Asteroidactive

Unknown

AI-narrated summarySnapshot 7f3a · 2026-07-17
Unknown is a 0-m Sq-type near-Earth asteroid discovered 19 June 2004 by R. A. Tucker, D. J. Tholen and F. Bernardi at Kitt Peak. Its 13 April 2029 Earth flyby will pass within 38 012 km of the geocenter — closer than geosynchronous orbit and visible to the naked eye from EMEA . Goldstone observations in 2021 cleared all impact possibilities through 2100.
Open questionsTumbling spin pole orientationInternal porosity2029 tidal deformation predictions
Physical parameters

What we know about the body

Orbit · Heliocentric J2000

Keplerian elements at epoch

Epoch Jul 17, 2026, 04:40 PM UTC·heliocentric ecliptic J2000

a · semi-major axis
0 AUJPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
e · eccentricity
0JPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
i · inclination
JPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
Ω · RAAN
JPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
ω · arg. of periapsis
JPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
M · mean anomaly
JPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
ν · true anomaly
JPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
period
0 dJPL SBDB
JPL SBDBPD-USG

NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
retrieved Jul 17, 2026, 04:40 PM UTC
Earth
Unknown relative to Earth orbit2D · projected to ecliptic
Ephemeris · JPL Horizons

Observation planning

Unknown — apparent RA/Dec/Mag/Range from chosen observer site, or Cartesian state vectors.

No ephemeris rows. Adjust the window or step, then re-run.
Close approaches

Past and predicted passes

Within ~0.3 AU of Earth · sourced live from JPL CAD (1.5 March 2023)

Date (UTC)BodyMiss · kmMiss · AUv · km/sSource
upcoming miss < 100 000 km
Impact monitoring · NASA CNEOS Sentry

Not on the Sentry risk list

Cum. IP
Palermo
Torino max
ReadingNot on the published Sentry risk list. Sentry only catalogues objects with non-zero impact probability over a 100-year window. Brand-new short-arc NEOs may still be on the Scout watch list.
Literature

Top 10 cited papers

Cross-referenced ADS + arXiv. Full citation metadata exports below.

  1. 1

    Velocity space origins of pressure-strain interaction in multi-population distributions and its application to magnetic reconnection

    2026
    M. Hasan Barbhuiya, Paul A. Cassak, Sarah Conley, et al. · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2606.03668Read
  2. 2

    A Calibrated Bayesian Search for Potential Chemical Technosignatures in Polluted White Dwarf

    2026
    Bo-Lun Huang, Zhen-Zhao Tao, Tong-Jie Zhang · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2605.29811Read
  3. 3

    Geophysical intensity problems: the axisymmetric case

    2025
    Ralf Kaiser · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2512.05010Read
  4. 4

    Separating flare and secondary atmospheric signals with RADYN modeling of near-infrared JWST transmission spectroscopy observations of TRAPPIST-1

    2025
    Ward S. Howard, Adam F. Kowalski, Michael Radica, et al. · ApJL 994, L31, 2025
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2512.04265Read
  5. 5

    Enhanced magnetostrophic waves with magnetic field orthogonal to the rotation axis

    2025
    Raviraj Narayan Shinde, Ghanesh Narasimhan · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2512.03120Read
  6. 6

    Resolving star spots on WASP-85 A using high-resolution transit spectroscopy

    2025
    Vedad Kunovac, Heather Cegla, Hritam Chakraborty, et al. · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2510.16881Read
  7. 7

    The Binary Broadening Function

    2024
    Tuan Yi · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2401.17225Read
  8. 8

    On Internal and External Alignment of Dust Grains in Protostellar Environments

    2022
    Thiem Hoang, Le Ngoc Tram, Vo Hong Minh Phan, et al. · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2205.02334Read
  9. 9

    Explosive instability of dust settling in a protoplanetary disc

    2022
    V. V. Zhuravlev · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2203.04792Read
  10. 10

    On the evolution of vortex in locally isothermal self-gravitating discs: a parameter study

    2021
    D. Tarczay-Nehéz, K. Rozgonyi, Zs. Regály · arXiv preprint
    arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv:2111.09073Read
Provenance

Where every value came from

Every cell above is hyperlinked to its primary source. Re-run this card 30 days from now and you’ll get the same numbers — or a diff if the upstream changed.

snapshot zob7-bed3
  • JPL SBDB
    JPL SBDBPD-USG

    NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).

    https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
    retrieved Jul 17, 2026, 04:40 PM UTC
    PD-USG
    NASA/JPL Solar System Dynamics, Small-Body Database (accessed 2026-07-17).
    https://ssd-api.jpl.nasa.gov/sbdb.api?sstr=2015+bf&phys-par=1&full-prec=1&discovery=1
    2026-07-17 16:40:50 UTC
  • arXiv
    arXivarXiv-API-ToU

    Thank you to arXiv for use of its open access interoperability.

    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    retrieved Jul 17, 2026, 04:40 PM UTC
    arXiv-API-ToU
    Thank you to arXiv for use of its open access interoperability.
    https://export.arxiv.org/api/query?search_query=cat:astro-ph.EP+AND+all:bf&start=0&max_results=10&sortBy=submittedDate&sortOrder=descending
    2026-07-17 16:40:49 UTC
What MCPOrbital will not do

Explicit non-promises

Saying no to these protects the brand, the safety posture, and your budget. MCPOrbital operates in research, simulation, decision-support, and sandbox modes only.

  • Send a burn command to a real asset
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  • Replace STK / GMAT for flight-grade analysis
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  • Write your dissertation chapter
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  • Peer-review a paper
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