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More than two dozen known asteroids have better than a one in a million chance of impacting into Earth within the next 100 years.<ref name="NYT-20130209"/>
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'''Sentry''' is a highly automated collision monitoring system that continually scans the most current [[asteroid]] catalog for possibilities of future impact with [[Earth]] over the next 100 years.<ref name="risk-table"/> Whenever a potential impact is detected it will be analyzed and the results immediately published on the [[Near Earth Object Program]].<ref name="risk-table"/>
{{short description|JPL program to monitor the Minor Planet Center's catalog for Earth impacts}}
[[File:2020VV risk corridor.png|thumb|right|Asteroid [[2020 VV]] risk corridor for the obsolete virtual impactor of 12 October 2033.]]
'''Sentry''' is a highly automated [[Asteroid impact prediction|impact prediction]] system operated by the [[JPL]] Center for NEO Studies (CNEOS) since 2002. It continually monitors the most up-to-date [[asteroid]] catalog for possibilities of future impact with [[Earth]] over the next 100+ years.<ref name="risk-table"/> Whenever a potential impact is detected it will be analyzed and the results immediately published by the [[Center for Near-Earth Object Studies]].<ref name="risk-table"/> However, several weeks of optical data are not enough to conclusively identify an impact years in the future.<ref name="Giorgini"/> By contrast, eliminating an entry on the risk page is a negative prediction (a prediction of where it will ''not'' be).<ref name="Giorgini"/>


Scientists warn against worrying about the possibility of impact with an object based on only a few weeks of optical data that show a possible Earth encounter years from now.<ref name="Giorgini"/> Sometimes, it cannot even be said for certain what side of the Sun such an object will be at the time of the listed virtual impactor date.<ref name="Giorgini"/> For example, even though {{mpl|2005 ED|224}} had a 1-in-500,000 chance of impacting Earth on 11 March 2023, it was expected to be farther than the Sun at the time.<ref name="NEODyS2023"/> Most objects on the Sentry Risk Table have an [[observation arc]] of less than 14 days and have not been observed for years.
Two or three weeks of optical data is not enough to conclusively identify an impact years in the future.<ref name="Giorgini"/> By contrast, eliminating an entry on the risk page is a negative prediction; a prediction of where it will ''not'' be.<ref name="Giorgini"/> As far as the public is concerned, it just isn't worth getting worried about an object with a couple weeks of optical data showing a possible Earth encounter years from now.<ref name="Giorgini"/>


There are 1620 near-Earth asteroids listed on the risk table with 37,736 virtual impactor dates. For each asteroid listed on the risk table there are on average about 23 virtual impactors. Only about 19 objects on the risk list are large enough to be considered [[potentially hazardous object]]s with a diameter greater than about 140 meters. The average size of an object on the default page of Sentry is 120 meters with an average impact probability of 1:500. More [[Orbital eccentricity|eccentric]] orbits (such as {{mp|2015 RD|36}}) that extend to nearly the orbit of [[Jupiter]] can make [[atmospheric entry]] at velocities of ~{{Convert|40|km/s|mi/s|abbr=unit}}.<ref name=velocity/>
The Impact Risk page lists a number of lost objects such as {{mpl|2004 BX|159}} that are, for all practical purposes, permanent residents of the risk page; their removal may depend upon a serendipitous rediscovery.<ref name="intro"/> Some objects on the Sentry Risk Table, such as {{mpl|2000 SG|344}}, might even be man-made.


