8 Flora

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8 Flora
8 Flora VLT (2021), deconvolved.pdf
Discovery
Discovered by J.R. Hind
Discovery date18 October 1847
Designations
(8) Flora
Pronunciation /ˈflɔːrə/
Named after
Flōra
Main belt (Flora family)
Adjectives Florian /ˈflɔːriən/
Symbol Flora symbol (bold).svg (historical)
Orbital characteristics [1]
Epoch 31 March 2024
(JD  2460400.5)
Aphelion 2.55  AU (381 million  km)
Perihelion 1.86 AU (278 million km)
2.20 AU (329 million km)
Eccentricity 0.15650
3.27 yr (1192.84 d)
317.3°
Inclination 5.889°
110.87°
1 February 2024
285.6°
Earth  MOID 0.87 AU (130 million km)
Proper orbital elements [2]
2.2014  AU
Proper eccentricity
0.1449
Proper inclination
5.574°
Proper mean motion
110.2  deg  / yr
3.26679 yr
(1193.194 d)
Precession of perihelion
32.017  arcsec  / yr
Precession of the ascending node
−35.51  arcsec  / yr
Physical characteristics
Dimensions136  km × 136  km × 113  km [3]
145 km × 145 km × 120 km [4]
Mean diameter
146±2 km [5]
128 km [3]
Flattening 0.18 [lower-alpha 1]
Mass (4±1.6)×1018 kg [5]
(6.62±0.84)×1018 kg [lower-alpha 2] [6]
Mean density
2.4±1.0 g/cm3 [5]
3.04±1.39 g/cm3 [6]
0.533 d (12.799 h) [1]
0.224 (calculated) [5]
0.226 [1]
S [1]
7.9 [7] to 11.6
6.61 [1]
0.21" to 0.053"

    Flora (minor planet designation: 8 Flora) is a large, bright main-belt asteroid. It is the innermost large asteroid: no asteroid closer to the Sun has a diameter above 25 kilometres (20% that of Flora), and not until 20-km 149 Medusa was discovered was an asteroid known to orbit at a closer mean distance. [8] It is the seventh-brightest asteroid with a mean opposition magnitude of +8.7. [9] Flora can reach a magnitude of +8.1 at a favorable opposition near perihelion, such as occurred in November 2020 when it was 0.88  AU (132 million  km ; 340  LD ) from Earth. [10]

    Contents

    Discovery and naming

    Flora was discovered by J. R. Hind on 18 October 1847. It was his second asteroid discovery after 7 Iris.[ citation needed ]

    The name Flora was proposed by John Herschel, from Flora, the Latin goddess of flowers and gardens, wife of Zephyrus (the personification of the West wind), and mother of Spring. The Greek equivalent is Chloris, who has her own asteroid, 410 Chloris, but in Greek 8 Flora is also called 8 Chloris (8 Χλωρίς).[ citation needed ] The old iconic symbol for 8 Flora has been variously rendered as Flora symbol (fixed width).svg , Flora symbol (simple, fixed width).svg , etc. It is in the pipeline for Unicode 17.0 as U+1CEC2 𜻂 ( Flora symbol (fixed width).svg ). [11] [12]

    Characteristics

    The orbit of 8 Flora compared with the orbits of Earth, Mars and Jupiter FloraOrbit.png
    The orbit of 8 Flora compared with the orbits of Earth, Mars and Jupiter

    Lightcurve analysis indicates that Flora's pole points towards ecliptic coordinates (β, λ) = (16°, 160°) with a 10° uncertainty. [4] This gives an axial tilt of 78°, plus or minus ten degrees.

    Flora is the parent body of the Flora family of asteroids, and by far the largest member, comprising about 80% of the total mass of this family. Nevertheless, Flora was almost certainly disrupted by the impact(s) that formed the family, and is probably a gravitational aggregate of most of the pieces.[ citation needed ]

    Flora's spectrum indicates that its surface composition is a mixture of silicate rock (including pyroxene and olivine) and nickel-iron metal. Flora, and the whole Flora family generally, are good candidates for being the parent bodies of the L chondrite meteorites. [13] This meteorite type comprises 35% of meteorites impacting the Earth. [14]

    Observational mishap

    During an observation on 25 March 1917, 8 Flora was mistaken for the 15th-magnitude star TU Leonis, which led to that star's classification as a U Geminorum cataclysmic variable star. [15] Flora had come to opposition on 1917 February 13, 40 days earlier. [15] This mistake was uncovered only in 1995. [15] [16]

    Occultation

    On 26 July 2013, Flora at magnitude 8.8 occulted the star 2UCAC 22807162 over parts of South America, Africa, and Asia. [17]

    In the 1968 science-fiction film The Green Slime , an orbital perturbation propels the asteroid Flora into a collision course with Earth.

