4868 Knushevia
Bright Hungaria asteroid and suspected binary system.
4868 Knushevia (temporarily designated 1989 UN2) is a bright asteroid belonging to the Hungaria group, located in the innermost part of the main asteroid belt. It is thought to be a possible binary system and has an estimated diameter of about 2 kilometers. The asteroid was discovered on October 27, 1989, by American astronomer Eleanor Helin at the Palomar Observatory in California. Its name honors Kyiv University in Ukraine.
Knushevia is a member of the Hungaria family, the densest cluster of asteroids closest to the Sun within the main belt. It travels around the Sun at a distance ranging from 1.8 to 2.1 astronomical units (AU), completing one orbit every 1,003 days (roughly 2 years and 9 months). Its orbit has a low eccentricity of 0.07 and a relatively high inclination of 22 degrees relative to the ecliptic.
Photometric observations by American astronomer Brian Warner between 2008 and 2011 produced three lightcurves of Knushevia, indicating a rotation period between 4.45 and 4.717 hours. The brightness variation was exceptionally small, only 0.01 magnitude. In May 2015, Warner measured a rotation period of 3.1422 hours with a brightness amplitude of 0.09 magnitude. These observations also suggested that Knushevia might be a binary asteroid, with a possible moon orbiting it every 11.922 hours, though this remains tentative.
Data from NASA's Wide-field Infrared Survey Explorer and its NEOWISE mission show that Knushevia has a diameter of 1.535 kilometers and an extremely high albedo of 1.000. In contrast, the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.40 (typical for bright E-type asteroids, based on 434 Hungaria) and calculates a diameter of 2.30 kilometers from an absolute magnitude of 14.8.
The asteroid was named for Kyiv University (officially the Taras Shevchenko National University of Kyiv), one of Ukraine’s oldest and most prestigious institutions, in recognition of its contributions to education, science, and culture. The naming citation was published by the Minor Planet Center on April 27, 2002.
Quick Facts
- Minorplanet
- yes
- Background
- #D6D6D6
- Discovered
- 27 October 1989
- Discoverer
- E. F. Helin
- Discovery Site
- Palomar Obs.
- Mpc Name
- (4868) Knushevia
- Named After
- Kyiv University / (in Ukraine)
- Mp Category
- main-belt(inner) / Hungaria
- Epoch
- 4 September 2017 (JD 2458000.5)
- Uncertainty
- 0
- Observation Arc
- 33.39 yr (12,196 days)
- Aphelion
- 2.0940 AU
Facts from the source article.
Lore & Background
Knushevia is a bright member of the Hungaria family, which forms the innermost dense concentration of asteroids in the Solar System. It orbits the Sun in the inner main-belt at a distance of 1.8–2.1 AU once every 2 years and 9 months (1,003 days), with an eccentricity of 0.07 and an inclination of 22° with respect to the ecliptic.
Between 2008 and 2011, three rotational lightcurves obtained by American astronomer Brian Warner gave a rotation period between 4.45 and 4.717 hours with an exceptionally low brightness amplitude of 0.01 magnitude. In May 2015, Warner measured a period of 3.1422 hours with an amplitude of 0.09, and photometric observations also revealed that Knushevia might be a binary asteroid with a minor-planet moon orbiting it every 11.922 hours, though the results are tentative only.
According to the NEOWISE survey, Knushevia measures 1.535 kilometers in diameter with an outstandingly high albedo of 1.000. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.40 for bright E-type asteroids and calculates a diameter of 2.30 kilometers based on an absolute magnitude of 14.8.
Reader's Guide
4868 Knushevia is notable as a bright Hungaria asteroid and a suspected binary system, with tentative evidence for a moon. Its discovery by Eleanor Helin at Palomar Observatory in 1989 adds to the catalog of inner-main-belt objects. The asteroid's exceptionally high albedo of 1.000 from NEOWISE data is remarkable, though the Collaborative Asteroid Lightcurve Link uses a different albedo assumption for E-type asteroids, leading to a larger diameter estimate. The naming honors Kyiv University, reflecting the tradition of recognizing educational institutions. The suspected binary nature, if confirmed, would make it a rare binary among Hungaria asteroids, but the results remain tentative. Its lightcurve studies, particularly the low amplitude and varying rotation periods, highlight the challenges in characterizing small asteroids.
Did You Know?
- Knushevia has an exceptionally high albedo of 1.000 according to NEOWISE data.
- It is a suspected binary asteroid with a possible moon orbiting every 11.922 hours.
- The asteroid was named after Kyiv University in Ukraine.
- Its rotation period has been measured between 4.45 and 4.717 hours, and also at 3.1422 hours.