==Sentry Risk Table==
Notable objects on the risk page include (numbered asteroids listed first): [[99942 Apophis]], {{mpl|(101955) 1999 RQ|36}}, {{mpl|2007 VK|184}}, {{mpl|1994 WR|12}}, and {{mpl|2011 BT|15}}.<ref name="risk-table"/>
{|class="wikitable sortable floatright" style="text-align:center; font-size:0.9em;"
|+Objects with better than a 1/500 (0.2%) cumulative chance of impact
! Object
! Cumulative<br/>Impact<br/>Probability
! Date of<br/>Greatest Risk
! Estimated<br/>Diameter<br/>(meters)
! [[Observation arc|Observation<br/>arc]]<br/>(days)
|-
| '''{{mpl|2010 RF|12}}''' || 10% || 2095-09-05 || 7 || 4374
|-
| '''{{mpl|2020 CD|3}}''' || 2.5% || 2082-09-09 || 2 || 742
|-
| '''{{mpl|2006 RH|120}}''' || 1.3% || 2044-02-08 || 4 || 281
|-
| {{mp|2017 WT|28}} || 1.2% || 2104-11-24 || 8 || 19
|-
| {{mp|2020 VW}} || 0.70% || 2074-11-02 || 7 || 14
|-
| '''{{mpl|2006 JY|26}}''' || 0.50% || 2074-05-03 || 7 || 3
|-
| {{mp|2020 CQ|1}} || 0.46% || 2070-02-03 || 6 || 29
|-
| {{mp|2022 SX|55}} || 0.40% || 2035-09-17 || 3 || 1
|-
| '''{{mpl|2022 NX|1}}''' || 0.32% || 2075-12-03 || 8 || 142
|-
| '''{{mpl|2000 SG|344}}''' || 0.27% || 2071-09-16 || 37 || 507
|-
| '''{{mpl|2022 YO|1}}''' || 0.23% || 2024-12-17 || 3 || 1
|-
| '''{{mpl|2020 VV}}''' || 0.23% || 2056-10-11 || 12 || 61
|-
| {{mp|2017 LD}} || 0.22% || 2079-06-10 || 11 || 45
|-
| {{mp|2000 LG|6}} || 0.21% || 2094-05-27 || 5 || 2
|}


The Impact Risk page lists a number of [[lost minor planet]]s that are, for all practical purposes, permanent residents of the risk page; their removal may depend upon a [[serendipity|serendipitous]] rediscovery.<ref name="intro"/> Lost asteroid [[1979 XB]] has been on the list since the list's inception.<ref name="Sentry2002"/> {{mpl|2007 FT|3}} and {{mpl|2014 MV|67}} with their very short 1-day observation arcs have missed virtual impactor dates as they were likely quite distant from the Earth at the time. {{mpl|1997 XR|2}} was serendipitously rediscovered in 2006 after being [[Lost minor planet|lost]] for more than 8 years. {{mpl|2004 BX|159}} was determined to be a harmless [[main belt]] asteroid in 2014. Some objects on the Sentry Risk Table, such as {{mpl|2000 SG|344}}, might even be artificial.<ref>{{cite web |title=Much Ado about 2000 SG344 |url=https://science.nasa.gov/science-news/science-at-nasa/2000/ast06nov_2 |website=NASA Science |publisher=NASA |access-date=27 September 2023}}</ref>
The diameter of most near-Earth asteroids that have not been studied by [[Radar astronomy|radar]] or [[Infrared astronomy|infrared]] can generally only be estimated within about a factor of 2 based on the asteroids [[Absolute magnitude#Solar System bodies (H)|absolute magnitude]] (H).<ref name="risk-table"/> More than two dozen known asteroids have better than a one in a million chance of impacting into Earth within the next 100 years.<ref name="NYT-20130209"/>

{{mpl|2010 RF|12}} is the asteroid with greatest probability (10%) of impacting Earth, but is only ~7 meters in diameter. The only [[Minor planet designation|numbered]] objects with [[observation arc]]s of several years are [[(29075) 1950 DA]] and [[101955 Bennu]].<ref name="risk-table"/> Notable asteroids removed from Sentry include (most recently removed listed first): [[99942 Apophis]], [[(410777) 2009 FD]], {{mpl|2006 QV|89}}, {{mpl|2017 XO|2}}, {{mpl|1994 WR|12}}, {{mpl|2007 VK|184}}, {{mpl|2013 BP|73}}, {{mpl|2008 CK|70}}, {{mpl|2013 TV|135}}, {{mpl|2011 BT|15}}, [[367943 Duende]], and {{mpl|2011 AG|5}}.

Of the 160 asteroids with better than a 1-in-10,000 chance of impacting Earth only [[101955 Bennu]] is larger than 50 meters in diameter.

