Summary Of The Lord Is Salvation - 1212 Words

His name was Hoshe a (â€Å"Salvation†) the son of Nun, of the tribe of Ephraim, but Moses went and renamed him Yehoshu a (â€Å"The Lord is Salvation†) or as in North American cultures traditionally known as Joshua (Numbers 13:16, NRSV). Joshua is a great leader from the bible he really shows how being faithful to God will end in complete success for you. I think it important to note, that just because he is a man in the bible and known as a great leader, Joshua was only human he let doubt settle in at times and wasn’t as some would say â€Å"super human† he had faults just like us and was not perfect. The book of Joshua is a great example that Yahweh is a promise-keeping God even if He works on His own time and in His own way. For example the Promise land was promised to the Israelites back in Genesis 15:18-21 where God states: â€Å"To your descendants I have given this land, from the river of Egypt as far as the great river the Euphrates. The lan d of the Kenites, Kenizites, Kadmonites; the Chitties, Perizites, Refaim; the Emorites, Canaanites, Gigashites and Yevusites.† The main purpose for the book of Joshua is the completion of the promise God made in Genesis 12-50 (Attridge, Harold W., 2006, P.310). To start off the process of the Israelites attaining the profiled promise of God they cross the Jordan river with Joshua, the rest of the book is set in a desert region as they journey to the land of Canaan (Joshua 1:2). As far as the social setting of this book the way they greetShow MoreRelatedThe Roman Road And The Romans Road1590 Words   |  7 PagesThe Roman Road Summary of Method -The intellectual method of evangelism the Romans Road uses a systematic way to explain salvation through Bible verses from the book of Romans (What Is Romans Road). The Romans Road method of evangelism is used by many evangelists and missionaries to share the good news of salvation. The Romans Road approach makes it easy to map out the road to salvation. Although there are different versions of the Romans Road the message of salvation remains the same. The RomansRead MoreJournal Article Critique Of John G Pauline Cosmic Christology And Ecological Crisis Essay1103 Words   |  5 Pages466-479. Submitted to Dr. Michael Chiavone, in partial fulfillment of the requirements for the completion of THEO 510-D01 Survey of Theology by Todd Bush November 6, 2016 Contents Introduction†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦...†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦...3 Brief Summary†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦...†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦.†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦.3 Critical Interaction†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦...†¦Ã¢â‚¬ ¦4 Conclusion†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦...5 Selected Bibliography†¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦7 Introduction The redemptive doors thatRead MoreThe Eucharist Of The Catholic Church883 Words   |  4 Pageslife.† Basically the Eucharist is the sum and summary of faith, â€Å"Our way of thinking is attuned to the Eucharist, and the Eucharist in turn confirms our way of thinking.† Section two titled What is This Sacrament Called? They call it the Eucharist because it is the action of thanksgiving to God. There are different names they call this, The Lords Supper, The memorial of the Lord’s Passion and Resurrection, Holy Communion and Holy Mass. The Lords Supper was the final meal that Jesus had on theRead MoreOld Testament Book Summaries Essay861 Words   |  4 PagesCheryl Welch L24623773 Bible 104 D67 November 15, 2011 Summary of the books of the Old Testament Books Leviticus The genre of this book is law and it was written by Moses, although it is believed that Joshua reported on his death. The key themes include God’s covenant with Israel, instructions on the early Israelite religion, instructions on the sacrificial system, holiness, cleanliness and the priesthood. God had intervened and delivered the people from slavery and was now establishingRead MoreMethods of Evangelism1018 Words   |  5 PagesSummary of Method This method is to use love, compassion, and service to reach people. We have to remember to always have a smile on our face and do this with a generous heart. Meaning that we want to the work of a servant, just as Jesus set an example by washing the disciple’s feet (John 13:1-17). Jesus wants to show that no one is above doing a servant’s work. I also see motivation of servant evangelism in Mathew 25. Jesus is telling his deciples to feed the hungry, give the homelessRead MoreAdvantages And Disadvantages Of The Romans Road1517 Words   |  7 PagesSummary of Method – The Romans Road is an evangelical intellectual method of sharing the gospel, using the approach of laying out the plan of salvation through verses from the book of Romans itself. Verses are fashioned into a teaching which outlines who is in need of salvation, why man needs salvation, how God provides that salvation, a response to salvation, and man’s own response to God’s sal vation. Advantages of Using This Method – One advantage to The Romans Road method, is that the processRead MoreThe Apostle Paul960 Words   |  4 Pageswith James, the Lord’s brother. It was from Peter that Paul learned of the tradition, i.e., the details of Jesus’ teachings during His earthly ministry. It was important for Paul to inquire about the teachings that the disciples had received from the Lord during his time on the earth. Paul was especially mindful to meet with the same two individuals who had seen Jesus after the resurrection, namely, Peter and James. The elements of the gospel which Paul learned from the disciples (tradition) areRead MoreSummary Of The Anchor Bible 1373 Words   |  6 Pagesare to be saved?