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Parameter introduced by the Minor Planet Center
The uncertainty parameter U is introduced by the Minor Planet Center (MPC) to quantify the uncertainty of a perturbed orbital solution for a minor planet
Uncertainty_parameter
Science of characterizing uncertainties
One way to categorize the sources of uncertainty is to consider: Parameter This comes from the model parameters that are inputs to the computer model
Uncertainty_quantification
Foundational principle in quantum physics
The uncertainty principle, also known as Heisenberg's indeterminacy principle, is a fundamental concept in quantum mechanics. It states that there is
Uncertainty_principle
Effect of variables' uncertainties on the uncertainty of a function based on them
In statistics, propagation of uncertainty is the effect of variables' uncertainties on the uncertainty of a function based on them. When the variables
Propagation_of_uncertainty
Factor of lower probability in measurement
agreement, this uncertainty has a probabilistic basis and reflects incomplete knowledge of the quantity value. It is a non-negative parameter. The measurement
Measurement_uncertainty
Situations involving imperfect or unknown information
Uncertainty or incertitude refers to situations involving imperfect or unknown information. It applies to predictions of future events, to physical measurements
Uncertainty
Study of uncertainty in the output of a mathematical model or system
model inputs are subject to sources of uncertainty, including errors of measurement, errors in input data, parameter estimation and approximation procedure
Sensitivity_analysis
System of geographic location identifiers
"uncertainty" value, separated by a semicolon, representing the uncertainty of the location in meters, and is described using the "u" URI parameter. A
Geo_URI_scheme
Small near-Earth asteroid
related to 2025 PN7. 2025 PN7 at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
2025_PN7
Near-Earth asteroid
Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters Portals: Astronomy Spaceflight Solar System
2026_JH2
Concept in celestial mechanics
gravitational parameter μ of a celestial body is the product of the gravitational constant G and the mass M of that body. For two bodies, the parameter may be
Standard gravitational parameter
Standard_gravitational_parameter
Time between earliest and latest observations of a Solar System body
timestamps have a lesser effect. A very short arc leaves a high uncertainty parameter. The object might be in one of many different orbits, at many distances
Observation_arc
Main-belt asteroid
Observational info 224 Oceana at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters v t e
224_Oceana
Lack of quantifiable knowledge in economics
In economics, Knightian uncertainty is a lack of any quantifiable knowledge about some possible occurrence, as opposed to the presence of quantifiable
Knightian_uncertainty
Potentially hazardous near-Earth asteroid
Apophis has no chance of impacting Earth in the next 100 years. The uncertainty in the 2029 approach distance has been reduced from hundreds of kilometres
99942_Apophis
Branch of applied probability theory
and probability to model how individuals would behave rationally under uncertainty. It differs from the cognitive and behavioral sciences in that it is
Decision_theory
Variable used for specification
A parameter (from Ancient Greek παρά (pará) 'beside, subsidiary' and μέτρον (métron) 'measure'), generally, is any characteristic that can help in defining
Parameter
Sednoid
2025. (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 1-sigma from JPL Small-Body Database.) Chen
2023_KQ14
Plutino with a thin atmosphere
Summary (612533) 2002 XV93 at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
(612533)_2002_XV93
First known asteroid of the Vatira population
the Palomar and Xingming observatories, reducing ꞌAylóꞌchaxnim's uncertainty parameter to 5. Upon discovery, the asteroid was given the internal designation
594913_ꞌAylóꞌchaxnim
Main-belt asteroid
determination of the asteroid well enough to give it an orbital uncertainty parameter of 0 by the Minor Planet Center. Although the asteroid first appeared
718492_Quro
