• Parasites, Hosts and Diseases
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• 제36권1호
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• pp.23-32
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• 1998

마우스 백혈병 바이러스인 LP-BM5 MuLV를 감염시켜 면역결핍 상태 (Murine AIDS: MfdDS)로 유도한 C57BL/6 마우스에 10 종류의 가시아메바 분리주를 감염시켜 가시아메바 분리 주별 병원성을 평가하였다. LP-BM5 MuLV에 감염된 C57BL/6 마우스는 MfdDS 모델의 특징적 소견인 비장 종대와 임파절 종대를 나타내었고, 가시아메바의 배양 온도에 따른 MAIDS 모델 마 우스의 치사율의 유의적 차이는 없었으나. 분리주에 따른 MAIDS 마우스의 치사율은 상당한 차이 가 있었다. 아메바성 육아종성 뇌염 환자의 뇌에서 분리한 A. henlvioc-3A주가 가장 높은 치사 율을 나타내었고. 조직 배양 중 분리된 A. culbensonih-1주가 2번째로 높은 치사율을 나타내었 다. 국내 토양에서 분리한 A. ccstellanii KA/S2주와 A.polvphagaga KAS3주는 매우 낮은 치사율 을 보였다. 가시아메바를 비강 내 접종으로 감염시킨 마우스는 정맥 내 주사로 감염시킨 마우스에 비해 만성적 경과를 보였다. 사망한 마우스의 폐와 뇌의 육안적 병리 소견은 일관된 성적을 나타 내지는 않았고. 마우스 개체마다 다양하였다 병리 조직학적 소견으로는 뇌 조직에서보다 폐 조직 에서 더 심한 염증과 괴사를 보였으나. OC-3A주로 감염시켜 사망한 마우스의 뇌조직에서는 심한 염증반응과 가시아메바 영양형을 관찰할 수 있었다. 가시아메바 분리주마다 병원성이 다른 것으로 미루어 보아 가시아메바의 병원성은 유전적 요인에 의해 결정될 것으로 생각되며 추후 가시아메바 병원성 결정인자에 대한 연구가 필요하다고 사료된다.

• 한국자원식물학회:학술대회논문집
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• 한국자원식물학회 2019년도 춘계학술대회
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• pp.32-32
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• 2019

Mutation breeding is the useful tool to improve agronomic traits in various crop species. Soybean is most important crop and is rich in protein and oil contents. Despite of the importance as economic value and various genetic resource of soybean, there have been limited studies of genetic relationship among mutant resources through radiation breeding. In this study, the agronomical phenotype for selecting various genetic resources was evaluated in 528 soybean mutant lines. As a result, 210 soybean mutants with their original cultivars were selected with various traits. We named 210 selected lines as Mutant Diversity Pool (MDP). The genetic diversity and the relationship of the MDP were investigated using TRAP and TE-TRAP markers. In TRAP analysis, sixteen primer combination (PC)s were used and a total of 551 fragments were amplified. The highest (84.00%) and the lowest (32.35%) polymorphism levels were showed in PC MIR157B+Ga5 and B14G14B+Ga3, respectively. The mean of PIC values was 0.15 ranging from 0.07 in B14G14B+Sa12 to 0.23 in MIR157B+Sa4. Phylogenetic and population structure analysis indicated that the 210 MDP lines dispersed to four groups among the wild types and their mutants. The highest genetic diversity among populations was observed between lines Paldal and 523-7 (Fst=0.409), whereas the lowest genetic diversity was between population KAS360-22 and 94seori (Fst=0.065). AMOVA showed 11.583 (21.0%) and 43.532 (79.0%) variations in inter and intra mutant population, respectively. Overall, the genetic similarity of each intra mutant populations was closer than that of inter mutant population. A total of 408 fragments were amplified in the 210 MDP using twelve PCs of TE-TRAP markers that were obtained from a combination of three TIR sequence of transposable elements (MITE-stowaway; M-s, MITE-tourist; M-t, PONG). The highest (77.42%) and the lowest (56.00%) polymorphism levels were showed in PONG+Sa4 and PONG+Sa12, respectively. The mean of PIC values was 0.15 ranging from 0.09 in M-s+Sa4 and M-s+Ga5 to 0.21 in M-t+Ga5. AMOVA of M-s showed 2.209 (20%) and 8.957 (80%) variations in inter and intra mutant population, respectively. AMOVA of M-t showed 2.766 (18%) and 12.385 (82%) variations in inter and intra mutant population, respectively. AMOVA of PONG showed 3.151 (29%) and 7.646 (71%) variations in inter and intra mutant population, respectively. According to our study, the PONG had higher inter mutant population and lower intra mutant population. This mean was that for aspect of radiation sensitivity, M-s and M-t showed higher mobility than that of PONG. Our results suggest that the TRAP and the TE-TRAP markers may be useful for assessing the genetic diversity and relationship among soybean MDP and help to improve our knowledge of soybean mutation/radiation breeding.

