Constructing ballistic capture orbits in the real Solar System model

Along with the development, the application can be used as a medium for learning. Augmented Reality is a technology that combines two-dimensional’s virtual objects and three-dimensional’s virtual objects into a real three-dimensional’s then projecting the virtual objects in real time and simultaneously. The introduction of Solar System’s material, students are invited to get to know the planets which are directly encourage students to imagine circumtances in the Solar System. Explenational of planets form and how the planets make the revolution and rotation in books are considered less material’s explanation because its only display objects in 2D. In addition, students can not practice directly in preparing the layout of the planets in the Solar System. By applying Augmented Reality Technology, information’s learning delivery can be clarified, because in these applications are combined the real world and the virtual world. Not only display the material, the application also display images of planets in 3D animation’s objects with audio.

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Implementasi Metode Luther untuk Pengembangan Media Pengenalan Tata Surya Berbasis Virtual Reality

BIOS : Jurnal Teknologi Informasi dan Rekayasa Komputer ◽

10.37148/bios.v1i1.3 ◽

2020 ◽

Vol 1 (1) ◽

pp. 1-14

Author(s):

Adhe Pandhu Dwi Prayogha ◽

Mudafiq Riyan Pratama

Keyword(s):

Virtual Reality ◽

Solar System ◽

Real World ◽

Multimedia Applications ◽

Concept Design ◽

The Real ◽

3 Dimensional ◽

3D Objects ◽

Artificial World ◽

Virtual Reality Application

The purpose of virtual reality is to enable a motor and cognitive sensor activity ofsomeone in the artificial world created digitally to become imaginary, symbolic orsimulate certain aspects in the real world [1]. This technology is applied to the mediaintroduction of the solar system using the Luther method. The Luther Method consistsof 6 stages, namely Concept, Design, Material Collecting, Assembly, Testing, andDistribution. Luther method has advantages compared to other methods because thereare stages of material collecting which is an important stage in the development ofmultimedia and this Luther method can be done in parallel or can go back to theprevious stage [2]. At the Assembly stage the implementation uses the Unity Engineand Google VR SDK for Unity, the result is a virtual reality application that can displaythe solar system with 3-dimensional objects and an explanation is available on eachobject. While testing the blackbox on a variety of Android devices with differentspecifications. From the results of the application of the Luther method, it is verystructured and can run well in the development of multimedia applications, while theresults of testing, this Android-based virtual reality application cannot run on devicesthat do not have Gyroscope sensors and can run on devices with a minimumspecification of 1GB RAM will but the rendering process on 3D objects is slow.

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Load-sharing system model and its application to the real data set

Mathematics and Computers in Simulation ◽

10.1016/j.matcom.2012.02.010 ◽

2012 ◽

Vol 82 (9) ◽

pp. 1615-1629 ◽

Cited By ~ 34

Author(s):

Bhupendra Singh ◽

Puneet Kumar Gupta

Keyword(s):

Real Data ◽

Load Sharing ◽

System Model ◽

Data Set ◽

The Real

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A note on the dynamics around the Lagrange collinear points of the Earth–Moon system in a complete Solar System model

Celestial Mechanics and Dynamical Astronomy ◽

10.1007/s10569-012-9459-2 ◽

2013 ◽

Vol 115 (2) ◽

pp. 185-211 ◽

Cited By ~ 16

Author(s):

Yijun Lian ◽

Gerard Gómez ◽

Josep J. Masdemont ◽

Guojian Tang

Keyword(s):

Solar System ◽

System Model ◽

Moon System ◽

The Earth

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Can narrow discs in the inner Solar system explain the four terrestrial planets?

