291 Alice

Last updated

291 Alice
291Alice (Lightcurve Inversion).png
A three-dimensional model of 291 Alice based on its light curve
Discovery
Discovered by Johann Palisa
Discovery date25 April 1890
Designations
(291) Alice
A890 HA, 1954 UJ3
main-belt
Orbital characteristics [1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 124.62 yr (45516 d)
Aphelion 2.4273  AU (363.12  Gm)
Perihelion 2.01631 AU (301.636 Gm)
2.22182 AU (332.380 Gm)
Eccentricity 0.092495
3.31 yr (1209.7 d)
115.293°
0° 17m 51.382s / day
Inclination 1.8555°
161.655°
331.580°
Physical characteristics
Dimensions14.97±1.1  km [1]
19×12×11 km [2] [3]
Mass ~
Mean density
~2.7 g/cm3 [4]
4.313  h (0.1797  d) [1]
0.180 d (4.32 h) [5]
0.2075±0.033 [1]
0.208 [2]
S [6]
11.45

    Alice (minor planet designation: 291 Alice) is a stony background asteroid from the inner region of the asteroid belt. It was discovered by Johann Palisa on 25 April 1890 at the Vienna Observatory.

    Contents

    Photometric observations of this asteroid at the Leura Observatory in Leura, Australia during 2006 gave a rotation period of 4.313 ± 0.002 hours and a brightness variation of 0.20 ± 0.02 in magnitude. This result is in agreement with previous studies. [7] Lightcurve analysis indicates that Alice's pole points towards either ecliptic coordinates (β, λ) = (55°, 65°) or (β, λ) = (55°, 245°) with a 10° uncertainty. [3] This gives an axial tilt of about 35° in both cases.

    See also

    Related Research Articles

    <span class="mw-page-title-main">20 Massalia</span> Main-belt Massalian asteroid

    Massalia, minor planet designation 20 Massalia, is a stony asteroid and the parent body of the Massalia family located in the inner region of the asteroid belt, approximately 145 kilometers in diameter. Discovered by Italian astronomer Annibale de Gasparis on 19 September 1852, it was named for the French city of Marseille, from which the independent discover Jean Chacornac sighted it the following night. It was the first asteroid that was not assigned an iconic symbol by its discoverer.

    <span class="mw-page-title-main">43 Ariadne</span> Main-belt asteroid

    Ariadne is a fairly large and bright main-belt asteroid. It is the second-largest member of the Flora asteroid family. It was discovered by N. R. Pogson on 15 April 1857 and named after the Greek heroine Ariadne.

    <span class="mw-page-title-main">108 Hecuba</span>

    Hecuba is a fairly large and bright main-belt asteroid. It was discovered by Karl Theodor Robert Luther on 2 April 1869, and named after Hecuba, wife of King Priam in the legends of the Trojan War in Greek Mythology. This object is orbiting the Sun with a period of 5.83 years and an eccentricity of 0.06. It became the first asteroid discovered to orbit near a 2:1 mean-motion resonance with the planet Jupiter, and is the namesake of the Hecuba group of asteroids.

    <span class="mw-page-title-main">135 Hertha</span> Main-belt asteroid

    Hertha is an asteroid from the inner region of the asteroid belt, approximately 77 kilometers in diameter. Discovered on 18 February 1874 by German–American astronomer Christian Peters at the Litchfield Observatory near Clinton, New York, it was named after the Teutonic and Scandinavian goddess of fertility, Hertha, also known as Nerthus. It orbits among the Nysa asteroid family, but its classification as a metallic M-type asteroid does not match the more common F-type asteroid for this family, suggesting that it may be an interloper. Spectroscopic analysis indicates the possible presence of hydrated silicates indicating that Hertha should possibly be reclassified from its present M-type to the proposed W-type.

    <span class="mw-page-title-main">159 Aemilia</span> Main-belt asteroid

    Aemilia is a large main-belt asteroid. Aemilia was discovered by the French brothers Paul Henry and Prosper Henry on January 26, 1876. The credit for this discovery was given to Paul. It is probably named after the Via Aemilia, a Roman road in Italy that runs from Piacenza to Rimini.

    <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.

    <span class="mw-page-title-main">258 Tyche</span> Main belt asteroid

    Tyche is a relatively large main belt asteroid discovered by Robert Luther at Düsseldorf-Bilk Observatory on 4 May 1886. The stony S-type asteroid measures about 65 kilometers in diameter and has a perihelion of 2.1 AU.