The soonest virtual impactor of an asteroid larger than 50 meters in diameter with a better than 1:1-million chance of impact is {{mp|2022 PX|1}} on 11 August 2040 with a 1:{{val|330000}} chance of impact.<ref name="VIs"/> It is estimated to be 120-meters in diameter, has a short observation arc of 3.1-days, and is expected to be {{convert|1.78|AU|e6km|abbr=unit|lk=on}} from Earth on 11 August 2040.<ref name=Horizons2022PX1/> The impact scenario is outside the [[3-sigma]] uncertainty region of {{Nowrap|± 240 million km}}.

{{anchor|2023}}
The asteroid with the greatest chance of impacting Earth in 2023 is {{mp|2016 LP|10}} (4-meters in diameter) with less than a 1-day observation arc.<ref name="VIs"/> It had a 1:53,000 chance of impact on 10 June 2023, but was expected to be around {{Convert|0.6|AU|e6km|abbr=unit|lk=on}} from Earth on that date.<ref name="Horizons2023"/> Such an impact would be similar to {{mpl|2008 TC|3}}.

With a 24-day observation arc, {{mp|2017 SA|20}} has the most virtual impactors with 1244 virtual impactor dates.<ref name="risk-table"/><ref>[https://cneos.jpl.nasa.gov/sentry/details.html#?des=2017%20SA20 Sentry: 2017 SA20] (1244 VIs) using 2022-Aug-30 solution</ref>

The diameter of most near-Earth asteroids that have not been studied by [[Radar astronomy|radar]] or [[Infrared astronomy|infrared]] can generally only be estimated within about a factor of 2 based on the asteroid's [[Absolute magnitude#Solar System bodies (H)|absolute magnitude]] (H).<ref name="risk-table"/> Their mass, consequently, is uncertain by about a factor of 10. For near-Earth asteroids without a well-determined diameter, Sentry assumes a generic [[Albedo#Astronomical albedo|albedo]] of 0.15.

In August 2013, the Sentry Risk Table started using planetary [[ephemeris]] ([[Jet Propulsion Laboratory Development Ephemeris#Ephemerides in the series|DE431]]) for all NEO orbit determinations.<ref name="notes"/> DE431 ([[JPL Small-Body Database|JPL small-body]] perturber ephemeris: SB431-BIG16) better models the gravitational [[Perturbation (astronomy)|perturbations]] of the planets and includes the 16 most massive [[main-belt asteroid]]s.<ref name="notes"/> In April 2021, Sentry transitioned to [[Jet Propulsion Laboratory Development Ephemeris#Ephemerides in the series|DE441]] which removed the very low impact probability of short-arc [[2014 MV67]] which had been less than 1:1-billion. The switch to DE441 also briefly added in the harmless Jupiter trojan [[2014 ES57]] with a very low impact probability of about 1:1-billion.

JPL launched major changes to the website in February 2017 and re-directed the classic page on 10 April 2017.

In 2021 JPL launched Sentry-II which handles the [[Yarkovsky effect]] that can significantly change a small asteroids path over decades and centuries.<ref name="Sentry-II"/> Sentry-II defaults to an Impact Pseudo-Observation (IOBS) analysis technique that runs an extended orbit-determination filter that tries to converge to an impacting solution compatible with the observational data.

== Numbers ==
[[File:Potentially Hazardous Asteroids 2013.png|thumb|Plot of orbits of known [[potentially hazardous asteroid]]s ]]
{{As of|2023|09}}, there are over 32,955 [[near-Earth object]]s of which roughly 1,620 near-Earth asteroids are listed on the risk table.<ref name="risk-table"/> Only around 19 objects on the risk table are large enough to qualify as potentially hazardous objects with a diameter greater than 140 meters ([[Absolute magnitude#Solar System bodies (H)|absolute magnitude]] brighter than 22). About 99% of the objects on the risk table are less than roughly 140 meters in diameter. Roughly 1,200 of these risk-listed near-Earth asteroids are estimated to be about the size of the [[Chelyabinsk meteor]] (H>26), which killed no one but had 1,491 non-direct injuries; or smaller. More than 3,140 asteroids have been removed from the risk table since it launched in 2002.<ref name="removed"/>

The only two comets that briefly appeared on the Sentry Risk Table are 197P/LINEAR (2003 KV2) and [[300P/Catalina]] (2005 JQ5).<ref name="removed"/>

== JPL SBDB comparison ==
The [[JPL Small-Body Database]] close approach table lists a [[Linearity|linearized]] uncertainty. Sentry computations explore alternate orbit solutions along the line of variations and account for orbit propagation nonlinearities.