for various sources of uncertainty in model input and design. A related field is sensitivity analysis. A calibrated parameter does not necessarily represent
Uncertainty_analysis
Distant body in the outer Solar System
is not expected to have a substantial atmosphere. Within the range of uncertainty, it is tied with Ceres in the asteroid belt as the largest dwarf planet
Sedna_(dwarf_planet)
Framework for modeling optimization problems that involve uncertainty
optimization problems that involve uncertainty. A stochastic program is an optimization problem in which some or all problem parameters are uncertain, but follow
Stochastic_programming
Small risk–listed near-Earth asteroid
distance and uncertainty on 2028-May-07". JPL Horizons. Retrieved 10 June 2023. "JPL Horizons: 2000 SG344 geocentric distance and uncertainty on 2030-Sep-22"
2000_SG344
Large trans-Neptunian object in the scattered disc
2025. Perihelion occurs when r‑dot flips from negative to positive (uncertainty region is 2.4 million km or 0.016 AU) "Asteroid size estimator". Center
2017_OF201
Factor in X-ray crystallography
In X-ray crystallography, the Flack parameter is a factor used to estimate the absolute configuration of a structural model determined by single-crystal
Flack_parameter
Postpositivist communication theory developed in 1975
The uncertainty reduction theory (URT), also known as initial interaction theory, developed in 1975 by Charles Berger and Richard Calabrese, is a communication
Uncertainty_reduction_theory
Risk-listed near-Earth asteroid
March 2025 indicate that it has a diameter of 60 m (200 ft), with an uncertainty of 7 m (23 ft). This makes 2024 YR4 around the same size as the asteroid
2024_YR4
Sub-kilometer-sized asteroid
pass of less than 30 million km in this century. JPL shows that the uncertainty region of the asteroid will cause it to most likely pass from 0.02 AU
4581_Asclepius
Scattered disc object
2014 UZ224 has not been numbered by the Minor Planet Center, as the uncertainty of its orbit is still large. The discoverers will have sole right to
2014_UZ224
Main-belt asteroid
designation 2017 BX232 was assigned to the object. After its orbital uncertainty parameter dropped to 0, the asteroid was numbered (697402). Discovery credit
697402_Ao
Standard unit of mass for atomic-scale entities
2007-12-09. "2022 CODATA Value: lattice parameter of silicon". The NIST Reference on Constants, Units, and Uncertainty. NIST. May 2024. Retrieved 2024-05-18
Dalton_(unit)
Trans-Neptunian object
Xewioso are unknown and its absolute magnitude also has significant uncertainty. Based on its size of 565+71 −73 km, it belongs to the proposed class
78799_Xewioso
Extreme trans-Neptunian object from the inner Oort cloud
@sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.) Michael E. Brown. "How many dwarf
2014_FE72
Large main-belt asteroid
Observational info 259 Aletheia at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
259_Aletheia
Trans-Neptunian object
the Minor Planet Center due to its short observation arc and orbital uncertainty. 2018 AG37 will be given a minor planet number when its orbit is well-secured
2018_AG37
Third-largest asteroid
pointing towards ecliptic coordinates (β, λ) = (30°, −16°) with a 5° uncertainty in the Ecliptic J2000.0 reference frame. This means that every Palladian
2_Pallas
Classical Kuiper belt object
in June 2003. These recovery observations significantly reduced the uncertainty of Máni's orbit, allowing for further extrapolation of its position backwards
307261_Máni
Physics generalization
the uncertainties in position and momentum, ℏ {\displaystyle \hbar } is the reduced Planck constant, and β {\displaystyle \beta } is a parameter related
Generalized uncertainty principle
Generalized_uncertainty_principle
Dwarf planet in the Kuiper belt
10 km (6.2 mi). Makemake has a bulk density of about 1.76 g/cm3 (with an uncertainty of ±0.17 g/cm3), similar to the trans-Neptunian dwarf planets Pluto,
Makemake
Observation in physical cosmology
Hubble constant H0 is constant at any given moment in time, the Hubble parameter H, of which the Hubble constant is the current value, varies with time
Hubble's_law
Sednoid
@sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.) Buie, Marc W.; Leiva, Rodrigo; Keller