The Naming of 4868 Knushevia
In 2002, the asteroid 4868 Knushevia received its designation in honour of the Taras Shevchenko National University of Kyiv. This celestial naming served as a cosmic tribute to one of Ukraine's most distinguished educational institutions. The university, also referred to by shorter names such as Kyiv University or Shevchenko University, has long stood as a beacon of higher learning in the country. The asteroid's designation connects the vastness of space to the grounded achievements of a public university in Kyiv that has trained specialists across numerous fields of knowledge and carried out research for nearly two centuries. It is a reminder that the contributions of academic institutions can transcend terrestrial boundaries and earn a permanent place in the catalog of objects orbiting the Sun, linking the scholarly traditions of a single city to the broader human endeavour of understanding the cosmos.
The Institution Behind the Name
The university honoured by asteroid 4868 Knushevia traces its origins to 1834, when Nicholas I of Russia established the Saint Vladimir Imperial University of Kiev, naming it after Vladimir the Great, the tenth- and eleventh-century ruler of Kievan Rus'. The choice reflected the Russian Empire's emphasis on Orthodox Christianity and Kyiv's role as the cradle of Eastern Christianity. The institution absorbed assets from Vilnius University and a Kremenets lyceum closed after the November Uprising of 1830. Its first cohort of sixty-two students began studies that year in a single Faculty of Philosophy. Over the decades it expanded to include Law and Medicine, and the original Faculty of Philosophy was eventually split into History and Philology and Natural Sciences. The university was renamed after Mykhailo Drahomanov in 1920, then after Taras Shevchenko in 1939. Shevchenko, the great Ukrainian poet and artist, had been banned from educational activities for political reasons but had worked for the university as a field researcher between 1845 and 1846.
Academic Prestige Worthy of Celestial Recognition
The university that gave its name to asteroid 4868 Knushevia is widely regarded as the most prestigious institution of higher education in Ukraine. It comprises fifteen faculties and five institutes, training specialists in a greater number of academic fields than any other Ukrainian educational body. With approximately thirty thousand students enrolled, it functions as both a major centre of learning and research and an important cultural hub. During the Soviet era it was counted among the top three universities in the entire USSR, alongside Moscow State University and Leningrad State University. In modern rankings it placed within the top six hundred and fifty universities worldwide according to QS between 2014 and 2017. Scopus data from 2009 identified it as the highest research paper producer in Ukraine by both output volume and total citation count. Delovoy magazine named it the best university in the country, and the independent Compas ranking placed it first for the adequacy of its graduates to the national labour market.
A Global Legacy Reflected in the Stars
The international footprint of the university behind asteroid 4868 Knushevia is substantial. Since 1960, when it first admitted international students, it has trained over twenty thousand highly qualified specialists for one hundred and twenty countries. The earliest foreign cohorts came from Cuba, Guinea, Indonesia, Ghana, Togo, Nigeria, Cameroon, Benin, Zanzibar, Yemen, Algeria, Namibia, and Afghanistan, going on to become doctors, engineers, diplomats, economists, and statesmen in their home nations. Today the university maintains relations and student exchange programmes with over four hundred partner institutions across forty countries. Its alumni roll includes luminaries such as Mykola Lysenko, Nikolay Berdyaev, Mikhail Bulgakov, Theodosius Dobzhansky, and Leonid Kravchuk. Even in conflict the institution has shown resilience: during the German-Soviet war it was evacuated to Kyzylorda in Kazakhstan, and in November 2024 Russian drone strikes damaged its Institutes of International Relations and Journalism. The asteroid's name endures as a symbol of this enduring commitment to knowledge.
Frequently Asked Questions
What is asteroid 4868 Knushevia?
It is a remarkably bright rocky body orbiting in the innermost region of the main asteroid belt, classified as part of the Hungaria group. At roughly 1.5 to 2 kilometers across, it is suspected to actually be two objects gravitationally bound together as a binary pair.
Who found 4868 Knushevia and when?
American astronomer Eleanor Helin spotted it on October 27, 1989, using the instruments at Palomar Observatory in California. It carried the temporary label 1989 UN2 before receiving its permanent number and name.
What makes 4868 Knushevia stand out among other asteroids?
Its surface reflectivity is extraordinarily high—NEOWISE data suggests an albedo near 1.0, meaning it bounces back nearly all incident sunlight. Combined with its compact size and suspected binary nature, it ranks among the brightest members of the Hungaria cluster.
What is the Hungaria group, and where does Knushevia fit in?
The Hungaria family is the tightest-packed swarm of asteroids that orbits closest to the Sun within the main belt. Knushevia is a confirmed member of this group, circling the Sun at distances that place it well inside the bulk of the belt.
Why is the asteroid named Knushevia?
The name pays tribute to Kyiv University in Ukraine, honoring the institution's long-standing contributions to science and education. It follows the common convention of naming asteroids after notable people, places, or institutions.
More in Notable Asteroids, Part 3 1-24
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