== Scout ==
Sentry's little brother Scout scans recently detected objects on the Minor Planet Center's [[Near-Earth Object Confirmation Page]] with designations that are user-assigned and unofficial as they have not been confirmed by additional observations.<ref name="Scout-intro"/> The impact risk assessment is rated on a scale of 0–4 (negligible, small, modest, moderate, or elevated).<ref group="note">"Negligible" (0) is for objects where no impacting solution was identified. "Small" (1) is for objects with a <0.1% chance of impact. "Modest" (2) is for a 0.1-1% chance. "Moderate" (3) is for a 1-10% chance, and "Elevated" (4) is for a >10% chance of impact.</ref> Scout is used to help identify imminent impactors.

==See also==
* [[Asteroid impact prediction]]
* [[Earth-grazing fireball]]
* [[Impact event]]
* [[List of asteroid close approaches to Earth]]
* [[List of Earth-crossing asteroids]]
* [[Meteoroid]]
* [[NEODyS]]
* [[Time-domain astronomy]]

==Notes==
{{reflist|group="note"}}


== References ==
== References ==
{{reflist
{{Reflist
| refs =
| refs =


<ref name="risk-table">{{cite web
<ref name="risk-table">{{cite web
|date=14 Oct 2011
|title=Sentry Risk Table
|title=Sentry Risk Table
|publisher=NASA/JPL Near-Earth Object Program Office
|publisher=NASA/JPL Near-Earth Object Program Office
|url=http://neo.jpl.nasa.gov/risk/
|url=https://cneos.jpl.nasa.gov/sentry/
|access-date=2017-04-13}} (Click "Use Unconstrained Settings" to see how many objects are on the list; H<=22 for list of PHAs)</ref>
|accessdate=2011-10-14}}</ref>


<ref name="Giorgini">{{cite web
<ref name="Giorgini">{{cite web
Line 26: Line 108:
|author=Jon Giorgini
|author=Jon Giorgini
|url=http://www.hohmanntransfer.com/by/giorgjon.htm
|url=http://www.hohmanntransfer.com/by/giorgjon.htm
|archive-url=https://web.archive.org/web/20021208202559/http://www.hohmanntransfer.com/by/giorgjon.htm
|accessdate=2011-11-21}}</ref>
|url-status=dead
|archive-date=8 December 2002
|access-date=2011-11-21}}</ref>


<ref name="intro">{{cite web
<ref name="intro">{{cite web
|date=31 Aug 2005
|date=31 Aug 2005
|title=IMPACT RISK ASSESSMENT: AN INTRODUCTION
|title=IMPACT RISK ASSESSMENT: AN INTRODUCTION
|publisher=NASA/JPL Near-Earth Object Program Office
|publisher=NASA/JPL Near-Earth Object Program Office
|url=http://neo.jpl.nasa.gov/risk/doc/sentry.html
|url=http://neo.jpl.nasa.gov/risk/doc/sentry.html
|archive-url=https://web.archive.org/web/20020419174057/http://neo.jpl.nasa.gov/risk/doc/sentry.html
|accessdate=2011-10-14}}</ref>
|url-status=dead
|archive-date=19 April 2002
|access-date=2011-10-14}}</ref>


<ref name="NYT-20130209">{{cite web
<ref name="notes">{{cite web
|title=Sentry Notes
|date=9 February 2013
|publisher=NASA/JPL Near-Earth Object Program Office
|title=Beware of Errant Asteroids
|date=2013-08-12
|publisher=[[New York Times]]
|author=[http://solarsystem.nasa.gov/deepimpact/science/dyeomans.cfm Donald K. Yeomans]
|url=https://cneos.jpl.nasa.gov/sentry/notes.html
|access-date=2017-04-13}}</ref>
|url=http://www.nytimes.com/2013/02/10/opinion/sunday/beware-of-errant-asteroids.html
|accessdate=10 February 2013 }}</ref>


