510 Mabella

Last updated

510 Mabella
Discovery
Discovered by Raymond Smith Dugan
Discovery site Heidelberg
Discovery date20 May 1903
Designations
(510) Mabella
1903 LT
Orbital characteristics [1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 112.91 yr (41239 d)
Aphelion 3.1096  AU (465.19  Gm)
Perihelion 2.1147 AU (316.35 Gm)
2.6122 AU (390.78 Gm)
Eccentricity 0.19043
4.22 yr (1542.0 d)
270.33°
0° 14m 0.456s / day
Inclination 9.5323°
202.719°
90.758°
Physical characteristics
Mean radius
28.72±1.4 km
19.4  h (0.81  d)
0.0687±0.007
9.73

    Mabella (minor planet designation: 510 Mabella) is a minor planet orbiting the Sun.

    Related Research Articles

    <span class="mw-page-title-main">170 Maria</span> S-type Main-belt asteroid

    Maria is a Main belt asteroid that was discovered by French astronomer Henri Joseph Perrotin on January 10, 1877. Its orbit was computed by Antonio Abetti, and the asteroid was named after his sister, Maria. This is the namesake of the Maria asteroid family; one of the first asteroid families to be identified by Japanese astronomer Kiyotsugu Hirayama in 1918.

    Caprera is a minor planet orbiting the Sun.

    Seppina is a minor planet orbiting the Sun.

    <span class="mw-page-title-main">502 Sigune</span>

    Sigune is a minor planet, specifically an asteroid orbiting primarily in the asteroid belt. Like 501 Urhixidur and 500 Selinur, it is named after a character in Friedrich Theodor Vischer's then-bestseller satirical novel Auch Einer.

    Laodica is a minor planet orbiting the Sun.

    <span class="mw-page-title-main">509 Iolanda</span>

    Iolanda is a minor planet orbiting the Sun.

    <span class="mw-page-title-main">518 Halawe</span>

    Halawe is a minor planet orbiting the Sun. It is named after the Middle Eastern confectionery halva.

    <span class="mw-page-title-main">533 Sara</span>

    Sara is a minor planet orbiting the Sun.

    <span class="mw-page-title-main">534 Nassovia</span>

    Nassovia is a minor planet orbiting the Sun. It is a member of the Koronis family of asteroids.

    <span class="mw-page-title-main">543 Charlotte</span> Minor planet asteroid

    Charlotte is a minor planet orbiting the Sun. It was discovered by Paul Götz on September 11, 1904, in Heidelberg.

    Misa is a minor planet orbiting the Sun.

    Irmgard is a minor planet orbiting the Sun.

    Bandusia is a minor planet orbiting the Sun.

    Luisa is a minor planet orbiting the Sun.

    625 Xenia is a minor planet orbiting the Sun. It was discovered by August Kopff in Heidelberg, Germany, on 11 February 1907. The name may have been inspired by the asteroid's provisional designation 1907 XN.

    635 Vundtia is a minor planet orbiting the Sun - though this claim has been disputed.

    733 Mocia is a minor planet orbiting the Sun. A possible occultation was observed by Oscar Canales Moreno on October 1, 2001.

    6144 Kondojiro (1994 EQ3) is an asteroid discovered on March 14, 1994 by Kin Endate and Kazuro Watanabe at the Kitami Observatory in eastern Hokkaidō, Japan. It is named after Jiro Kondo, a Japanese Egyptologist and professor of archaeology at Waseda University.

    2021 LL37 is a large trans-Neptunian object in the scattered disc, around 600 kilometres (370 miles) in diameter. It was discovered on 12 June 2021, by American astronomers Scott Sheppard and Chad Trujillo using Cerro Tololo Inter-American Observatory's Dark Energy Camera in Chile, and announced on 31 May 2022. It was 73.9 astronomical units from the Sun when it was discovered, making it one of the most distant known Solar System objects from the Sun as of May 2022. It has been identified in precovery images from as far back as 28 April 2014.

    2021 RR205 is an extreme trans-Neptunian object and sednoid discovered by astronomers Scott Sheppard, David Tholen, and Chad Trujillo with the Subaru Telescope at Mauna Kea Observatory on 5 September 2021. It resides beyond the outer extent of the Kuiper belt on a distant and highly eccentric orbit detached from Neptune's gravitational influence, with a large perihelion distance of 55.5 astronomical units (AU). Its large orbital semi-major axis (~1,000 AU) suggests it is potentially from the inner Oort cloud. Like 2013 SY99, 2021 RR205 lies in the 50–75 AU perihelion gap that separates the detached objects from the more distant sednoids; dynamical studies indicate that such objects in the inner edge this gap weakly experience "diffusion", or inward orbital migration due to minuscule perturbations by Neptune.

    References

    1. "510 Mabella (1903 LT)". JPL Small-Body Database . NASA/Jet Propulsion Laboratory . Retrieved 6 May 2016.