• 천문학회보
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• 제46권2호
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• pp.58.1-59
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• 2021

Exploration of asteroids' internal structure is essential for understanding their evolutional history. It also provides a fundamental information about the history of coalescence and collision of the solar system. Among several models of the internal structures, the rubble-pile model, confirmed by the near-Earth asteroid (25143) Itokawa by Hayabusa mission [1], is now widely regarded as the most common to asteroids with size ranging from 200 m to 10 km [2]. On the contrary, monolithic and core-mantle structures are also possible for small asteroids [3]. It is, however, still challenging to look through the interior of a target object using remote-sensing devices. In this presentation, we introduce our ongoing research conducted at Seoul National and propose an idea to infer the internal structure of Apophis using available instruments. Itokawa's research provides an important benchmark for Apophis exploration because both asteroids have similar size and composition [4][5]. We have conducted research on Itokawa's evolution in terms of collision and space weathering. Space weathering is the surface alteration process caused by solar wind implantation and micrometeorite bombardment [6]. Meanwhile, resurfacing via a collision acts as a counter-process of space weathering by exposing fresh materials under the matured layer and lower the overall degree of space weathering. Therefore, the balance of these two processes determine the space weathering degrees of the asteroid. We focus on the impact evidence on the boulder surface and found that space weathering progresses in only 100-10,000 years and modifies the surface optical properties (Jin & Ishiguro, KAS 2020 Fall Meeting). It is important to note that the timescale is significantly shorter than the Itokawa's age, suggesting that the asteroid can be totally processed by space weathering. Accordingly, our result triggers a further discussion about why Itokawa indicates a moderately fresh spectrum (Sq-type denotes less matured than S-type). For example, Itokawa's smooth terrains show a weaker degree of space weathering than other S-type asteroids [7]. We conjecture that the global seismic shaking caused by collisions with >1 mm-sized interplanetary dust particles induces granular convection, which hinders the progression of space weathering [8]. Note that the efficiency of seismic wave propagation is strongly dependent on the internal structure of the asteroid. Finally, we consider possible approaches to investigate Apophis's internal structure. The first idea is studying the space weathering age, as conducted for Itokawa. If Apophis indicates a younger age, the internal structure would have more voids [9]. In addition, the 2029 close encounter with Earth provides a rare natural opportunity to witness the contrast between before and after the event. If the asteroid exhibits a slight change in shape and space weathering degree, one can determine the physical structure of the internal materials (e.g., rubble-pile monolithic, thick or thin regolith layer, the cohesion of the materials). We will also consider a possible science using a seismometer.

• Journal of Applied Biological Chemistry
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• 제53권2호
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• pp.65-70
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• 2010

중쇄지방산은 탄소수가 8-12개로 구성된 포화지방산으로, 장쇄지방산과 달리 인체내 흡수가 빠르고 분해가 빨리 일어나 체지방으로 축적되지 않으면서 열효율이 높아 소화장애환자의 식이요법에 이용된다. 또한 최근 의료분야의 위장침투향상기술에 중쇄지방산 또는 중쇄지방산 유도물질이 사용되며, 이 기술은 최첨단 약물전달시스템 분야에 매우 중요하게 적용되고 있다. 이처럼 효용가치가 높은 중쇄지방산 기름은 아열대작물인 코코넛, 팜 그리고 쿠페아 종자에서 주로 생산되고 있는데, 기름함량이 적고 재배가 까다로워 상업적 이용의 어려움이 있다. 이러한 이유로 재배지역이 넓고 재배가 용이한 유채의 종자에서 중쇄지방산을 생산하고 함량을 증대시키기 위해 그 동안 많은 연구가 수행되어 왔다. 지금까지 밝혀진 중쇄지방산 생산에 관여하는 유전자는 크게 Thioesterase(지방산 사슬 길이), KAS(지방산 사슬 연장), 그리고 Acyltransferase(지방산 전이)로 알려져 있다. 이러한 유전자를 단독 또는 동시에 유채에 형질전환 한후, 여기에서 얻어진 형질전환체 계통을 이용하여 고전육종과 분자육종의 병행을 통해 유채 종자에서 중쇄지방산인 Laurate함량이 60 mol%까지 축적되는 결과를 얻었다. 또한 Caprylate와 Caprate함량은 각 각 8 mol%와 27 mol%까지 축적되었다. 비록 유채 종자에서 일부 중쇄지방산의 생산이 성공적으로 생산되는 결과를 얻었다 할지라도 실제 상업적으로 이용하려면 중쇄지방산 함량이 더 많이 생산되어야 한다. 본 총설에서는 지금까지 유채 종자 내에서 중쇄지방산이 생산된 연구결과를 면밀히 살펴보았고, 향후 연구방향에 대해 간략하게 논하였다.