<ref name="removed">{{cite web
}}
|title = Removed Objects
|publisher = NASA/JPL Near-Earth Object Program Office
|url = http://cneos.jpl.nasa.gov/sentry/removed.html
|archive-url = https://archive.today/20170225212225/http://cneos.jpl.nasa.gov/sentry/removed.html
|archive-date = 2017-02-25
|url-status = live
|access-date = 2017-02-16
}}(Search for "P/" to list comets removed.)</ref>

<ref name="Scout-intro">{{cite web
|title=Scout: NEOCP Hazard Assessment
|publisher=NASA/JPL Near-Earth Object Program Office
|url=https://cneos.jpl.nasa.gov/scout/intro.html
|access-date=2019-06-26}}</ref>

<ref name="Sentry2002">{{cite web
|title=2002 Archive of Sentry Risk Table
|url=http://neo.jpl.nasa.gov/risk/ |archive-url=https://web.archive.org/web/20020321092735/http://neo.jpl.nasa.gov/risk/ |url-status=dead |archive-date=2002-03-21 }}</ref>

<ref name="NEODyS2023">{{cite web
|title=2005ED224 Ephemerides for March 2023
|publisher=NEODyS (Near Earth Objects{{Snd}} Dynamic Site)
|url=https://newton.spacedys.com/neodys/index.php?pc=1.1.3.1&n=2005ED224&oc=500&y0=2023&m0=3&d0=10&h0=0&mi0=0&y1=2023&m1=3&d1=12&h1=0&mi1=0&ti=1.0&tiu=days
|access-date=2021-03-26}} (Having not been observed since 2005 with an orbital period of 2.6±0.3 years, we do not know where on its orbit 2005 ED224 is.)</ref>

<ref name=velocity>{{cite web
|title=Sentry Risk Table: 2015 RD36
|type=using 2022-Sep-13 solution
|publisher=NASA JPL [[Center for Near-Earth Object Studies|CNEOS]]
|url=https://cneos.jpl.nasa.gov/sentry/details.html#?des=2015%20RD36
|access-date=2022-10-02 }}</ref>

<ref name="VIs">{{cite web
|title=VI (Virtual Impactor) Data
|publisher=NASA/JPL Near-Earth Object Program Office
|url=https://cneos.jpl.nasa.gov/sentry/vi.html
|access-date=2022-11-09}} Unconstrained Settings, Sort by Date. For objects larger than the [[Chelyabinsk meteor]] and better than 1:1 million also include Impact Probability ≥ 1e-6 and H≤26 (17–38 meters).</ref>

<ref name="Horizons2023">{{cite web
|title=Horizons Batch for 2023-06-10 Virtual Impactor
|publisher=[[JPL Horizons On-Line Ephemeris System|JPL Horizons]]
|url=https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%272016+LP10%27&START_TIME=%272023-06-10%27&STOP_TIME=%272023-06-11%27&STEP_SIZE=%272%20day%27&QUANTITIES=%2720,39%27
|archive-url=https://web.archive.org/web/20221109223456/https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%272016+LP10%27&START_TIME=%272023-06-10%27&STOP_TIME=%272023-06-11%27&STEP_SIZE=%272%20day%27&QUANTITIES=%2720,39%27
|archive-date=2022-11-09
|url-status=live
|accessdate=2021-11-09}} RNG_3sigma = uncertainty range in km. (JPL#4/Soln.date: 2021-Apr-15 generates RNG_3sigma = {{val|134116335|u=km}} for 2023-Jun-10.)</ref>

<ref name=Horizons2022PX1>{{cite web
|title=JPL Horizons: 2022 PX1 geocentric distance and uncertainty on 11 August 2040
|publisher=JPL Horizons
|url=https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%272022+PX1%27&START_TIME=%272040-Aug-11%27&STOP_TIME=%272040-Aug-12%27&STEP_SIZE=%272%20day%27&QUANTITIES=%2720,39%27
|accessdate=2023-03-15}}</ref>

<ref name="Sentry-II">{{cite web
|title=NASA's Next-Generation Asteroid Impact Monitoring System Goes Online
|publisher=NASA/JPL Near-Earth Object Program Office
|url=https://www.jpl.nasa.gov/news/nasas-next-generation-asteroid-impact-monitoring-system-goes-online
|date=2021-12-06}}</ref>