† Jesus answers to them in verse 24, â€Å"Strive to enter through the narrow door, for many, I tell you, will seek to get in, but will not be able to.† Luke carries on to the second part of his account with Jesus’ statements about salvation and reception or non-reception into the kingdom (Luke 13:22-30) these statements give an outlook for the whole second part which are closely linked with the two final parables which ended the first part. Both deal with accounts of the kingdom ofRead MoreMormonism: Exploring the Beliefs of Mormons and Christians Essay750 Words   |  3 PagesMormons worldwide, there are approximately 6 million Mormons in the United States. Mormonism is â€Å"the fastest and most successful cult in the history of the United States†¦an average (increasing) rate of 300,000 converts a year† (Ridenour 130). Analysis/Summary of Topic First of all, we must explore the origin of Mormonism. In 1820, a 14 year old boy named, Joseph Smith, Jr., had a vision of what he thought was the Father and the Son. The boy asked them what Christian denomination he should be, and theyRead MoreThe Hermits1206 Words   |  5 Pagestaller, also old, in a torn coat, but he is a powerful man. And the third is tall, eyebrows hanging over his eyes. The bishop goes to the island and saw the hermits. He says there they seek salvation in the island, praying for people to Christ the Lord. He told them that it is not the right to way to pray to the Lord, the Bishop did not leave the hermits until he had taught them the whole of the Lords Prayer. The Bishop took leave of the hermits, back to the ship and sailed out. The bishop can’t sleep

Time Management At The Workplace - 1675 Words

Time Management at the Workplace and The Importance of Being on Time Hunter J. Bullock 4th Ranger Training Battalion Time Management at the Workplace and The Importance of Being on Time â€Å"The average person uses 13 different methods to control and manage their time.† Wetmore, D. E. (1999, August 23). Time Management Facts and Figures. Retrieved from http://www.balancetime.com/articles/tm_facts_and_figures.htm It is imperative to arrive on time to anything and everything that has been pre-planned. If everyone was to show up late to their appointments, jobs, or social events it would cause complete disorganization and extreme stress. Having excellent Time Management skills could help you excel greatly in your everyday life. Time†¦show more content†¦It creates the ability to get more things done even when time is tight. â€Å"Ways to practice Time Management skills include many things such as carrying a schedule and recording all of your activities, scheduling time for interruptions or distractions and taking at least 30 minutes every morning to plan your day.† Mathews, J. (2016). How to Manage time with 10 tips that Work. Retrieved from https://www.entrepreneur.com/article/219553 Possessing great Time Management skills can reduce stress and increase confidence. â€Å"If an individual lacks Productive Time Management skills, he/she will obtain a poor professional reputation, missed deadlines, inefficient work flow, higher stress levels, and have poor work quality. There are many mistakes you can make while practicing Time management such as failing to keep a to-do list, not stopping and taking breaks during the day, procrastination and failing to manage distractions. When keeping a to -do list, you must first prioritize the material on it. Make sure the important things are finished first. If you fail to stop and take breaks, you can’t and won’t produce the highest quality of work. Taking a 5-10-minute break every hour or two shouldn’t be notified as â€Å"wasting time†. Procrastination is something every person does. One useful strategy is to tell yourself that you’re only going to start on a project for ten minutes. When you fail to manage distractions, the minutes you spend on

My favourite game free essay sample

A star is a massive, luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun, which is the source of most of the planets energy. Some other stars are visible from Earth during the night, appearing as a multitude of fixed luminous points due to their immense distance. Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of stars have been assembled by astronomers, which provide standardized star designations. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the stars interior and then radiates into outer space. Once the hydrogen in the core of a star is nearly exhausted, almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the stars lifetime and, for some stars, by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, luminosity, and spectrum respectively. The total mass of a star is the principal determinant of its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the stars environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities, known as a Hertzsprung–Russell diagram (H–R diagram), allows the age and evolutionary state of a star to be determined. A stars life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. Once the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process. [1] The remainder of the stars interior carries energy away from the core through a combination of radiative and convective processes. The stars internal pressure prevents it from collapsing further under its own gravity. Once the hydrogen fuel at the core is exhausted, a star with at least 0.4 times the mass of the Sun[2] expands to become a red giant, in