541132_Leleākūhonua
Asteroid
info 52246 Donaldjohanson at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
52246_Donaldjohanson
Approach to controller design that explicitly deals with uncertainty
parametric and non-parametric modeling uncertainty. Parametric uncertainty refers to the case where modeling parameters or external disturbances in feedback
Robust_control
Trans-Neptunian object, prototype of cubewanos
Observational info 15760 Albion at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
15760_Albion
Possible dwarf planet
campaigns have progressively narrowed Salacia's orbital path from an early uncertainty of about 2300 km. On 27 December 2018, an event monitored by the LESIA
120347_Salacia
Sednoid
Planet Center 2012 VP113 at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
2012_VP113
Near-Earth asteroid
properties · Summary 1998 KY26 at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
1998_KY26
Trans-Neptunian dwarf planet
submillimeter estimates its diameter at 958.4 km (595.5 mi), with an uncertainty of 22.9 km (14.2 mi). Orcus appears to have an albedo of about 21–25%
Orcus_(dwarf_planet)
Near-Earth Asteroid
mythological name. The orbit of 2020 XL5 is well known with an uncertainty parameter of 0 and a long observation arc over 8 years. The asteroid has been
(614689)_2020_XL5
Near-Earth asteroid
Summary (153591) 2001 SN263 at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
(153591)_2001_SN263
Asteroid
Observational info 1692 Subbotina at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
1692_Subbotina
Distribution of an uncertain quantity
selection. The prior distributions of model parameters will often depend on parameters of their own. Uncertainty about these hyperparameters can, in turn
Prior_probability
Small near-Earth asteroid
observation arc of 63 days, virtual clones of the asteroid that fit the uncertainty region in the known trajectory showed a 1-in-430 chance that the asteroid
2023_DZ2
Multiple simulation method for weather forecasting
techniques to represent model uncertainty have been proposed. When developing a parametrisation scheme, many new parameters are introduced to represent
Ensemble_forecasting
Near-Earth asteroid
Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters Portals: Astronomy Stars Spaceflight Outer space Solar System
433_Eros
Near-Earth asteroid of the Apollo and Alinda group
and 2016, it is listed as a potentially hazardous object. With an uncertainty parameter of 0, the orbit of Toutatis is very well determined for the next
4179_Toutatis
Range to estimate an unknown parameter
that confidence intervals quantify uncertainty in estimating parameters, while prediction intervals quantify uncertainty in forecasting future observations
Confidence_interval
Absolute dielectric permittivity of free space
0.13 parts per billion) from the former defined value is within its uncertainty (1.6×10−10, in relative terms, or 0.16 parts per billion). The historical
Vacuum_permittivity
Main-belt asteroid
Observational info 298 Baptistina at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
298_Baptistina
Lost near-Earth asteroid
127°. The object has never been confirmed by a second observatory. The uncertainty region for this asteroid is now hundreds of millions of kilometers long
1979_XB
Asteroid visited by New Horizons
Observational info 132524 APL at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
132524_APL
Dwarf planet in the scattered-disc
Pluto's moon Charon, although Gonggong's current size estimate has an uncertainty of 50 km (31 mi). Gonggong has been classified as a dwarf planet by several
Gonggong_(dwarf_planet)
Random change in the energy inside a volume
of energy in a point in space, as prescribed by Werner Heisenberg's uncertainty principle. They are minute random fluctuations in the values of the fields
Quantum_fluctuation
Binary near-Earth asteroid
Orbit animation 66391 Moshup at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
66391_Moshup
Near-Earth micro-asteroid
at Mount Lemmon. 2013 GM3 has a poorly determined orbit with an uncertainty parameter of 7, due to its short 12-day observation arc. Based on the preliminary
2013_GM3
Ringed dwarf planet in the Kuiper belt
@sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.) Proudfoot, Benjamin; Nolthenius, Richard;
Quaoar
Most hazardous risk–listed near-Earth asteroid
the measurements of angular positions; a 74-year observation arc; an uncertainty region controlled by resonance. Main-belt asteroid 78 Diana (~125 km
(29075)_1950_DA
Minor planet in the scattered disc
hard to reconcile with such celestial mechanics. This has led to some uncertainty as to the current theoretical understanding of the outer Solar System
(612911)_2004_XR190
Asteroid
original on 26 October 2022. Retrieved 26 October 2022. RNG_3sigma = uncertainty range in km. (JPL#95/Soln.date: 2022-Jul-11 generates RNG_3sigma = 5
4769_Castalia
Second object orbiting the Sun entirely within Venus's orbit
Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters Portals: Astronomy Outer Space v t e
2025_SC79
Lost risk–listed hazardous near-Earth asteroid
October 2024. Since the asteroid has a short observation arc and the uncertainty in the orbit of the asteroid intersects Earth's orbit, simulations could
2007_FT3
S-type asteroid in the inner asteroid belt with stony mineralogical composition
campaign was implemented by the Galileo spacecraft team to reduce the uncertainty of Gaspra's position using images captured during the approach to Gaspra
951_Gaspra
Asteroid
XE133 was recovered and now has a well established orbit with an uncertainty parameter of 0. The asteroid often makes close approaches to Earth within
2012_XE133
Near-Earth asteroid and Earth trojan
Close-Approach Data: (2010 TK7)" (2011-08-03 last obs (arc=40 days; Uncertainty=2)). Retrieved 21 January 2012. "AstDyS 2010TK7 Ephemerides for 2012"
(706765)_2010_TK7
Measure of dependence between two variables
Y} share: It measures how much knowing one of these variables reduces uncertainty about the other. For example, if X {\displaystyle X} and Y {\displaystyle
Mutual_information
Scattered disc object
has been observed 548 times, the orbit is well determined with an uncertainty parameter of 1. The object is named after Rumīna, a Roman goddess who protected
145451_Rumina
Planet
Observational info 600 Musa at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters v t e
600_Musa
Main-belt asteroid
Observational info 408 Fama at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters v t e
408_Fama
Main-belt asteroid
Observational info 46610 Bésixdouze at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
46610_Bésixdouze
Classical Kuiper belt object
@sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.) "(19521) Chaos = 1998 WH24". IAU Minor
19521_Chaos
Aten asteroid co-orbital with Earth
Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters Portals: Astronomy Stars Spaceflight Outer space Solar System
3753_Cruithne
Stony near-Earth asteroid
infrared data - Significance of the shape model and the pole orientation uncertainties". Icarus. 256: 101–116. arXiv:1504.04199. Bibcode:2015Icar..256..101H
1036_Ganymed
Large asteroid
direction of right ascension 115° or 310° and declination 55°, with a 5° uncertainty. This gives an axial tilt of about 33°.[citation needed] With an apparent
5_Astraea
Cosmological time duration
in 1965 finally brought an effective end to the remaining scientific uncertainty over the expanding universe. It was a chance result from work by two
Age_of_the_universe
Main-belt asteroid
info 583 Klotilde at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters v t e
583_Klotilde
Near-Earth asteroid
the Horizons time of closest approach giving them slightly different uncertainty regions. Horizons values are calculated using the JPL SBDB time of closest
2023_BU
Ringed centaur in the outer Solar System
dimensions. Chariklo has a synodic rotation period of 7.004 hours, with an uncertainty of 0.036 hours (2.2 minutes). Due to Chariklo's elongated shape, its
10199_Chariklo
Units, and Uncertainty. NIST. May 2024. Retrieved 2024-05-18. Planck Collaboration (2020). "Planck 2018 results. VI. Cosmological parameters (page 17:
List_of_physical_constants
Volatility, uncertainty, complexity and ambiguity in leadership
Bennis and Burt Nanus, to describe or to reflect on the volatility, uncertainty, complexity and ambiguity of general conditions and situations. The U
VUCA
Scattered disc object
