 10 November 1857. It was calculated to have a retrograde trajectory around the Sun.

References

  1. "C/1890 V1 (Zona) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory . Retrieved 7 November 2024.
  2. G. W. Kronk (2003). Cometography: A Catalog of Comets. Vol. 2: 1800–1899. Cambridge University Press. pp. 658–660. ISBN   978-0-521-58505-7.
  3. T. Zona (1891). "Osservazioni della Cometa 1890 IV (Zona Nov. 15)" (PDF). Astronomische Nachrichten (in Italian). 126 (9): 141–142. Bibcode:1891AN....126..141Z. doi: 10.1002/asna.18911260907 .