}} <!-- end of reflist -->


==External links==
==External links==
* [http://neo.jpl.nasa.gov/news/news126.html SENTRY - An Automatic Near-Earth Asteroid Collision Monitoring System]@ neo.jpl.nasa.gov
* [https://cneos.jpl.nasa.gov/sentry/intro.html Sentry: Introduction]
* [http://neo.jpl.nasa.gov/risk/doc/sentry.html IMPACT RISK ASSESSMENT: AN INTRODUCTION]
* [https://cneos.jpl.nasa.gov/sentry/ Sentry: Impact Risk Data table]
* List of [https://cneos.jpl.nasa.gov/sentry/removed.html objects for which all previously detected potential impacts have been eliminated]
* [http://neo.jpl.nasa.gov/risk/ Sentry Risk Table]
* Similar lists: [https://newton.spacedys.com/neodys/index.php?pc=4.1 NEODyS CLOMON2] / [https://neo.ssa.esa.int/risk-list ESA NEO Risk List] / [http://www.brera.mi.astro.it/sormano/teca.html Sormano Observatory TECA] / [https://robertinventor.online/booklets/sentry_table_simplified.htm Simplified List]
* [http://newton.dm.unipi.it/neodys/index.php?pc=4.1 NEODyS CLOMON2]
* [https://www.youtube.com/watch?v=8M_27st1ZCI&t=142 Asteroid Hazards, Part 3: Finding the Path] – [[Minor Planet Center]] on YouTube
* List of [http://neo.jpl.nasa.gov/risk/removed.html objects for which all previously detected potential impacts have been eliminated]
* [https://cneos.jpl.nasa.gov/scout/intro.html Scout: NEOCP Hazard Assessment: Introduction]


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Latest revision as of 14:56, 13 October 2023

Asteroid 2020 VV risk corridor for the obsolete virtual impactor of 12 October 2033.

Sentry is a highly automated impact prediction system operated by the JPL Center for NEO Studies (CNEOS) since 2002. It continually monitors the most up-to-date asteroid catalog for possibilities of future impact with Earth over the next 100+ years.[1] Whenever a potential impact is detected it will be analyzed and the results immediately published by the Center for Near-Earth Object Studies.[1] However, several weeks of optical data are not enough to conclusively identify an impact years in the future.[2] By contrast, eliminating an entry on the risk page is a negative prediction (a prediction of where it will not be).[2]

Scientists warn against worrying about the possibility of impact with an object based on only a few weeks of optical data that show a possible Earth encounter years from now.[2] Sometimes, it cannot even be said for certain what side of the Sun such an object will be at the time of the listed virtual impactor date.[2] For example, even though 2005 ED224 had a 1-in-500,000 chance of impacting Earth on 11 March 2023, it was expected to be farther than the Sun at the time.[3] Most objects on the Sentry Risk Table have an observation arc of less than 14 days and have not been observed for years.

There are 1620 near-Earth asteroids listed on the risk table with 37,736 virtual impactor dates. For each asteroid listed on the risk table there are on average about 23 virtual impactors. Only about 19 objects on the risk list are large enough to be considered potentially hazardous objects with a diameter greater than about 140 meters. The average size of an object on the default page of Sentry is 120 meters with an average impact probability of 1:500. More eccentric orbits (such as 2015 RD36) that extend to nearly the orbit of Jupiter can make atmospheric entry at velocities of ~40 km/s (25 mi/s).[4]

Sentry Risk Table[edit]

Objects with better than a 1/500 (0.2%) cumulative chance of impact
Object Cumulative
Impact
Probability
Date of
Greatest Risk
Estimated
Diameter
(meters)
Observation
arc

(days)
2010 RF12 10% 2095-09-05 7 4374
2020 CD3 2.5% 2082-09-09 2 742
2006 RH120 1.3% 2044-02-08 4 281
2017 WT28 1.2% 2104-11-24 8 19
2020 VW 0.70% 2074-11-02 7 14
2006 JY26 0.50% 2074-05-03 7 3
2020 CQ1 0.46% 2070-02-03 6 29
2022 SX55 0.40% 2035-09-17 3 1
2022 NX1 0.32% 2075-12-03 8 142
2000 SG344 0.27% 2071-09-16 37 507
2022 YO1 0.23% 2024-12-17 3 1
2020 VV 0.23% 2056-10-11 12 61
2017 LD 0.22% 2079-06-10 11 45
2000 LG6 0.21% 2094-05-27 5 2