some cases fusing heavier elements at the core or in shells around the core. The star then evolves into a degenerate form, recycling a portion of its matter into the interstellar environment, where it will contribute to the formation of a new generation of stars with a higher proportion of heavy elements. [3] Meanw hile, the core becomes a stellar remnant: a white dwarf, a neutron star, or (if it is sufficiently massive) a black hole. Binary and multi-star systems consist of two or more stars that are gravitationally bound, and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution. [4] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy. Distribution A white dwarf star in orbit around Sirius (artists impression). NASA image In addition to isolated stars, a multi-star system can consist of two or more gravitationally bound stars that orbit each other. The simplest and most common multi-star system is a binary star, but systems of three or more stars are also found. For reasons of orbital stability, such multi-star systems are often organized into hierarchical sets of binary stars. [77] Larger groups called star clusters also exist. These range from loose stellar associations with only a few stars, up to enormous globular clusters with hundreds of thousands of stars. It has been a long-held assumption that the majority of stars occur in gravitationally bound, multiple-star systems. This is particularly true for very massive O and B class stars, where 80% of the stars are believed to be part of multiple-star systems. However the proportion of single star systems increases for smaller stars, so that only 25% of red dwarfs are known to have stellar companions. As 85% of all stars are red dwarfs, most stars in the Milky Way are likely single from birth. [78] Stars are not spread uniformly across the universe, but are normally grouped into galaxies along with interstellar gas and dust. A typical galaxy contains hundreds of billions of stars, and there are more than 100 billion (1011) galaxies in the observable universe. [79] A 2010 star count estimate was 300 sextillion (3 ?1023) in the observable universe. [80] While it is often believed that stars only exist within galaxies, intergalactic stars have been discovered. [81] The nearest star to the Earth, apart from the Sun, is Proxima Centauri, which is 39. 9 trillion kilometres, or 4. 2 light-years away. Travelling at the orbital speed of the Space Shuttle (8 kilometres per second—almost 30,000 kilometres per hour), it would take about 150,000 years to get there. [82] Distances like this are typical inside galactic discs, including in the vicinity of the solar system. Stars can be much closer to each other in the centres of galaxies and in globular clusters, or much farther apart in galactic halos. Due to the relatively vast distances between stars outside the galactic nucleus, collisions between stars are thought to be rare. In denser regions such as the core of globular clusters or the galactic center, collisions can be more common. [84] Such collisions can produce what are known as blue stragglers. These abnormal stars have a higher surface temperature than the other main sequence stars with the same luminosity in the cluster. [85] Characteristics OBESERVATION HISTORY Historically, stars have been important to civilizations throughout the world. They have been part of religious practices and used for celestial navigation and orientation. Many ancient astronomers believed that stars were permanently affixed to a heavenly sphere, and that they were immutable. By convention, astronomers grouped stars into constellations and used them to track the motions of the planets and the inferred position of the Sun. [5] The motion of the Sun against the background stars (and the horizon) was used to create calendars, which could be used to regulate agricultural practices. The Gregorian calendar, currently used nearly everywhere in the world, is a solar calendar based on the angle of the Earths rotational axis relative to its local star, the Sun. The oldest accurately dated star chart appeared in ancient Egyptian astronomy in 1534 BC. [8] The earliest known star catalogues were compiled by the ancient Babylonian astronomers of Mesopotamia in the late 2nd millennium BC, during the Kassite Period (ca. 1531–1155 BC). [9] The first star catalogue in Greek astronomy was created by Aristillus in approximately 300 BC, with the help of Timocharis. The star catalog of Hipparchus (2nd century BC) included 1020 stars and was used to assemble Ptolemys star catalogue. [11] Hipparchus is known for the discovery of the first recorded nova (new star). [12] Many of the constellations and star names in use today derive from Greek astronomy. In spite of the apparent immutability of the heavens, Chinese astronomers were aware that new stars could appear. [13] In 185 AD, they were the first to observe and write about a supernova, now known as the SN 185. The brightest stellar event in recorded history was the SN 1006 supernova, which was observed in 1006 and written about by the Egyptian astronomer Ali ibn Ridwan and several Chinese astronomers. [15] The SN 1054 supernova, which gave birth to the Crab Nebula, was also observed by Chinese and Islamic astronomers. [16][17][18] Medieval Islamic astronomers gave Arabic names to many stars that are still used today, and they invented numerous astronomical instruments that could compute the positions of the stars. They built the first large observatory research institutes, mainly for the purpose of producing Zij star catalogues. Among these, the Book of Fixed Stars (964) was written by the Persian astronomer Abd al-Rahman al-Sufi, who