    Size comparison: the first 10 asteroids profiled against Earth's Moon. Flora is third from the right. Moon and Asteroids 1 to 10.svg
    Size comparison: the first 10 asteroids profiled against Earth's Moon. Flora is third from the right.

    Notes

    1. Flattening derived from the maximum aspect ratio (c/a): , where (c/a) = 0.82±0.05. [5]
    2. (3.33±0.42)×10−12 M

    Related Research Articles

    <span class="mw-page-title-main">3 Juno</span> Asteroid in the asteroid belt

    Juno is a large asteroid in the asteroid belt. Juno was the third asteroid discovered, in 1804, by German astronomer Karl Harding. It is one of the twenty largest asteroids and one of the two largest stony (S-type) asteroids, along with 15 Eunomia. It is estimated to contain 1% of the total mass of the asteroid belt.

    <span class="mw-page-title-main">5 Astraea</span> Large asteroid

    Astraea is an asteroid in the asteroid belt. This object is orbiting the Sun at a distance of 385 million kilometres (2.5735 AU) with a period of 4.13 yr and an orbital eccentricity of 0.19. The orbital plane is inclined at an angle of 5.37° to the plane of the ecliptic. It is spinning with a period of 16.8 h. The surface of Astraea is highly reflective and its composition is probably a mixture of nickel–iron with silicates of magnesium and iron. It is an S-type asteroid in the Tholen classification system.

    <span class="mw-page-title-main">6 Hebe</span> Large main-belt asteroid

    Hebe is a large main-belt asteroid, containing around 0.5% of the mass of the belt. However, due to its apparently high bulk density, Hebe does not rank among the top twenty asteroids by volume. This high bulk density suggests an extremely solid body that has not been impacted by collisions, which is not typical of asteroids of its size – they tend to be loosely-bound rubble piles.

    <span class="mw-page-title-main">7 Iris</span> Large main-belt asteroid

    Iris is a large main-belt asteroid and possible remnant planetesimal orbiting the Sun between Mars and Jupiter. It is the fourth-brightest object in the asteroid belt. 7 Iris is classified as an S-type asteroid, meaning that it has a stony composition.

    <span class="mw-page-title-main">9 Metis</span> Main-belt asteroid

    Metis is one of the larger main-belt asteroids. It is composed of silicates and metallic nickel-iron, and may be the core remnant of a large asteroid that was destroyed by an ancient collision. Metis is estimated to contain just under half a percent of the total mass of the asteroid belt.

    <span class="mw-page-title-main">11 Parthenope</span> Main-belt asteroid

    Parthenope is a large, bright main-belt asteroid.

    <span class="mw-page-title-main">17 Thetis</span> Main-belt asteroid

    Thetis, minor planet designation 17 Thetis, is a stony asteroid from the inner regions of the asteroid belt, approximately 90 kilometers in diameter. It was discovered on 17 April 1852, by German astronomer Robert Luther at Bilk Observatory in Düsseldorf, Germany who deferred to Friedrich Wilhelm August Argelander the naming his first asteroid discovery after Thetis from Greek mythology. Its historical symbol was a dolphin and a star; it is in the pipeline for Unicode 17.0 as U+1CECA 𜻊.

    <span class="mw-page-title-main">18 Melpomene</span> Main-belt asteroid

    Melpomene is a large, bright main-belt asteroid that was discovered by J. R. Hind on 24 June 1852, and named after Melpomenē, the Muse of tragedy in Greek mythology. Its historical symbol was a dagger over a star; it is in the pipeline for Unicode 17.0 as U+1CECB 𜻋.