The Impact Risk page lists a number of lost minor planets that are, for all practical purposes, permanent residents of the risk page; their removal may depend upon a serendipitous rediscovery.[5] Lost asteroid 1979 XB has been on the list since the list's inception.[6] 2007 FT3 and 2014 MV67 with their very short 1-day observation arcs have missed virtual impactor dates as they were likely quite distant from the Earth at the time. 1997 XR2 was serendipitously rediscovered in 2006 after being lost for more than 8 years. 2004 BX159 was determined to be a harmless main belt asteroid in 2014. Some objects on the Sentry Risk Table, such as 2000 SG344, might even be artificial.[7]

2010 RF12 is the asteroid with greatest probability (10%) of impacting Earth, but is only ~7 meters in diameter. The only numbered objects with observation arcs of several years are (29075) 1950 DA and 101955 Bennu.[1] Notable asteroids removed from Sentry include (most recently removed listed first): 99942 Apophis, (410777) 2009 FD, 2006 QV89, 2017 XO2, 1994 WR12, 2007 VK184, 2013 BP73, 2008 CK70, 2013 TV135, 2011 BT15, 367943 Duende, and 2011 AG5.

Of the 160 asteroids with better than a 1-in-10,000 chance of impacting Earth only 101955 Bennu is larger than 50 meters in diameter.

The soonest virtual impactor of an asteroid larger than 50 meters in diameter with a better than 1:1-million chance of impact is 2022 PX1 on 11 August 2040 with a 1:330000 chance of impact.[8] It is estimated to be 120-meters in diameter, has a short observation arc of 3.1-days, and is expected to be 1.78 AU (266 million km) from Earth on 11 August 2040.[9] The impact scenario is outside the 3-sigma uncertainty region of ± 240 million km.

The asteroid with the greatest chance of impacting Earth in 2023 is 2016 LP10 (4-meters in diameter) with less than a 1-day observation arc.[8] It had a 1:53,000 chance of impact on 10 June 2023, but was expected to be around 0.6 AU (90 million km) from Earth on that date.[10] Such an impact would be similar to 2008 TC3.

With a 24-day observation arc, 2017 SA20 has the most virtual impactors with 1244 virtual impactor dates.[1][11]

The diameter of most near-Earth asteroids that have not been studied by radar or infrared can generally only be estimated within about a factor of 2 based on the asteroid's absolute magnitude (H).[1] Their mass, consequently, is uncertain by about a factor of 10. For near-Earth asteroids without a well-determined diameter, Sentry assumes a generic albedo of 0.15.

In August 2013, the Sentry Risk Table started using planetary ephemeris (DE431) for all NEO orbit determinations.[12] DE431 (JPL small-body perturber ephemeris: SB431-BIG16) better models the gravitational perturbations of the planets and includes the 16 most massive main-belt asteroids.[12] In April 2021, Sentry transitioned to DE441 which removed the very low impact probability of short-arc 2014 MV67 which had been less than 1:1-billion. The switch to DE441 also briefly added in the harmless Jupiter trojan 2014 ES57 with a very low impact probability of about 1:1-billion.

JPL launched major changes to the website in February 2017 and re-directed the classic page on 10 April 2017.

In 2021 JPL launched Sentry-II which handles the Yarkovsky effect that can significantly change a small asteroids path over decades and centuries.[13] Sentry-II defaults to an Impact Pseudo-Observation (IOBS) analysis technique that runs an extended orbit-determination filter that tries to converge to an impacting solution compatible with the observational data.

Numbers[edit]

Plot of orbits of known potentially hazardous asteroids

As of September 2023, there are over 32,955 near-Earth objects of which roughly 1,620 near-Earth asteroids are listed on the risk table.[1] Only around 19 objects on the risk table are large enough to qualify as potentially hazardous objects with a diameter greater than 140 meters (absolute magnitude brighter than 22). About 99% of the objects on the risk table are less than roughly 140 meters in diameter. Roughly 1,200 of these risk-listed near-Earth asteroids are estimated to be about the size of the Chelyabinsk meteor (H>26), which killed no one but had 1,491 non-direct injuries; or smaller. More than 3,140 asteroids have been removed from the risk table since it launched in 2002.[14]

The only two comets that briefly appeared on the Sentry Risk Table are 197P/LINEAR (2003 KV2) and 300P/Catalina (2005 JQ5).[14]

JPL SBDB comparison[edit]

The JPL Small-Body Database close approach table lists a linearized uncertainty. Sentry computations explore alternate orbit solutions along the line of variations and account for orbit propagation nonlinearities.