observed a number of stars, star clusters (including the Omicron Velorum and Brocchis Clusters) and galaxies (including the Andromeda Galaxy). [20] According to A. Zahoor, in the 11th century, the Persian polymath scholar Abu Rayhan Biruni described the Milky Way galaxy as a multitude of fragments having the properties of nebulous stars, and also gave the latitudes of various stars during a lunar eclipse in 1019. According to Josep Puig, the Andalusian astronomer Ibn Bajjah proposed that the Milky Way was made up of many stars which almost touched one another and appeared to be a continuous image due to the effect of refraction from sublunary material, citing his observation of the conjunction of Jupiter and Mars on 500 AH (1106/1107 AD) as evidence. [22] Early European astronomers such as Tycho Brahe identified new stars in the night sky (later termed novae), suggesting that the heavens were not immutable. In 1584 Giordano Bruno suggested that the stars were like the Sun, and may have other planets, possibly even Earth-like, in orbit around them,[23] an idea that had been suggested earlier by the ancient Greek philosophers, Democritus and Epicurus,[24] and by medieval Islamic cosmologists[25] such as Fakhr al-Din al-Razi. [26] By the following century, the idea of the stars being the same as the Sun was reaching a consensus among astronomers. To explain why these stars exerted no net gravitational pull on the Solar System, Isaac Newton suggested that the stars were equally distributed in every direction, an idea prompted by the theologian Richard Bentley. [27] The Italian astronomer Geminiano Montanari recorded observing variations in luminosity of the star Algol in 1667. Edmond Halley published the first measurements of the proper motion of a pair of nearby fixed stars, demonstrating that they had changed positions from the time of the ancient Greek astronomers Ptolemy and Hipparchus. [23] William Herschel was the first astronomer to attempt to determine the distribution of stars in the sky. During the 1780s, he performed a series of gauges in 600 directions, and counted the stars observed along each line of sight. From this he deduced that the number of stars steadily increased toward one side of the sky, in the direction of the Milky Way core. His son John Herschel repeated this study in the southern hemisphere and found a corresponding increase in the same direction. [28] In addition to his other accomplishments, William Herschel is also noted for his discovery that some stars do not merely lie along the same line of sight, but are also physical companions that form binary star systems. The science of stellar spectroscopy was pioneered by Joseph von Fraunhofer and Angelo Secchi. By comparing the spectra of stars such as Sirius to the Sun, they found differences in the strength and number of their absorption lines—the dark lines in a stellar spectra due to the absorption of specific frequencies by the atmosphere. In 1865 Secchi began classifying stars into spectral types. [29] However, the modern version of the stellar classification scheme was developed by Annie J. Cannon during the 1900s. Alpha Centauri A and B over limb of Saturn The first direct measurement of the distance to a star (61 Cygni at 11. 4 light-years) was made in 1838 by Friedrich Bessel using the parallax technique. Parallax measurements demonstrated the vast separation of the stars in the heavens. [23] Observation of double stars gained increasing importance during the 19th century. In 1834, Friedrich Bessel observed changes in the proper motion of the star Sirius, and inferred a hidden companion. Edward Pickering discovered the first spectroscopic binary in 1899 when he observed the periodic splitting of the spectral lines of the star Mizar in a 104-day period. Detailed observations of many binary star systems were collected by astronomers such as William Struve and S. W. Burnham, allowing the masses of stars to be determined from computation of  the orbital elements. The first solution to the problem of deriving an orbit of binary stars from telescope observations was made by Felix Savary in 1827. [30] The twentieth century saw increasingly rapid advances in the scientific study of stars. The photograph became a valuable astronomical tool. Karl Schwarzschild discovered that the color of a s tar, and hence its temperature, could be determined by comparing the visual magnitude against the photographic magnitude. The development of the photoelectric photometer allowed very precise measurements of magnitude at multiple wavelength intervals. In 1921 Albert A. Michelson made the first measurements of a stellar diameter using an interferometer on the Hooker telescope. [31] Important theoretical work on the physical structure of stars occurred during the first decades of the twentieth century. In 1913, the Hertzsprung-Russell diagram was developed, propelling the astrophysical study of stars. Successful models were developed to explain the interiors of stars and stellar evolution. Cecilia Payne-Gaposchkin first proposed that stars were made primarily of hydrogen and helium in her 1925 PhD thesis. The spectra of stars were further understood through advances in quantum physics. This allowed the chemical composition of the stellar atmosphere to be determined. [33] With the exception of supernovae, individual stars have primarily been observed in our Local Group of galaxies,[34] and especially in the visible part of the Milky Way (as demonstrated by the detailed star catalogues available for our galaxy). [35] But some stars have been observed in the M100 galaxy of the Virgo Cluster, about 100 million light years from the Earth.