    <span class="mw-page-title-main">292 Ludovica</span> Main-belt asteroid

    Ludovica is a main belt asteroid.

    <span class="mw-page-title-main">390 Alma</span> Main-belt asteroid

    Alma is an asteroid from the intermediate asteroid belt, approximately 24 kilometers in diameter. It was Guillaume Bigourdan's only asteroid discovery. He discovered it on 24 March 1894 in Paris.

    <span class="mw-page-title-main">462 Eriphyla</span> Main-belt asteroid

    462 Eriphyla is a Koronian asteroid from the outer regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 22 October 1900. The stony S-type asteroid has a rotation period of 8.7 hours and measures approximately 35 kilometers in diameter. It was named after Eriphyle, from Greek mythology.

    Friederike is a minor planet orbiting in the asteroid belt. It is a member of the Hygiea family of asteroids.

    <span class="mw-page-title-main">573 Recha</span> Minor planet orbiting in the asteroid belt

    Recha is a minor planet, specifically an asteroid orbiting in the asteroid belt between Mars and Jupiter. The asteroid, discovered by German astronomer Max Wolf on September 19, 1905, was named after a character in Gotthold Ephraim Lessing's play Nathan the Wise and may have been inspired by the asteroid's provisional designation 1905 RC.

    Renate is a minor planet, specifically an asteroid orbiting in the asteroid belt which was discovered by German astronomer Max Wolf on September 19, 1905. The name may have been inspired by the asteroid's provisional designation 1905 RE.

    630 Euphemia is a mid-sized Eunomian asteroid.

    639 Latona is a minor planet, specifically an asteroid orbiting in the asteroid belt. It was discovered by German astronomer Karl Lohnert on July 19, 1907, at Heidelberg.

    <span class="mw-page-title-main">867 Kovacia</span>

    867 Kovacia is an elongated, dark asteroid and member of the Hygiea family from the outer regions of the asteroid belt. It was discovered on 25 February 1917, by astronomer Johann Palisa at the Vienna Observatory in Austria. The carbonaceous C/B-type asteroid has a rotation period of 8.7 hours and measures approximately 24 kilometers in diameter. It was named after Austrian physician Friedrich Kovacs (1861–1931).

    5642 Bobbywilliams, provisional designation 1990 OK1, is an eccentric, stony asteroid and Mars-crosser from the inner regions of the asteroid belt, approximately 4.7 kilometers in diameter.

    4957 Brucemurray, provisional designation 1990 XJ, is a stony asteroid, classified as near-Earth object of the Amor group and as Mars-crosser, approximately 3 kilometers in diameter. It was discovered by American astronomer Eleanor Helin at the Palomar Observatory in California on 15 December 1990. The asteroid was named after American planetary scientist Bruce C. Murray.

    <span class="mw-page-title-main">1251 Hedera</span>

    1251 Hedera is a background asteroid from the central regions of the asteroid belt, approximately 13 kilometers in diameter. It was discovered on 25 January 1933, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named for the climbing plant Hedera, commonly known as "ivy".

    <span class="mw-page-title-main">1996 PW</span>

    1996 PW is an exceptionally eccentric trans-Neptunian object and damocloid on an orbit typical of long-period comets but one that showed no sign of cometary activity around the time it was discovered. The unusual object measures approximately 10 kilometers in diameter and has a rotation period of 35.4 hours and likely an elongated shape.

    References

    1. 1 2 3 4 Yeomans, Donald K., "291 Alice", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory , retrieved 11 May 2016.
    2. 1 2 Supplemental IRAS Minor Planet Survey Archived June 23, 2006, at the Wayback Machine
    3. 1 2 A. Kryszczyńska; et al. (1996). "CCD Photometry of Seven Asteroids: New Spin Axis and Shape Determinations". Icarus. 124 (1): 134–140. Bibcode:1996Icar..124..134K. doi:10.1006/icar.1996.0194.
    4. G. A. Krasinsky; et al. (2002). "Hidden Mass in the Asteroid Belt". Icarus. 158 (1): 98–105. Bibcode:2002Icar..158...98K. doi:10.1006/icar.2002.6837.
    5. PDS lightcurve data
    6. "Asteroid Taxonomy". Planetary Science Institute . Retrieved 27 February 2016.
    7. Oey, Julian (December 2006), "Lightcurves analysis of 10 asteroids from Leura Observatory", The Minor Planet Bulletin, 33 (4): 96–99, Bibcode:2006MPBu...33...96O.