Monthly Notices of the Royal Astronomical Society ◽

10.1093/mnras/staa1625 ◽

2020 ◽

Vol 496 (3) ◽

pp. 3688-3699 ◽

Cited By ~ 1

Author(s):

Patryk Sofia Lykawka

Keyword(s):

Solar System ◽

Planet Formation ◽

Terrestrial Planet ◽

Giant Planets ◽

System Model ◽

Terrestrial Planets ◽

P System ◽

Orbital Mass ◽

System A ◽

System 2

ABSTRACT A successful Solar system model must reproduce the four terrestrial planets. Here, we focus on (1) the likelihood of forming Mercury and the four terrestrial planets in the same system (a 4-P system); (2) the orbital properties and masses of each terrestrial planet; and (3) the timing of Earth’s last giant impact and the mass accreted by our planet thereafter. Addressing these constraints, we performed 450 N-body simulations of terrestrial planet formation based on narrow protoplanetary discs with mass confined to 0.7–1.0 au. We identified 164 analogue systems, but only 24 systems contained Mercury analogues, and eight systems were 4-P ones. We found that narrow discs containing a small number of embryos with individual masses comparable to that of Mars and the giant planets on their current orbits yielded the best prospects for satisfying those constraints. However, serious shortcomings remain. The formation of Mercury analogues and 4-P systems was too inefficient (5 per cent and 2 per cent, respectively), and most Venus-to-Earth analogue mass ratios were incorrect. Mercury and Venus analogues also formed too close to each other (∼0.15–0.21 au) compared to reality (0.34 au). Similarly, the mutual distances between the Venus and Earth analogues were greater than those observed (0.34 versus 0.28 au). Furthermore, the Venus–Earth pair was not reproduced in orbital-mass space statistically. Overall, our results suggest serious problems with using narrow discs to explain the inner Solar system. In particular, the formation of Mercury remains an outstanding problem for terrestrial planet formation models.

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Secular Perturbations on the Minor Bodies of the Solar System

Symposium - International Astronomical Union ◽

10.1017/s0074180900006884 ◽

1972 ◽

Vol 45 ◽

pp. 440-440

Author(s):

I. V. Galibina

Keyword(s):

Solar System ◽

Meteor Stream ◽

The Real ◽

Secular Perturbations ◽

Meteor Streams ◽

The Earth ◽

The Stability ◽

Osculating Elements ◽

First Time

By means of the Gauss-Halphen-Goryachev method secular orbital variations have been studied for a period of 4000 yr (from −50 to +3950). The method has been applied to the periodic comets Halley, Brorsen-Metcalf, Pons-Brooks, Westphal, Olbers, Neujmin 1, and Encke. Investigations have demonstrated that the use of the method for most comets is not expedient as it does not allow for the possibility of approaches to the major planets and thus does not reflect the real evolution of the cometary orbits. Application of the method over the interval of 2000 years back from the epoch 1950.0 for the planets 279 Thule, 1162 Larissa, 1180 Rita, and 1202 Marina, as well as from the epoch 1850.0 for 1 Ceres has given adequate results and has displayed the stability of these orbits. Study of the secular perturbations on the Leonids over the interval of 4000 yr has confirmed the stability of that meteor stream. By means of the same method 14 minor meteor streams were investigated, and their orbits also proved to be stable. The availability of the various systems of osculating elements has permitted us to estimate for the first time the possibility of the encounter of those streams with the Earth over a 4000-yr period. For further details see Galibina (1970a, 1970b, 1971).

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Reply: The Solar System Model for the Reconstructive Ladder

Plastic & Reconstructive Surgery ◽

10.1097/prs.0b013e3182173e8d ◽

2011 ◽

Vol 128 (1) ◽

pp. 337-338 ◽

Cited By ~ 1

Author(s):

Karsten Knobloch ◽

Peter M. Vogt

Keyword(s):

Solar System ◽

System Model ◽

Reconstructive Ladder

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A Research on Suppression of SSO Based on the Real Time Digital Simulation

Advanced Materials Research ◽

10.4028/www.scientific.net/amr.732-733.1415 ◽

2013 ◽

Vol 732-733 ◽

pp. 1415-1419 ◽

Cited By ~ 1

Author(s):

Chun Lin Guo ◽

Jian Ting Xu ◽

Yang Zhao ◽

Xiang Ning Xiao

Keyword(s):

Real Time ◽

Digital Simulation ◽

Operation Mode ◽

System Model ◽

The Real ◽

Model Based ◽

Operation Modes ◽

Simulation Results

According to the first project using SVC to mitigate SSO in China, this paper builds the system model based on real time digtal simulator,and gives an introduction to the sysem model. Under typical operation mode and fault conditions,the performance of SVC is fully validated,it also analysis and comparise the performance of SVC under different operation modes. Simulation results show that the SVC can mitigate the SSO phenomenon.

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