(461 mi) (full range 660 to 820 km or 410 to 510 mi when including uncertainties), according to Atacama Large Millimeter Array measurements of its thermal
532037_Chiminigagua
Asteroid
Observational info 1189 Terentia at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
1189_Terentia
Near-Earth asteroid
Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters Zou, Yongliao; Xue, Changbin; Jia, Yingzhuo; Li, Mingtao; Xu
2015_XF261
Trans-Neptunian object
It will reach its perihelion of 36.7 AU on 5 September 2066 with an uncertainty rate of 3 days. As of 2020, Uni is 40 AU from the Sun. The Minor Planet
55637_Uni
Near-Earth asteroid
JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters Portals: Astronomy Outer Space
2025_TF
Given the significant uncertainty at play, the use of sensitivity analysis to apportion the output uncertainty into input parameters is crucial in the context
Applications of sensitivity analysis in epidemiology
Applications_of_sensitivity_analysis_in_epidemiology
Method for model fitting in statistics
estimates reflect only random errors in the measurements. The true uncertainty in the parameters is larger due to the presence of systematic errors, which, by
Weighted_least_squares
Main-belt asteroid
Observational info 1252 Celestia at the JPL Small-Body Database Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters
1252_Celestia
Near-Earth asteroid
hour, the trajectory is poorly constrained and the asteroid has an uncertainty parameter of 9 making long-term predictions of the asteroids position nearly
2014_LY21
UNCERTAINTY PARAMETER
UNCERTAINTY PARAMETER
Surname or Lastname
English and Irish of uncertain origin
English and Irish of uncertain origin : of uncertain origin: perhaps from a Norman nickname for a stubborn person, from Old French tirel, used of an animal which pulls on the reins, a derivative of tirer ‘to pull’.English and Irish of uncertain origin : Woulfe suggests that it may be from the personal name Thurold, Old Norse Thorvaldr, composed of the elements þórr, name of the Norse god of thunder (see Thor) + valdr ‘rule’.
Surname or Lastname
English (Kent) of uncertain derivation
English (Kent) of uncertain derivation : of uncertain derivation: it could be a topographic name for someone living in an area planted with bushes, French bussière, or a habitational name from any of various minor places in Essex, perhaps named with this word.English (Kent) of uncertain derivation : alternatively it may be a nickname for a heavy drinker, from an agent derivative of Middle English bouse(n) ‘to drink’, ‘to booze’ (from Middle Dutch bÅ«sen) or Middle English bous, boos ‘intoxicating drink’ (from Middle Dutch bÅ«se).English (Kent) of uncertain derivation : lastly, it could be an occupational name for a stockman, from a derivative of Middle English bos(e), buse ‘stall for livestock’, ‘cowstall’, ‘manger’ (from Old English bÅs).
Female
Egyptian
, an uncertain goddess.
Male
Egyptian
, an uncertain deity.
Female
Egyptian
, an uncertain goddess.
Biblical
[uncertain derivation]; olive tree
Female
Egyptian
, an uncertain goddess.
Surname or Lastname
English of much discussed but uncertain origin.
English of much discussed but uncertain origin. : of much discussed but uncertain origin. It may be from a medieval personal name, but if so the form is unclear.English of much discussed but uncertain origin. : Alternatively, it may be a nickname for a quarrelsome or deceitful person, from Middle English bar(r)et(t)e, bar(r)at ‘trouble’, ‘strife’, ‘deception’, ‘cheating’ (Old French barat ‘commerce’, ‘dealings’, a derivative of barater ‘to haggle’). It is possible that the original sense of barat survived unrecorded into Middle English as a word for a market trader; the Italian cognate Baratta has this sense. It could also be a nickname or metonymic occupational name from Old French barette ‘cap’, ‘bonnet’.
Surname or Lastname
English (Suffolk) of uncertain derivation;
English (Suffolk) of uncertain derivation; : of uncertain derivation; perhaps from a reduced form of the personal name Dominicus (see Dominick).English (Suffolk) of uncertain derivation; : alternatively, as Reaney proposes, it may be from the Breton personal name Menguy, a compound of men ‘stone’ + ki ‘dog’.
