Difference between revisions of "Part:BBa K1893010"

Revision as of 16:27, 29 October 2016

Constitutive STAR (J23119+STAR)

This is the STAR construct under control of the constitutive promoter j23119. When transcribed, it produces the STAR-antisense RNA (pAD1.A5), which can bind to the sense STAR-target attenuator sequence (pAD1.S5). Thus, only in the presence of STAR-antisense, transcription and expression of coding sequences downstream to the STAR-target is activated.

Usage and Biology

For designing a small transcriptional activating RNA through an anti-terminator mechanism, Chappell et. al. investigated transcriptional terminators from different plasmids and of different lengths and sequences. Of these, the sense pAD1 plasmid attenuator sequence no. 5 (pAD1.S5) and its associated STAR-antisense sequence no. 5 (pAD1.A5) pair gave the highest (94-fold) activation of the reporter gene, SFGFP [Chappell et al., 2015]. Thus, we used the pAD1.S5 sequence as our STAR target-encoding DNA and the pAD1.A5 sequence as the STAR-antisense-encoding DNA.

STAR binds a sense target RNA sequence, the pAD1 plasmid attenuator sequence, which is fused upstream of the gene of interest. In the absence of STAR, the pAD1 plasmid attenuator sequence forms an intrinsic hairpin structure, preventing RNA polymerase from transcribing the gene and thus acting as a terminator of transcription. However, when STAR is produced, it binds to the target sequence and interferes with the hairpin formation, allowing transcription of the downstream gene.

Characterisation

We generated a two-plasmid system for characterisation experiments. The first plasmid contains the STAR sequence downstream of a constitutive Anderson promoter and followed by the t500 transcriptional terminator on a high-copy plasmid. The second plasmid is a reporter plasmid that contains the superfolder GFP (SFGFP) gene with a ribosome binding site immediately downstream of the STAR-target (pAD1 plasmid attenuator) sequence. The SFGFP coding sequence is under the control of a constitutive Anderson promoter and also has its own TrrnB terminator.

We characterised STAR activity at 30 and 37 degrees Celsius by using a plate reader to record the fluorescence of SFGFP over 200 minutes in cells with both plasmids, as well as in cells with just the reporter plasmid to determine to what degree STAR was able to activate SFGFP transcription.

Initially, we characterised the STAR system in terms of fold activation of GFP expression from the reporter plasmid in the absence and presence of STAR molecules. For this experiment, Top 10 E. coli cell lines were co-transformed with either the reporter plasmid and a plasmid with the J23119 promoter (no STAR) or with the reporter plasmid and the J23119-STAR plasmid. Cell cultures of these two cell lines were grown in microplates and well fluorescence was monitored over time using a microplate reader. The fluorescence signal from each well was normalised by dividing with the O.D. 600 value of that well. This gave the normalised fluorescence value for that cell line (FI/Abs). To account for cell autofluorescence, DH10B cells (similar to Top10) were used to determine background normalised fluorescence value.

Next, an experiment was carried out to investigate STAR system functionality at different temperatures. RNA elements functionality can be strongly depended on temperature and thermodynamics. In the case that we needed to use the STAR system under different circumstances (co-culture with B. subtilis that grows better at 30 degrees Celcius) we characterised the STAR system at 30 degrees Celsius cell culture condition. Cell cultures of the previously mentioned cell lines were grown for 5 hours in exponential phase. Then, the cell cultures were normalised at O.D. 600 = 0.4 and the fluorescent signal for each condition was recorded.

Figure 1: Characterisation of STAR system in TOP10 E. coli cells. (A) Normalised fluorescence monitored over time for cell lines incorporating the STAR system in the absence or presence of transcribed STAR molecules (B) Normalised endpoint fluorescence (100 minutes) for cell lines in the absence or presence of STAR molecules. We used the two-plasmid system described in the Experimental Design for characterisation experiments involving STAR. For the absence of STAR condition, the plasmid did not include STAR sequence but just the J23119 promoter. Normalised fluorescence was calculated by dividing fluorescent signal by the O.D.600 value of the culture. Background was determined by the use of DH10B cells with no plasmid transformed. Error bars represent standard deviation from 3 technical repeats.

Figure 2: Characterisation of STAR system in TOP10 E. coli cells at different temperatures. (A) Cell culture fluorescence at 30°C (B) Cell culture fluorescence assay at 37°C. (C) Fold activation SFGFP expression in presence of STAR. We used the two-plasmid system described in the Experimental Design for characterisation experiments involving STAR. For the absence of STAR condition, the plasmid did not include STAR sequence but just the J23119 promoter. The autofluorescence background control used is E. coli Top 10 cells with no reporter plasmid. Error bars represent standard deviation from 3 technical repeats.

Sequence and Features