Scout[edit]

Sentry's little brother Scout scans recently detected objects on the Minor Planet Center's Near-Earth Object Confirmation Page with designations that are user-assigned and unofficial as they have not been confirmed by additional observations.[15] The impact risk assessment is rated on a scale of 0–4 (negligible, small, modest, moderate, or elevated).[note 1] Scout is used to help identify imminent impactors.

See also[edit]

Notes[edit]

  1. ^ "Negligible" (0) is for objects where no impacting solution was identified. "Small" (1) is for objects with a <0.1% chance of impact. "Modest" (2) is for a 0.1-1% chance. "Moderate" (3) is for a 1-10% chance, and "Elevated" (4) is for a >10% chance of impact.

References[edit]

  1. ^ a b c d e f "Sentry Risk Table". NASA/JPL Near-Earth Object Program Office. Retrieved 13 April 2017. (Click "Use Unconstrained Settings" to see how many objects are on the list; H<=22 for list of PHAs)
  2. ^ a b c d Jon Giorgini (30 July 2002). "Understanding Risk Pages". Columbine, Inc. (hohmanntransfer). Archived from the original on 8 December 2002. Retrieved 21 November 2011.
  3. ^ "2005ED224 Ephemerides for March 2023". NEODyS (Near Earth Objects – Dynamic Site). Retrieved 26 March 2021. (Having not been observed since 2005 with an orbital period of 2.6±0.3 years, we do not know where on its orbit 2005 ED224 is.)
  4. ^ "Sentry Risk Table: 2015 RD36" (using 2022-Sep-13 solution). NASA JPL CNEOS. Retrieved 2 October 2022.
  5. ^ "IMPACT RISK ASSESSMENT: AN INTRODUCTION". NASA/JPL Near-Earth Object Program Office. 31 August 2005. Archived from the original on 19 April 2002. Retrieved 14 October 2011.
  6. ^ "2002 Archive of Sentry Risk Table". Archived from the original on 21 March 2002.
  7. ^ "Much Ado about 2000 SG344". NASA Science. NASA. Retrieved 27 September 2023.
  8. ^ a b "VI (Virtual Impactor) Data". NASA/JPL Near-Earth Object Program Office. Retrieved 9 November 2022. Unconstrained Settings, Sort by Date. For objects larger than the Chelyabinsk meteor and better than 1:1 million also include Impact Probability ≥ 1e-6 and H≤26 (17–38 meters).
  9. ^ "JPL Horizons: 2022 PX1 geocentric distance and uncertainty on 11 August 2040". JPL Horizons. Retrieved 15 March 2023.
  10. ^ "Horizons Batch for 2023-06-10 Virtual Impactor". JPL Horizons. Archived from the original on 9 November 2022. Retrieved 9 November 2021. RNG_3sigma = uncertainty range in km. (JPL#4/Soln.date: 2021-Apr-15 generates RNG_3sigma = 134116335 km for 2023-Jun-10.)
  11. ^ Sentry: 2017 SA20 (1244 VIs) using 2022-Aug-30 solution
  12. ^ a b "Sentry Notes". NASA/JPL Near-Earth Object Program Office. 12 August 2013. Retrieved 13 April 2017.
  13. ^ "NASA's Next-Generation Asteroid Impact Monitoring System Goes Online". NASA/JPL Near-Earth Object Program Office. 6 December 2021.
  14. ^ a b "Removed Objects". NASA/JPL Near-Earth Object Program Office. Archived from the original on 25 February 2017. Retrieved 16 February 2017.(Search for "P/" to list comets removed.)
  15. ^ "Scout: NEOCP Hazard Assessment". NASA/JPL Near-Earth Object Program Office. Retrieved 26 June 2019.

External links[edit]