Surname or Lastname
English of uncertain origin; possibly
English of uncertain origin; possibly : of uncertain origin; possibly: habitational name from an unidentified place named with Old English hwīt ‘white’ + ēg ‘island’ or (ge)hæg ‘enclosure’.English of uncertain origin; possibly : nickname for someone with unusually pale eyes, from Middle English whit ‘white’ + eye ‘eye’.
Girl/Female
Tamil
Nischita | நீஸà¯à®šà¯€à®¤à®¾
Certainty, Confidence
Nischita | நீஸà¯à®šà¯€à®¤à®¾
Female
Egyptian
, an uncertain goddess.
Girl/Female
Tamil
Nischitha | நீஸà¯à®šà¯€à®¤à®¾Â
Certainty, Confidence
Nischitha | நீஸà¯à®šà¯€à®¤à®¾Â
Girl/Female
Hindu
Certainty, Confidence
Female
Egyptian
, an uncertain goddess.
Surname or Lastname
English of uncertain origin.
English of uncertain origin. : of uncertain origin. Perhaps a topographic name for someone who lived near a fig tree, or a metonymic occupational name for someone who sold figs, from Old French figue (Latin ficus).English of uncertain origin. : Reaney has it as a variant of Fitch.English of uncertain origin. : It may also be from an unidentified personal name.
Surname or Lastname
English of uncertain origin.
English of uncertain origin. : of uncertain origin. Reaney and Wilson cite 13th- and 14th-century examples such as Richard Averil, which they associate with the name of the month (see April; the Old French word Avrill was taken into Middle English as Averil before being altered under Latin influence to April).English of uncertain origin. : As a North American surname, it may be a habitational name from Haverhill in Suffolk, which is probably named from Old English hafri ‘oats’ + hyll ‘hill’. The traditional English pronunciation of this place name was Have-rill. Compare Avery.English of uncertain origin. : William Averill (c.1590–1635) brought his family from Worcestershire, England, to VA in 1635.
Male
Egyptian
, an uncertain deity.
Female
Egyptian
, an uncertain goddess.
Girl/Female
Hindu
Certainty, Confidence
UNCERTAINTY PARAMETER
UNCERTAINTY PARAMETER
Boy/Male
Bengali, Indian
Lord Narayana
Girl/Female
Anglo, German
Friend of the Elves
Boy/Male
Tamil
Boy/Male
Indian
Lack of difficulty
Boy/Male
Biblical
Vowing of his own accord.
Girl/Female
Gujarati, Indian
Goddess Durga
Boy/Male
Tamil
Pradynesh | பà¯à®°à®¤à¯à®¯à®¨à¯‡à®·
Budhicha Dev means Lord Ganesh
Girl/Female
Arabic, Muslim
Kind; Compassionate
Boy/Male
English
Noble or bright.
Girl/Female
American, Australian, British, Christian, English, German, Greek, Indian, Latin, Polish
Merry; Happy; Cheerful; Joyful
UNCERTAINTY PARAMETER
UNCERTAINTY PARAMETER
UNCERTAINTY PARAMETER
UNCERTAINTY PARAMETER
UNCERTAINTY PARAMETER
n.
Certainty.
adv.
In an uncertain manner.
n.
Doubt; uncertainty.
n.
That which is uncertain; something unknown.
n.
Inexactness; uncertainty; as, geographical inexactitude.
n.
Absence of confidence; uncertainty; doubt.
n.
Uncertainty of event or issue.
n.
Certainty.
n.
Uncertainty; doubtfulness; doubt.
n.
The quality or state of being uncertain.
a.
To make uncertain.
n.
Doubt; uncertainty.
n.
Uncertainty.
a.
Uncertainty; instability.
a.
Irresolute; inconsonant; variable; untrustworthy; as, an uncertain person; an uncertain breeze.
n.
Possibility; uncertainty.
n.
Uncertainty of meaning; ambiguity; indefiniteness.
v. i.
Uncertainty of condition.
pl.
of Uncertainty
n.
Doubtfulness; uncertainty; doubt.