    <span class="mw-page-title-main">19 Fortuna</span> Main-belt asteroid

    Fortuna is one of the largest main-belt asteroids. It has a composition similar to 1 Ceres: a darkly colored surface that is heavily space-weathered with the composition of primitive organic compounds, including tholins.

    <span class="mw-page-title-main">28 Bellona</span> Main-belt asteroid

    Bellona is a large main-belt asteroid. It was discovered by German astronomer R. Luther on March 1, 1854, and named after Bellōna, the Roman goddess of war; the name was chosen to mark the beginning of the Crimean War. Its historical symbol was Bellona's whip and spear; it is in the pipeline for Unicode 17.0 as U+1CECE 𜻎.

    <span class="mw-page-title-main">29 Amphitrite</span> Main-belt asteroid

    Amphitrite is one of the largest S-type asteroids, approximately 200 kilometers in diameter, and probably fifth largest after Eunomia, Juno, Iris and Herculina.

    <span class="mw-page-title-main">146 Lucina</span> Main-belt asteroid

    Lucina is a main-belt asteroid that was discovered by Alphonse Borrelly on June 8, 1875, and named after Lucina, the Roman goddess of childbirth. It is large, dark and has a carbonaceous composition. The spectra of the asteroid displays evidence of aqueous alteration.

    <span class="mw-page-title-main">152 Atala</span> Main-belt asteroid

    Atala is a large main belt asteroid that was discovered by brothers Paul Henry and Prosper Henry on 2 November 1875, but the discovery was credited to Paul. It is a type D asteroid, meaning that it is composed of carbon, organic rich silicates and possibly water ice.

    <span class="mw-page-title-main">230 Athamantis</span> Main-belt asteroid

    Athamantis is a fairly large main-belt asteroid that was discovered by the German-Austrian astronomer K. de Ball on September 3, 1882, in Bothkamp. It was his only asteroid discovery. The asteroid was named after Athamantis, daughter of Athamas the mythical Greek king of Orchomenus.

    <span class="mw-page-title-main">238 Hypatia</span> Main-belt asteroid

    Hypatia is a very large main-belt asteroid that was discovered by Russian astronomer Viktor Knorre on July 1, 1884, in Berlin. It was the third of his four asteroid discoveries. The name was given in honour of philosopher Hypatia of Alexandria. Based upon the spectrum, it is classified as a C-type asteroid and is probably composed of primitive carbonaceous material. Like many asteroids of this type, its surface is very dark in colour.

    <span class="mw-page-title-main">248 Lameia</span> Asteroid

    Lameia is a typical main belt asteroid. It was discovered by Austrian astronomer Johann Palisa on 5 June 1885 in Vienna and was named after the Lamia, a lover of Zeus in Ancient Greek mythology. 248 Lameia is orbiting the Sun with a period of 3.88 years and a low eccentricity (ovalness) of 0.067. The semimajor axis of 2.47 AU is slightly inward from the 3:1 Kirkwood Gap. Its orbital plane is inclined by 4° to the plane of the ecliptic.

    <span class="mw-page-title-main">381 Myrrha</span> Main-belt asteroid

    Myrrha is a main-belt asteroid that was discovered by the French astronomer Auguste Charlois on January 10, 1894, in Nice. It has been classified as a C-type asteroid and is most likely composed of carbonaceous material.

    Chloris is a very large main-belt asteroid that was discovered by Auguste Charlois on January 7, 1896, in Nice. It is classified as a C-type asteroid and is probably composed of primitive carbonaceous material. The spectrum of the asteroid displays evidence of aqueous alteration. It is the namesake of the Chloris family of asteroids.

    618 Elfriede is a minor planet orbiting the Sun. On July 24, 2013, it occulted the magnitude 12.8 star 2UCAC 23949304, over parts of Mexico and southwestern United States.

    3703 Volkonskaya, provisional designation 1978 PU3, is a Vestian asteroid and asynchronous binary system from the inner regions of the asteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 9 August 1978, by Soviet astronomers Lyudmila Chernykh and Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. It was named by the discoverers after the Russian princess Mariya Volkonskaya. The V-type asteroid has a rotation period of 3.2 hours. The discovery of its 1.4-kilometer minor-planet moon was announced in December 2005.

    References

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    16. "IAUC 6174".
    17. Asteroid Occultation Index Page